เหตุการณ์ใน-นอกโลก VS ภัยธรรมชาติ และupdate พายุสุริยะ

ในห้อง 'ภัยพิบัติและการเตรียมการ' ตั้งกระทู้โดย Falkman, 10 มกราคม 2011.

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หน้า 92 ของ 233
  1. sunny430

    sunny430 เป็นที่รู้จักกันดี

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    ดีใจแทบแย่ครับพี่ falkman
     
    sunny430, 24 มีนาคม 2012

    #1821
  2. somsweet

    somsweet เป็นที่รู้จักกันดี

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    กลับมาพร้อมของแถมเบาๆ..rabbit_cry
     
    somsweet, 24 มีนาคม 2012

    #1822
  3. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

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    STCE Newsletter

    12 Mar 2012 - 18 Mar 2012

    Published by the STCE - this issue : 23 Mar 2012.
    The Solar-Terrestrial Centre of Excellence (STCE) is a collaborative network of the Belgian Institute for Space Aeronomy, the Royal Observatory of Belgium and the Royal Meteorological Institute of Belgium.


    Review of solar activity (12 Mar 2012 - 18 Mar 2012)


    Solar activity was at active levels during the past week with four M-flares observed. The first one, a M7.9, occurred on March 13th at 1741UT (peak time) in NOAA AR 1429, and was associated with a mild proton event observed for >10 and >50 MeV protons. This proton event ended 2 days later (10 MeV protons), on March 15th around 0620 UT. A fast CME (v>1400 Km/s) was associated with this event. The next 2 M flare events: a M2.8 flare peaking at 15:21 UT on March 14th, and a M1.8 flare peaking at 0752UT on March 15th took place in NOAA AR 1432. These two events were associated with slower CMEs (550 and 450 km/s). The last event, a M1.3 flare peaking at 2039UT on March 17th occurred in NOAA AR 1434. No CME was observed.


    Review of geomagnetic activity (12 Mar 2012 - 18 Mar 2012)


    Geomagnetic activity reached minor to major storm conditions at planetary levels on two occasions. On March 12th, a shock was detected by ACE around 0840 UT, which was attributed to the CME observed with the M6.3 flare on March 9th. Major storm conditions (Kp=6) were observed during 6 hours on March 12th between 09 and 15 UT. Active to minor storm conditions were observed locally at Dourbes.
    On March 15th, around 1240 UT, a shock was observed by ACE and associated to the CME accompanying the M7.9 flare of March 13th. Minor to major storm conditions occurred for 9 hours on that day (from 12 to 21 UT) at planetary levels. Minor storm conditions were noticed locally. Unsettled to isolated minor storm conditions were then observed locally (Dourbes) from March 16th to March 18th due a coronal hole at a geoeffective position.


    Noticeable Solar Events (12 Mar 2012 - 18 Mar 2012)


    <table class="notic" style="border-collapse: collapse; -webkit-border-horizontal-spacing: 5px; -webkit-border-vertical-spacing: 5px; border-top-width: 1px; border-right-width: 1px; border-bottom-width: 1px; border-left-width: 1px; border-top-style: solid; border-right-style: solid; border-bottom-style: solid; border-left-style: solid; border-top-color: black; border-right-color: black; border-bottom-color: black; border-left-color: black; border-image: initial; text-align: center; "> </table> <table class="notic" style="border-collapse: collapse; -webkit-border-horizontal-spacing: 5px; -webkit-border-vertical-spacing: 5px; border-top-width: 1px; border-right-width: 1px; border-bottom-width: 1px; border-left-width: 1px; border-top-style: solid; border-right-style: solid; border-bottom-style: solid; border-left-style: solid; border-top-color: black; border-right-color: black; border-bottom-color: black; border-left-color: black; border-image: initial; text-align: center; "> <tbody><tr><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">DAY</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">BEGIN</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">MAX</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">END</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">LOC</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">XRAY</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">OP</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">10CM</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">TYPE</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">Cat</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">NOAA</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">NOTE</td></tr><tr><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">13</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1712</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1741</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1825</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">N17W66</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">M7.9</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">
    </td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">0</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">VI/1</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">65</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1429</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">
    </td></tr><tr><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">14</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1508</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1521</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1536</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">N14E05</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">M2.8</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1N</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">72</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">
    </td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">67</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1432</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">
    </td></tr><tr><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">15</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">0723</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">0752</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">0808</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">N14W03</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">M1.8</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1F</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">0</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">II/1</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">67</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1432</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">
    </td></tr><tr><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">17</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">2032</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">2039</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">2042</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">S20W25</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">M1.3</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">SF</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">54</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">III/2 II/2</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">68</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">1434</td><td style="border-top-width: 1px; border-top-style: solid; border-top-color: black; border-bottom-width: 1px; border-bottom-style: solid; border-bottom-color: black; font-family: monospace; padding-left: 10px; padding-right: 10px; ">
    </td></tr></tbody> </table>
    <table> </table> <table> <tbody><tr><td>LOC: approximate heliographic location</td><td>TYPE: radio burst type</td></tr><tr><td>XRAY: X-ray flare class</td><td>Cat: Catania sunspot group number</td></tr><tr><td>OP: optical flare class</td><td>NOAA: NOAA active region number</td></tr><tr><td>10CM: peak 10 cm radio flux</td></tr></tbody> </table>

    Geomagnetic Observations at Dourbes (12 Mar 2012 - 18 Mar 2012)


    <center style="color: rgb(34, 34, 34); font-family: Verdana, Arial, sans-serif; font-size: 13px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; background-color: rgb(255, 255, 255); ">[​IMG]</center>

    PROBA2 Observations (12 Mar 2012 - 18 Mar 2012)


    Solar activity fluctuated between LOW and MODERATE.


    4 M-flares were detected on-board PROBA2.


    Hereunder are presented the SWAP images and LYRA curves related to the 3 most energetic flares of this week, i.e.
    *M7.9 from Tue 13th Mar (AR 11429)
    *M2.8 from Wed 14th Mar (AR 11432)
    *M1.8 from Thu 15th Mar (AR 11432)


    The following curves are visible on the LYRA time series:
    *black: Zirconium Channel LYRA Unit 2
    *blue: Aluminium Channel of LYRA Unit 2
    *purple: SWAVINT (solar intensity derived from integrated SWAP images)


    M7.9 Flare on Tue March 13; 17:12 (west limb) - from AR 11429


    <center style="color: rgb(34, 34, 34); font-family: Verdana, Arial, sans-serif; font-size: 13px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; background-color: rgb(255, 255, 255); ">[​IMG]</center>
    <center style="color: rgb(34, 34, 34); font-family: Verdana, Arial, sans-serif; font-size: 13px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; background-color: rgb(255, 255, 255); ">[​IMG]</center>
    M2.8 Flare on Wed March 14; 15:08 (just left of meridian) - from AR 11432

    <center style="color: rgb(34, 34, 34); font-family: Verdana, Arial, sans-serif; font-size: 13px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; background-color: rgb(255, 255, 255); ">[​IMG]</center>
    LYRA was in calibration mode during the occurrence of this flare.

    M1.8 Flare on Thu March 15; 07:52 (just right of meridian) - from AR 11432


    <center style="color: rgb(34, 34, 34); font-family: Verdana, Arial, sans-serif; font-size: 13px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; background-color: rgb(255, 255, 255); ">[​IMG]</center>
    <center style="color: rgb(34, 34, 34); font-family: Verdana, Arial, sans-serif; font-size: 13px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; background-color: rgb(255, 255, 255); ">[​IMG]</center>
    Before AR 11429 turned behind the western limb, it exhibited several filament/prominence eruptions on Tuesday 13th and Wednesday 14th.

    Future Events


    For more details, see Future Events | European Space Weather Portal


    Spectroscopy of the Dynamic Sun

    Start : 2012-04-18 - End : 2012-04-20
    We are hosting a conference celebrating the careers of Prof. George Doschek from NRL and Prof. Tetsuya Watanabe from NAOJ focussing on the topic of Spectroscopy of the Dynamic Sun.
    George Doschek has played a major part in space solar spectroscopy for many decades. Following a key role in exploiting Skylab data, he made huge contributions to the design and build of instruments on board the P78-1, Yohkoh and Hinode missions, being US PI for the Hinode EIS. His knowledge of spectroscopy is recognized and respected internationally and he has published very many papers on high temperature solar plasmas.
    Tetsuya Watanabe is a leading spectroscopist in Japan. Following work with stellar atmospheres, he has been involved from the start of Japanese space solar physics with significant roles in the Bragg spectrometers the Tansei 4, Hinotori and Yohkoh missions. He is Japanese PI for Hinode EIS. He has published extensively on solar X-ray and EUV spectra.
    This conference will focus on recent results using spectroscopy to probe fundamental questions in solar physics.
    Website:
    http://msslxr.mssl.ucl.ac.uk:8080/SolarB/spectrosun/index.jsp


    EGU General Assembly in Vienna, Austria

    Start : 2012-04-22 - End : 2012-04-27
    The EGU General Assembly 2012 will bring together geoscientists from all over the world into one meeting covering all disciplines of the Earth, Planetary and Space Sciences. Especially for young scientists the EGU appeals to provide a forum to present their work and discuss their ideas with experts in all fields of geosciences. The EGU is looking forward to cordially welcome you in Vienna.
    Space weather related sessions:
    Impact of solar and geomagnetic variabilities on the Earth's lower,middle and upper atmospheres (Thierry Dudok de Wit, Jean Lilensten, F.-J. Lübken, M. Kaufmann and P. Preusse)
    This interdisciplinary session focuses on the multiple impacts of solar activity on climate variability. The session will address both forcing mechanisms such as solar spectral irradiance, geomagnetic perturbations and galactic cosmic rays, and the response of the upper, middle and lower atmosphere. Special attention will be payed to the solar flares and geomagnetic storms as well as to the role of the long-term trends of the solar activity, in particular, in global climate changes and modern global warming. Papers involving the physical processes in the ionosphere and stratosphere will be welcome in the first place. The objective is to go beyond correlation analyses and gain a better quantitative understanding of the different contributions of solar variability to the terrestrial environment.
    More information:
    CO Meeting Organizer EGU2012
    Space Weather and its Effects on Terrestrial and Geo -Space Environments: Science and Applications (Viviane Pierrard (BIRA-IASB, Belgium), Hanna Rothkaehl (Space Research Centre PAS, Poland), Norma Crosby (BIRA-IASB, Belgium)
    This session gathers together scientists with expertise in various fields of solar-terrestrial physics that deal with the effects of space phenomena on different levels of geo -space. Effects range from those observed on spacecraft related activities all the way down to Earth, including technological systems, human health and the Earth's climate. We welcome contributions (theoretical and observational) as well as applied (effects on terrestrial and geo -space environments), on all aspects of space weather . Contributions related to the ESA Space Situational Awareness (SSA) programme, or the EU FP7 programme, are very welcome. We look forward to a dynamic and interdisciplinary session.
    Website:
    EGU2012 - Home


    NOAA Space Weather Workshop in Boulder (USA)

    Start : 2012-04-24 - End : 2012-04-27
    Space Weather Workshop is an annual conference that brings industry, academia, and government agencies together in a lively dialog about space weather . What began in 1996 as a conference for the space weather user community, Space Weather Workshop has evolved into the Nation’s leading conference on all issues relating to space weather .
    The conference addresses the remarkably diverse impacts of space weather on today’s technology. The program highlights space weather impacts in several areas, including communications, navigations, spacecraft operations, aviation, and electric power. The presentations and discussions at the Space Weather Workshop also focus on identifying the highest priority needs for operational services that can guide future research and identifying new high-value capabilities that can be transitioned into operations. The conference fosters communication among researchers, space weather service providers, and users of space weather services.
    Researchers have the opportunity to discuss relevant research in many areas of the space environment. Recent progress in large-scale modeling efforts will be featured; while new developments in Sun-to-Earth coupled modeling systems will also be a highlight.
    Website:
    Space Weather Prediction Center


    26th NSO Workshop: 'Solar Origins of Space Weather and Space Climate: Connecting the Interior to the Corona'

    Start : 2012-04-30 - End : 2012-05-04
    As the impact of space weather and climate on daily life is becoming more important, it is timely to discuss the latest reseach on the solar origin of these phenomena. Recent advances in helioseismology have demonstrated that subsurface dynamics are closely associated with aspects of solar activity from the long-term timing of the solar cycle to the short-term eruption of solar flares. The advent of synoptic vector magnetic field measurements is opening up a new path for research on active regions, flares and CME 's. Coronal magnetic field measurements should become available in the next 5-10 years, supplying another physical constrain on space weather events.
    Website:
    NSO Workshop #26 Reroute | NSO


    Advances on space radiation and plasma environment monitoring, data analysis and flight opportunities workshop in Noordwijk, NL

    Start : 2012-05-09 - End : 2012-05-11
    The workshop on 'Advances on Space Radiation and Plasma Environment Monitoring, Data Analysis Methods and Flight Opportunities Workshop' is the forth of a series of workshops proposed under the auspices of the Space Environments and Effects Network of Technical Competences established to further cooperation in Europe.
    The number of flying or ready to fly European radiation and plasma instruments has increased significantly since the last SEENoTC workshop on the subject in 2008 and a round-table at CNES in 2009. Research programmes have also made good progresses in investigating innovative technologies and new concepts designs which will allow a substantial reduction of mass, power and data rate budgets compared to traditional instrumentation, whilst providing equivalent or higher detection efficiency. With many future missions in Navigation, Telecommunications, Exploration, Science, GMES domains flying in severe radiation environments and carrying highly sensitive components and systems, the need for such radiation instrumentation is increasing. Accurate measurements of the Space Environment plays also a crucial role in improvement of radiation enviroment models and the development of the space weather services required by the Space Situational Awareness programme.
    The intention of this workshop is to provide a venue for discussing the latest developments on space plasma and radiation environments and effects instrumentation, to examine possible flight opportunities for such instruments, and to establish the necessary technical and management steps necessary to ensure collaboration on future data analyses, databases, data sharing, and lessons learned from flight experience. It will also allow further discussion and capture of explicit experiment needs and further the harmonization of cooperation on instrument development, flight plans and data exploitation.
    Website:
    Home


    Annular solar eclipse

    Start : 2012-05-20 - End : 2012-05-20
    For more information:
    NASA - Google Maps and Solar Eclipse Paths: 2001 - 2020


    HELAS-5: The Modern Era of Helio- and Asteroseismology

    Start : 2012-05-20 - End : 2012-05-25
    Helioseismology and asteroseismology are the only means to investigate the interior of the Sun and stars. They are crucial for understanding the structure and evolution of stars, which produce all chemical elements in the universe heavier than helium, and which host and influence planets which may carry life. Understanding the physics of the Sun's interior is essential for understanding the solar dynamo and consequently for predicting solar magnetic activity, which has a severe impact on the operation of space missions. Understanding the interior of the stars is essential for understanding those astronomical objects that host and influence planets. With the suite of the latest instruments and missions, e.g. BiSON, GONG, SOHO , SDO, Hinode and Picard for solar exploration and MOST, CoRoT, Kepler, BRITE, SONG for stellar and exoplanetary research, the precision on the seismically determined quantities, e.g. flows in the solar interior or the ages and radii of stars will be greatly improved. This will allow creating new knowledge in solar physics and astrophysics and therefore makes the proposed conference particularly timely.
    Website:
    Confdetail383 : European Science Foundation


    Workshop on Coronal Magnetism at Boulder, Colorado (USA)

    Start : 2012-05-21 - End : 2012-05-23
    The purpose of this workshop is to foster the development of tools to interpret current and future measurements of coronal magnetic fields in order to improve our understanding of the Sun and the sources of Space Weather . This is motivated by the anticipated rapid growth over the next decade in our remote sensing capabilities of the coronal plasma . These new capabilities can only be exploited with improvements in our ability to model the polarized radiative transfer through the coronal plasma and by coupling information on the coronal magnetic field and plasma conditions with models extending to the near Earth environment.
    This workshop will include a wide variety of subjects including, but not limited to, instrumentation, the interpretation of polarimetric signals in EUV and UV emission lines, techniques to mitigate the effects of line-of-sight integration effects of the optically thin corona such as tomographic inversions and forward modeling, models of the polarized radiative transfer at radio wavelengths, extrapolation and MHD modeling of coronal magnetic fields, as well as discussions on how to move forward with coupling these inferences of the coronal plasma with models of heliospheric structure and Space Weather prediction.
    Website:
    Coronal Magnetism Workshop 2012


    Heliophysics Summer School in Boulder, Colorado

    Start : 2012-05-31 - End : 2012-06-07
    The 2012 Heliophysics Summer School will focus on the science underlying current and future heliophysical missions, including but not limited to MMS, Themis , RBSP, IRIS, SDO, and Solar Probe Plus. After providing students with broad overviews of the solar atmosphere, the solar wind , the Earth’s magnetosphere , and ionosphere , the course will cover the basic concepts and unanswered questions pertaining to magnetic reconnection, shocks, plasma instabilities, turbulence, and heating, and the manner in which these concepts and questions affect our understanding of phenomena such as substorms, radiation belt and chromospheric dynamics, solar wind turbulence and particle heating, and heliospheric shocks.
    Link:
    Heliophysics || Summer School || About the Program || Overview


    Los Alamos Space Weather Summer School

    Start : 2012-06-04 - End : 2012-07-27
    The Los Alamos National Laboratory established a summer school in 2011 dedicated to space weather , space science and applications. Every year we solicit applications for the Los Alamos Space Weather Summer School. This summer school is sponsored by IGPP (Institute of Geophysics and Planetary Physics) and PADSTE (Principal Associate Directorate for Science, Technology and Engineering), and PADGS (Principal Associate Directorate for Global Security) and has been established to bring together top space science students with internationally recognized researchers at LANL.
    Website:
    Los Alamos: Space Weather Summer School


    First European School on: Fundamental processes in Space Weather in Spineto, Italy

    Start : 2012-06-04 - End : 2012-06-09
    The Space Weather Integrated Forecasting Framework network (Space Weather Integrated Forecasting Framework web page) organizes in June 2012 the “First European School on Fundamental processes in space weather , a challenge in numerical modelingâ€. The School will focus on the theoretical study of Space plasmas, in particular on those systems where a continuous energy injection flow leads to a self-consistent coupling of the large scale, low frequency motions with the small scale, high frequency fluctuations including kinetic effects. Progress in this field heavily relies on numerical simulations that, as a matter of fact, are nowadays more similar to laboratory experiments than to theoretical exercises. This is true in terms of planning efforts in the preparatory phase, of manpower required, of data analysis and cost. The understanding of these processes represents a fundamental step for the future of Space Weather models.
    Website:
    First European School on: Fundamental processes in Space Weather: a challenge in numerical modeling


    Space Weather Effects on Humans: in Space and on Earth in Moscow, Russia

    Start : 2012-06-04 - End : 2012-06-08
    During the last thirty years there has been steady progress in our understanding of the influence that space weather has on the state of human health both in Space and at Earth. This development is mainly based on research conducted on humans onboard space stations and spacecrafts, as well as on ground based observations and experimental studies simulating conditions in space. This interdisciplinary field of research requires a wide exchange of expertise in various topics. Only with a global approach it will be possible to establish a mutual understanding, in regard to defining the current state of this research problem as well as identifying what should be pursued in future research activities.
    Website:
    Space Weather and Humans 2012


    Remote Sensing of the Inner Heliosphere 2011 in Aberystwyth, UK

    Start : 2012-06-06 - End : 2012-06-10
    We announce the 'Second Remote Sensing of the Inner Heliosphere Workshop' to be hosted by Aberystwyth University and held in Aberystwyth, Wales, UK, 06-10 June 2011. The workshop aims to gather experts from the various fields of remote-sensing observations of the inner heliosphere , including white-light, EUV, and radio observation, together with modellers in order to tackle key outstanding science issues, establish closer working relations, and devise the best ways to move the field forward. In addition, the science learned from remote-sensing observations is key to improving our capabilities of space weather forecasting. The workshop also aims to look at ways in which we can more easily and efficiently share and access the various types of data between individual groups and sub-communities, ways in which we model the inner heliosphere looking at the advantages and disadvantages of the available modelling, updates on present and future remote-sensing capabilities - including those on the STEREO /SDO/Solar Orbiter/Solar Probe+ Missions, and progress on use of the LOw Frequency ARray (LOFAR) and Murchison Widefield Array (MWA) radio arrays - pathfinders for the Square Kilometre Array (SKA) - linking remote-sensing observations of the inner heliosphere with those closer-in to the Sun as well as with in-situ measurements, and investigating further the ways in which these data sets all complement each other and are necessary to gain knowledge and understanding of the fundamental physical processes that occur within the inner heliosphere .
    Website:
    Welcome to Remote Sensing Workshop 2011


    Solar Wind 13

    Start : 2012-06-17 - End : 2012-06-22
    The Thirteenth International Solar Wind Conference, organized by the University of Alabama in Huntsville's Center of Space Plasma and Aeronomic Research (CSPAR) and the the University of California, Berkeley's Space Sciences Laboratory, will take place at Sheraton Keauhou Resort on Big Island, Hawaii, USA, from 17 to 22 June 2012. Please note that scientific sessions will start on Monday 18 June.
    The conference will conform to the traditional solar wind themes, addressing the current state of knowledge in the relevant fields of solar and heliospheric physics. In particular, the conference will focus on the physics ofthe corona, the origin and acceleration of the solar wind , its dynamical interactions throughout the heliosphere and the interstellar medium and its boundaries. The program will be composed of both invited lectures and contributed talks and posters.
    Website: SOLAR WIND 13


    SHINE Conference 2012 in Wailea Maui, Hawaii

    Start : 2012-06-25 - End : 2012-06-29
    SHINE stands for Solar Heliospheric and INterplanetary Environment. It is an affiliation of researchers within the solar, interplanetary, and heliospheric communities, dedicated to promoting an enhanced understanding of the processes by which energy in the form of magnetic fields and particles are produced by the Sun and/or accelerated in interplanetary space and on the mechanisms by which these fields and particles are transported to the Earth through the inner heliosphere .
    SHINE research focuses in particular upon the connection between events and phenomena on the Sun and their relation to solar wind structures in the inner heliosphere . The goal of SHINE activities is to enrich and strengthen both physical understanding and predictive capabilities for these phenomena.
    Website:
    SHINE Conference 2011


    Toulouse Space Show (France)

    Start : 2012-06-25 - End : 2012-06-28
    Toulouse will host the most important players in the global aerospace industry, particularly those focusing on space applications. It will provide the opportunity to meet with more than 1000 experts, service providers, clients, users, researchers and students from all over the world.
    Website:
    TOULOUSE SPACE SHOW


    European Week of Astronomy and Space Science in Rome, Italy

    Start : 2012-07-01 - End : 2012-07-06
    We have the pleasure to invite you in July 2012 to attend the European Week of Astronomy and Space Science, the now classical Ewass meeting, formely known as Jenam. In 2012, the meeting will take place in Rome, Italy, at the Pontificia Università Lateranense.
    Website:
    Ewass 2012 Website | European Week of Astronomy and Space Science


    International Summer School 'Solar Astrophysics: Modern trends and techniques' in Bogota, Colombia

    Start : 2012-07-03 - End : 2012-07-19
    The Sun is our closest and most well studied celestial object. From the beginnings of human civilizations, the Sun has played a major role in their development, and in the rituals and customs that can still be perceived in the modern world. Unprecedented advances and new missions have revealed the real complexity of the Sun. New missions like SDO, SolarProbe Plus and other satellite missions (RHESSI, SOHO , TRACE , YOHKOH , etc.) provide information that may help to unveil the secrets of our star . The Observatorio Astronomico Nacional and the Universidal Nacional de Colombia organises an International Summer School in Solar Physics, with the purpose of promoting the solar research in Colombia and help in the personal development of postgraduate students and young postdocs in this area from other countries.
    The International Summer School is intended to provide an advanced training in the field of solar physics to last year ungraduate students who are willing to write their final work in any area of solar physics, postgraduate students, and young post-docs having already some initial work in the fields of solar physics.
    Website:
    Universidad Nacional de Colombia - Solar Astrophysics School: Modern Trends and Techniques


    International Summer School 'Solar Astrophysics: Modern trends and techniques' in Bogota, Colombia

    Start : 2012-07-03 - End : 2012-07-19


    BUKS2012 in Fodele Beach, Crete, Greece

    Start : 2012-07-04 - End : 2012-07-07
    The Sun is the most important astronomical object for humankind with solar activity having a direct impact on Earth. From a fundamental point of view the Sun offers an exceptional physics laboratory where the interactions of the astrophysical plasma and the magnetic field can be studied in detail.
    The BUKS workshops on MHD waves and oscillations of the solar atmosphere is organised by the following research groups from Belgium, Spain and the UK:
    * The Centre for Plasma Astrophysics, Katholieke Universiteit Leuven, Belgium
    * The Solar Physics &amp; Space Plasma Research Centre, University of Sheffield, UK
    * The Solar &amp; Magnetospheric Theory Group, University of St Andrews, UK
    * The Centre for Fusion, Space &amp; Astrophysics, University of Warwick, UK
    * The Solar Physics Group, Universitat de les Illes Balears, Spain
    * The Astrophysics Research Centre, Queen's University Belfast, UK
    BUKS2012 will also honour the contributions of Prof Marcel Goossens to the field of MHD waves and offer an opportunity to celebrate his 65th birthday.
    Website:
    https://habu.pst.qub.ac.uk/groups/buks2012/


    23rd NASA Space Radiation Investigators’ Workshop in Durham, North Carolina (USA)

    Start : 2012-07-08 - End : 2012-07-11
    The 23rd Annual NASA Space Radiation Investigators’ Workshop will be held July 8–12, 2012, at the Washington Duke Inn, Durham, North Carolina. The purpose of this workshop is to provide an opportunity for active researchers in the NASA Space Radiation Program to share the results of their work and to explore new directions for research that may benefit the NASA program. The workshop format will include plenary sessions, poster sessions, and a poster contest to recognize and honor student investigators. In addition, there will be special sessions on space physics and technology allowing opportunities for a comprehensive discussion on NASA’s overall space radiation protection goals.
    Principal investigators receiving NASA funds (including those from the NASA /DOE joint program and the NSBRI) are required to attend; principal investigators funded by the Department of Energy are strongly encouraged to attend. Although attendance at the workshop is by invitation only, other scientists with a legitimate interest in space radiation research are also welcome. If you wish to attend, please send your requests directly to . Requests should be accompanied by an explanation of your relationship to the Space Radiation Program and the type of contribution you wish to make.
    Website:
    23rd Annual NASA Space Radiation Investigators' Workshop


    ESOF 2012 in Dublin, Ireland

    Start : 2012-07-11 - End : 2012-07-15
    From 11th-15th of July 2012 international researchers, policy makers, business leaders and global media will gather in the Convention Centre in Dublin, Ireland to take part in the Euroscience Open Forum (ESOF), 2012. A science conference like no other, ESOF 2012 is unique in representing the largest convergence of the Sciences, Humanities and Culture in Europe in 2012. Some of the keynote speakers at ESOF 2012 will include Craig Venter, Rolf-Dieter Heuer, Charles Bolden, Mary Robinson, and Bob Geldof.
    Website: ESOF 2012 DUBLIN


    39th COSPAR Scientific Assembly

    Start : 2012-07-14 - End : 2012-07-22
    The 39th COSPAR Scientific Assembly will be held at the Global Education Centre, 2 Infosys Training Centre Mysore, Karnataka India from 14 - 22 July 2012. This Assembly is open to all bona fide scientists.
    Website:
    COSPAR ZARM - Online Abstract Handling


    CISM Summer School in Boulder (USA)

    Start : 2012-07-16 - End : 2012-07-27
    The CISM Space Weather Summer School is a 2-week intensive program targeted to first-year graduate students but also attended by undergraduates and space weather professionals. The daily schedule includes morning lectures, followed by afternoon laboratory sessions where students further explore the day's topics using CISM model simulations, observational data, and sophisticated visualization tools. CISM is making the laboratory materials publicly available for use by others, for example to supplement lecture courses or for student independent study. The deadline for applications is May 1.
    Website:
    CISM // Summer School Overview


    IGS Workshop 2012 in Olsztyn, Poland

    Start : 2012-07-23 - End : 2012-07-27
    The Department of Astronomy and Geodynamics of the University of Warmia and Mazury (UWM) is hosting the 2012 IGS Workshop.
    This workshop will be composed or plenary sessions with invited oral presentations, and afternoon sessions composed of poster sessions and IGS Working Group splinter meetings. For this workshop we are soliciting abstracts for the poster sessions.
    The key dates for this workshop are as follows:
    * Poster Abstract Submissions: March 25 - April 30, 2012.
    * Registration: March 25- May 28, 2012.
    * Hotel Reservations: March 25- May 28, 2012.
    * Workshop: July 23 - July 27, 2012.
    Website:
    Welcome to the Frontpage


    International Radiation Symposium in Berlin (Germany)

    Start : 2012-08-06 - End : 2012-08-10
    The IRC's International Radiation Symposium 2012 provides a forum for the scientific community to exchange recent results and evolving ideas relevant to many areas of atmospheric radiation. Quadrennially convened, the IRS assembles a global network of scientists and students engaged in studies pertaining to the Earth-atmosphere-Sun system, and encourages international cooperation in radiation research crucial to understanding and predicting Earth's dynamic climate and habitability. The IRC invites you to Berlin and welcomes your participation in this endeavor.
    Website: IRS2012 - Home


    Asia Oceania Geosciences Society (AOGS) Assembly in Singapore

    Start : 2012-08-13 - End : 2012-08-17
    An international body established since 2003, the Asia Oceania Geosciences Society (AOGS) aims to promote geosciences and advance its applications for the benefit of humanity in Asia and Oceania.
    Sessions:
    * Atmospheric Sciences
    * Biogeosciences
    * Hydrological Sciences
    * Ocean Sciences
    * Planetary Sciences
    * Solar &amp; Terrestrial Sciences
    * Solid Earth Sciences
    * Interdisciplinary Working Groups
    Website:
    AOGS 2012


    Solar Information Processing Workshop (SIPWork VI), at Montana State University, Bozeman

    Start : 2012-08-13 - End : 2012-08-16
    You will have a noticed the slight re-branding of these workshops from ‘Image’ to ‘Information’ processing. We think it is time to expand the attention of these workshops to discuss more generally how information about the Sun can be derived, stored, shared, transformed and analyzed using appropriate techniques from many other disciplines. We will still be covering image processing and computer vision techniques applied to solar physics, but we will also be including other topics such as machine learning, data mining and new computing strategies. The re-branding simply acknowledges and makes explicit what the community has been doing to determine the physics of the Sun.
    Link: Solar Image Processing Workshops


    XXVIII IAU General Assembly in Beijing, China

    Start : 2012-08-20 - End : 2012-08-31
    In August 2012 China will for the first time host the General Assembly of the International Astronomical Union in Beijing. This triennial gathering of astronomers from around the world to discuss and debate the most recent discoveries about the universe is an important part of the vitality of our science. Astrophysics remains one of the most exciting areas of human endeavor, and the venue of the Beijing GA will be equally impressive: the new China National Convention Center that is housed in the Olympic Park in a beautiful, spacious building and area that is full of amenities for conference participants and visitors.
    The contributions of Chinese astronomy to human knowledge and our understanding of the cosmos have been of historical significance, from the earliest to modern times. GA participants will have an opportunity to experience the wide range of astronomical activities now taking place in China that include new projects, facilities, and institutes. They will also report on, and hear, the latest research results from every field of astronomy. An exciting scientific programme is being developed that will hold the interest of everyone. I am pleased to welcome all Union members and invited guests to join us in Beijing for what will be a memorable General Assembly.
    Website:
    http://www.astronomy2012.org


    International Meteor Conference in La Palma, Spain

    Start : 2012-09-20 - End : 2012-09-23
    Every year, the International Meteor Organization (IMO) organizes the International Meteor Conference (IMC). This conference deals with all aspects of meteor observation as well as the underlying physics and is aimed at both amateurs and professionals.
    The International Meteor Organization (IMO) will hold the 31st annual International Meteor Conference (IMC) on La Palma, Canary Islands, Spain, from 20 till 23 September, 2012. The conference will be organized by the Astro Travels agency in collaboration with the Cabildo of La Palma island authority which will sponsor this event.
    Website:
    Welcome | International Meteor Conference 2012


    63rd International Astronautical Congress in Naples, Italy

    Start : 2012-10-01 - End : 2012-10-05
    At the forthcoming 63rd International Astronautical Congress in Naples a special session on the theme 'Effects of Space Weather on GEO Satellites' will be held as part of the 25th Symposium on Space Policy, Regulations and Economics.
    This session will discuss case histories and mechanisms of effects of space weather on GEO satellites, models for prediction, and mitigation approaches. We would like to invite you to consider submitting abstracts for this session.
    The call for papers can be found at The deadline for abstract submission is 29 February 2012.
    http://www.iafastro.org/docs/2012/iac/IAC2012_CallForPapers.
    Website: IAC 2012 - 63RD INTERNATIONAL ASTRONAUTICAL CONGRESS


    Space Weather and Challenges for Modern Society in Oslo, Norway

    Start : 2012-10-22 - End : 2012-10-24
    2012 – 2013 is expected to be years with high solar activity. This can trigger larger solar storms which can generate geomagnetic induced currents (GIC ) on the earth. GIC can affect the normal operation of specific industrial operations and critical infrastructure (e.g power grids, telecom, navigation systems, etc).
    During space weather events, like solar storms, electric currents in the magnetosphere and ionosphere experience large variations, which manifest also in the earth's magnetic field. These variations induce currents (GIC ) in conductors operated on the surface of the earth. Electric transmission grids and buried pipelines are common examples of such conductor systems. GIC can cause problems, such as increased corrosion of pipeline steel and may disturb and possible damaged high-voltage power transformers and it can also have damaging effects on communication systems, navigation systems and oil and gas operations.
    Vulnerable industries are the oil and gas industry, railways, telecommunication industry, navigation industry and not at least the society, which is very vulnerable concerning short or long term interruption of critical infrastructure.
    The conference will focus on increasing the general knowledge of solar storms, space weather and GIC and the possible consequences for different industries and critical infrastructure, and look into reasonable means of protection, and consider possible early warning solutions.
    More information:
    http://www.tiems.info/images/stories/tiems 2012 oslo conference call for papers.pdf


    Ninth European Space Weather Week in Brussels, Belgium

    Start : 2012-11-05 - End : 2012-11-09
    We are pleased to announce that the Ninth European Space Weather Week will take place at the Académie Royale de Belgique, Brussels, Belgium between 5 and 9 November 2012.
    This meeting is being jointly organised by the Solar-Terrestrial Centre of Excellence (STCE), ESA , the SWWT and the COST ES0803 communities. The local organisation is done by the STCE. This event will continue to build on the advances made during the first eight European Space Weather Weeks held between 2004 and 2011.
    Website:
    esww9 - Home


    International Symposium on Solar-Terrestrial Physics in Pune, India

    Start : 2012-11-06 - End : 2012-11-09
    The International Symposium on Solar-Terrestrial Physics will be held during November 6 - 9, 2012 at the Indian Institute of Science, Education and Research, Pune, India. This meeting under the aegis of the SCOSTEP is expected to draw leading scientists from around the world in the increasingly important, interdisciplinary fields of Solar activity and its impact on geospace and life on the Earth. With major observational solar facilities being planned in India, this meeting is especially pertinent in the Indian context.
    The meeting is expected to involve professional scientists as well as graduate students, and will have a mixture of invited and contributed talks and posters. There will also be a one-day tutorial for the benefit of young people beginning work in the field of solar-terrestrial physics.
    Website:
    International Symposium on Solar-Terrestrial Physics


    Eclipse on the Coral Sea: Cycle 24 Ascending

    Start : 2012-11-12 - End : 2012-11-16
    As we emerge from one of the deepest and longest solar minima on record, with a new and powerful eye on the Sun -SDO- we invite all those with an interest is solar activity to gather in beautiful Palm Cove, Australia to review and assess our current knowledge and understanding of our magnetic star , and to experience the awe and wonder of a total solar eclipse on November 14, 2012.
    Website:
    Eclipse on the Coral Sea: Cycle 24 Ascending


    Total solar eclipse

    Start : 2012-11-13 - End : 2012-11-13
    For more information:
    NASA - Eclipses During 2012


    Tracing the Connections in Solar Eruptive Events in Petaluma, CA, USA

    Start : 2012-11-30 - End : 2012-12-05
    The overarching objective of the conference is to examine the connections amongst the phenomena that lead to solar eruptive events. The current state of themes includes:
    * Measuring the Coronal Magnetic Field;
    * Connections to, and Reactions of, the Large-Scale Corona;
    * Large-scale Magnetic Connectivity of Active Regions;
    * Transfer of Energy to, and Storage of Energy in, the Corona;
    * The High-Energy Particle - Flare - CME connection.
    Working groups will address topics such as:
    * Energy Transfer throughout a Solar Eruptive Event;
    * Global Energetics of an Ensemble of Events;
    * Coronal Influences to the Lower Atmosphere;
    * CME Initiation and Type II Bursts;
    * The Release of Energetic Particles in the Low Corona;
    * Flows vs. Waves;
    * Microflares/Nanoflares.
    Website:
    Solar in Sonoma Conference: Tracing the Connections in Solar Eruptive Events


    Earth-Sun System Exploration 5 in Kona, Hawai'i USA

    Start : 2013-01-13 - End : 2013-01-19
    Information coming soon!
    Website:
    Earth-Sun System Exploration 5 Conference


    Annular solar eclipse

    Start : 2013-05-10 - End : 2013-05-10
    For more information:
    http://eclipse.gsfc.nasa.gov/SEplot/SEplot2001/SE2013May10A.GIF


    Hybrid solar eclipse

    Start : 2013-11-03 - End : 2013-11-03
    For more information:
    http://eclipse.gsfc.nasa.gov/SEplot/SEplot2001/SE2013Nov03H.GIF
     
    Falkman, 24 มีนาคม 2012

    #1823
  4. tian3p

    tian3p สมาชิกใหม่

    วันที่สมัครสมาชิก:
    30 ธันวาคม 2011
    โพสต์:
    6
    ค่าพลัง:
    +1
    ไม่มีแบบสั้นๆเหรอ..ตาลาย
     
    tian3p, 24 มีนาคม 2012

    #1824
  5. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    อันนี้ไม่ต้องไปสนใจมันมากจ้า เอาเฉพาะคนที่อยากได้รายละเอียดจริงๆ ที่จะเอาข้อมูลไปวิเคราะห์
     
    Falkman, 24 มีนาคม 2012

    #1825
  6. nickybamby

    nickybamby เป็นที่รู้จักกันดี

    วันที่สมัครสมาชิก:
    11 ตุลาคม 2011
    โพสต์:
    216
    ค่าพลัง:
    +174
    แล้วช่วงที่ขาดหายไปหลายชั่วโมง จะรุ้ได้ไงว่าเกิดอะไรขึ้นบ้าง? :boo:
     
    nickybamby, 24 มีนาคม 2012

    #1826
  7. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    <table style="color: rgb(0, 0, 0); font-family: arial, sans-serif; font-size: 13px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; background-color: rgb(204, 255, 204); margin-bottom: 5px; display: table; " border="0" cellpadding="5" cellspacing="0" height="364" width="100%"><tbody><tr><td rowspan="1" colspan="1" style="margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; font-family: 'Times New Roman', Times; background-color: rgb(153, 153, 0); font-size: 18pt; color: rgb(255, 255, 0); text-align: center; " align="center" bgcolor="#999900" width="99%">
    Large 7.2 Quake Hits Chile -
    Tsunami Warning Issued​
    ​
    ​
    </td><td rowspan="1" colspan="1" style="margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; font-family: arial, sans-serif; background-color: rgb(153, 153, 0); text-align: left; " align="left" background="https://imgssl.constantcontact.com/letters/images/1101093164665/top_right.gif" bgcolor="#999900" width="1%">
    </td></tr><tr><td rowspan="1" colspan="2" style="margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; font-family: Verdana, Geneva, Arial, Helvetica, sans-serif; color: rgb(0, 0, 0); font-size: 10pt; text-align: left; " align="left">by Mitch Battros - Earth Changes Media

    [​IMG]
    A 7.2 magnitude earthquake struck central Chile prompting an evacuation of coastal areas for fear of a tsunami and causing scenes of panic in an area devastated by a massive quake two years ago.
    ​
    [​IMG] ​
    ​
    ​
    There were no immediate reports of deaths or significant damage, officials in Chile said; but authorities ordered the evacuation of the central coast of Chile -- the same area devastated in 2010, when officials were criticized for waiting too long to allow residents to escape a tsunami.
    ​
    [​IMG] ​
    ​
    ​
    The Pacific Tsunami Warning Center said "a destructive Pacific-wide tsunami is not expected." Government spokesman Andres Chadwick said the Office of National Emergencies had issued the evacuation order as a precaution due to "observation of a certain intake of the sea."
    ​
    [​IMG]​
    ​
    ​
    Recent solar activity may have contributed to this event.Watch for continued extreme weather events over the next 72 hours. This includes earthquakes, volcanoes, tornadoes, and hurricanes.

    Equation:​
    Charged Particles (sunspots, solar flares, filament, coronal holes, etc.) => Magnetic Field Shift => Shifting Ocean and Jet Stream Currents => Extreme Weather and Human Disruption (mitch battros 1998 Updated: 2012).



    FULL ARTICLE - http://bit.ly/H4qlS6​
    </td></tr></tbody></table>
     
    Falkman, 26 มีนาคม 2012

    #1827
  8. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    <table style="color: rgb(0, 0, 0); font-family: arial, sans-serif; font-size: 13px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; background-color: rgb(204, 255, 204); margin-top: 0.5px; margin-right: 0pt; margin-bottom: 0.5px; margin-left: 0pt; " border="0" cellpadding="5" cellspacing="0" width="100%"><tbody><tr><td rowspan="1" colspan="1" style="margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; font-family: Verdana, Geneva, Arial, Helvetica, sans-serif; color: rgb(0, 0, 0); font-size: 10pt; text-align: right; " align="right">
    <wbr> March 25, 2012
    ​
    </td></tr></tbody></table><table style="color: rgb(0, 0, 0); font-family: arial, sans-serif; font-size: 13px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; background-color: rgb(204, 255, 204); margin-bottom: 5px; display: table; " border="0" cellpadding="5" cellspacing="0" height="364" width="100%"><tbody><tr><td rowspan="1" colspan="1" style="margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; font-family: 'Times New Roman', Times; background-color: rgb(153, 153, 0); font-size: 18pt; color: rgb(255, 255, 0); text-align: center; " align="center" bgcolor="#999900" width="99%">
    Several CMEs Observed
    Over Past 24 Hours
    ​
    </td><td rowspan="1" colspan="1" style="margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; font-family: arial, sans-serif; background-color: rgb(153, 153, 0); text-align: left; " align="left" background="https://imgssl.constantcontact.com/letters/images/1101093164665/top_right.gif" bgcolor="#999900" width="1%">
    </td></tr><tr><td rowspan="1" colspan="2" style="margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; font-family: Verdana, Geneva, Arial, Helvetica, sans-serif; color: rgb(0, 0, 0); font-size: 10pt; text-align: left; " align="left">by Mitch Battros - Earth Changes Media

    [​IMG]
    Several CMEs were also observed over the last 24 hours coming from one or two sunspot regions just now rotating around the eastern limb of the Sun bringing them to face Earthside.
    ​
    [​IMG] ​
    ​
    ​
    Although this series of CMEs (coronal mass ejection) was not Earth directed, they do indicate active sunspot regions are rotating Earthside and like to produce moderate to large solar flares.

    An M1-class flare occurred at the southeast limb of the Sunfrom sunspot region 1445. There is a very low possibility this event will have any effect to Earth due to its location.
    ​
    [​IMG]​
    ​
    ​
    In addition, there is a trans-equatorial coronal hole that just passed the solar central meridian which may produce a cloud of charged particles which would be directly in-line with Earth creating a geomagnetic storm as it hits Earth's magnetic field.
    ​
    [​IMG] ​
    ​
    ​
    VIDEO of SEVERAL CME EVENTS BELOW​
    ​
    ​
    </td></tr></tbody></table>
     
    Falkman, 26 มีนาคม 2012

    #1828
  9. somsweet

    somsweet เป็นที่รู้จักกันดี

    วันที่สมัครสมาชิก:
    6 เมษายน 2011
    โพสต์:
    6,138
    ค่าพลัง:
    +9,874
    27 March 2012

    เหตุการณ์ที่ไม่คาดฝันทั่วโลกตลอด 3 เดือน ตั้งแต่ก้าวข้ามสู่ปี 2012มา เกิดอะไรขึ้นบ้าง มาดูกัน


    [ame="http://www.youtube.com/watch?v=MgGWrX3jxJo&feature=player_embedded"]2012-Signs in the Sun, Moon, and Stars-Just The First 3 Months - YouTube[/ame]#!


    B5 - War Room Falkman
     
    somsweet, 27 มีนาคม 2012

    #1829
  10. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    Falkman, 27 มีนาคม 2012

    #1830
  11. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    [​IMG]
     
    Falkman, 27 มีนาคม 2012

    #1831
  12. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    ANOTHER CME FROM SUNSPOT AR1429: Transiting the farside of the sun, never-say-die sunspot AR1429 erupted during the late hours of March 26th, producing its 11th major CME. The Solar and Heliospheric Observatory (SOHO) photographed the cloud flying over the sun's eastern limb:

    ​
    [​IMG]​
    According to a forecast track prepared by analysts at the Goddard Space Weather Lab, the CME will hit two spacecraft, STEREO-B and Spitzer, on March 28th. Earth is not in the line of fire.


    ​
    This event shows that AR1429, the source of several [ame="http://www.youtube.com/watch?v=EEFQHDSYP1I"]strong geomagnetic storms[/ame] in early March, is still active. It will begin turning back toward our planet about a week from now. Stay tuned.



    SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids​
     
    Falkman, 28 มีนาคม 2012

    #1832
  13. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    [​IMG]
     

    ไฟล์ที่แนบมา:

    Falkman, 28 มีนาคม 2012

    #1833
  14. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    NORTHERN LIGHTS OVER NEBRASKA: A solar wind stream is buffeting Earth's magnetic field, causing magnetic unrest and auroras at high latitudes. Last night faint Northern Lights descended all the way south to Nebraska. Click to view a movie of the display, photographed by Chris Allington of Crofton, NE:​
    [​IMG]​
    "I certainly didn't expect this tonight, but the plots were interesting enough to get me out and investigate the northern sky with the camera," says Allington. "Suprisingly, around 9:30pm local time I could see the color of the aurora on my camera so I decided to head to a wind farm near my house. The display got much more vibrant and lasted nearly 4 hours from 10pm to 2am. It's not often that auroras are hardly in the forecast and we see them as far south as NEBRASKA! "​
    The cause of the display was the interplanetary magnetic field (IMF), which tipped south and opened a crack in Earth's magnetosphere. Solar wind poured in to fuel the light. More high-latitude auroras are possible tonight: NOAA forecasters estimate a 50% chance of polar geomagnetic storms as the solar wind continues to blow. Aurora alerts: text, phone.


    SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids​
     
    Falkman, 29 มีนาคม 2012

    #1834
  15. FALCON1

    FALCON1 เป็นที่รู้จักกันดี

    วันที่สมัครสมาชิก:
    2 กรกฎาคม 2010
    โพสต์:
    3,522
    ค่าพลัง:
    +4,863
    [​IMG]

    C5 - War Room Falkman<!-- google_ad_section_end --><!-- google_ad_section_end -->
     
    FALCON1, 29 มีนาคม 2012

    #1835
  16. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    Gigantic Solar Tornado Is 5 Times the Size of Earth





    [​IMG]
    This enormous tornado erupting from the surface of the sun is big enough to swallow the Earth. In fact, it could swallow five Earths.
    Discovered using NASA’s Solar Dynamic Observatory satellite, this colossal twisting mass is made up of superheated gas at a temperature of between 90,000 and 3.6 million degrees Fahrenheit.
    [​IMG]Over the course of three hours, this behemoth reached up from the sun’s surface to a height of 125,000 miles, or roughly half the distance between the Earth and the moon. The hot gases were whipped up to nearly 186,000 miles per hour. In comparison, the wind speed of terrestrial tornadoes generally reaches a paltry 100 miles per hour.
    Scientists have previously seen smaller solar tornadoes with other sun-observing satellites but this one — spotted in September 2011 — is thought to be the first one ever filmed (left). Since then, researchers have seen at least one more solar tornado, an Earth-sized twister seen in the video below.
    These tornadoes often precede events known as coronal mass ejections — huge eruptions of charged particles that blast out of the sun’s surface with tremendous energy. Such flare-ups are thought to be related to interactions among the sun’s magnetic field lines, whose corkscrewing movements also shape the solar tornado.
    The top images and movie were presented at the National Astronomy Meeting 2012 in Manchester, England on Mar. 29.


    Images and first movie: NASA/SDO/AIA/Aberystwyth University/Li/Morgan/Leonard
    Second movie: Another enormous solar tornado, spotted Feb. 7 to 8, 2012. SDO/VideosFromSpace/Youtube




    ที่มา Gigantic Solar Tornado Is 5 Times the Size of Earth | Wired Science | Wired.com
     
    Falkman, 29 มีนาคม 2012

    #1836
  17. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    'Habitable' planets found orbiting red dwarf stars in our galaxy - and there could be billions, including 100 'next door' to Earth

    By Rob Waugh

    PUBLISHED: 09:57 GMT, 28 March 2012 | UPDATED: 09:57 GMT, 28 March 2012


    Billions of potentially habitable planets may exist in our galaxy, the Milky Way - including 100 'super Earths' within 30 light years from our solar system.

    A survey of red dwarf stars in the Milky Way found nine super-Earths - and two in the 'habitable zone' where liquid water could exist.

    Red dwarf stars account for 80% of the 200-400 billion stars in the Milky Way - and the scientists now believe that 40% of those might have a planet in the habitable zone.
    [​IMG]

    A sunset seen from the super-Earth planet Gliese 667 Cc. Billions of potentially habitable planets may exist in our galaxy, the Milky Way, according to a new study

    A sunset seen from the super-Earth planet Gliese 667 Cc. Billions of potentially habitable planets may exist in our galaxy, the Milky Way, according to a new study

    They calculate that around 40% of red dwarfs have a rocky planet not much bigger than Earth orbiting the ‘habitable zone’ where liquid surface water can exist.

    Where there is water, there could be life - although being in the habitable zone is no guarantee that life has evolved on a planet.

    Dr Xavier Bonfils, from Grenoble University in France, who led the international team, said: ‘Because red dwarfs are so common - there are about 160 billion of them in the Milky Way - this leads us to the astonishing result that there are tens of billions of these planets in our galaxy alone.’


    The astronomers surveyed a carefully chosen sample of 102 red dwarfs using the European Southern Observatory's 3.6-metre telescope at La Silla, Chile.

    A total of nine super-Earths - planets with masses between one and 10 times that of Earth - were found.

    Two were located within the habitable zones of the stars Gliese 581 and Gliese 667 C.

    [​IMG]

    A simplified diagram showing the sizes of stars. 80% of stars in our Milky Way galaxy are red dwarf stars

    A simplified diagram showing the sizes of stars. 80% of stars in our Milky Way galaxy are red dwarf stars

    [​IMG]

    An artist's impression of the surface of a planet orbiting a red dwarf. The new discovery hints there may be billions of habitable worlds in the Milky Way

    An artist's impression of the surface of a planet orbiting a red dwarf. The new discovery hints there may be billions of habitable worlds in the Milky Way


    These data were combined with other observations, including those of stars which did not have planets.

    The astronomers worked out that habitable zone super-Earths orbiting red dwarfs occurred with a frequency of around 41%.

    On the other hand massive planets similar to Jupiter and Saturn were rare around red dwarfs. Less than 12% of the stars were expected to have such ‘gas giants’.

    Because red dwarfs are common near the sun, many ‘super-Earths’ may not be far away in astronomical terms. The scientists estimate there could be around 100 habitable zone planets within 30 light years.

    Red dwarfs are cooler than the sun, which means planets must orbit close to their parent stars to be warm enough to be habitable.

    This might not be good news for life.

    ‘The habitable zone around a red dwarf, where the temperature is suitable for liquid water to exist on the surface, is much closer to the star than the Earth is to the sun,’ said team member Dr Stephane Udry, from Geneva Observatory.

    ‘But red dwarfs are known to be subject to stellar eruptions or flares, which may bathe the planet in X-rays or ultraviolet radiation, and which may make life there less likely.’

    The research is reported in the journal Astronomy & Astrophysics.

    Read more: 'Habitable' planets found orbiting red dwarf stars in our galaxy - and there could be billions more, including 100 'next door' to our solar system | Mail Online
     
    Falkman, 29 มีนาคม 2012

    #1837
  18. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    มันจะหมุนกลับมาอีกแล้ว 1429

    RETURN OF THE SUNSPOT: Sunspot AR1429, the source of many [ame="http://www.youtube.com/watch?v=EEFQHDSYP1I"]strong flares[/ame] and geomagnetic storms earlier this month, is about to re-appear following a two-week trip around the backside of the sun. Magnetic loops towering over the sun's NE limb herald the sunspot's approach:​
    [​IMG]​
    Earlier today, NASA's Solar Dynamics Observatory photographed plumes of plasma rising and falling over the limb: movie. Moreover, a pair of solar flares (C5- and C7-class) in the sunspot's towering magnetic canopy caused waves of ionization to ripple through the high atmosphere over Europe.


    ​
    While sunspot AR1429 was transiting the farside, it erupted multiple times. Between March 23rd and March 27th, the Solar and Heliospheric Observatory (SOHO) recorded four coronal mass ejections, each racing away from the sun faster than 3 million mph: movie. Collectively, these events suggest AR1429 might still be capable of potent solar activity. Stay tuned. Solar flare alerts: text, phone.



    SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids​
     
    Falkman, 30 มีนาคม 2012

    #1838
  19. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    Daily Sun: 31 Mar 12 <table border="0" cellpadding="0" cellspacing="0" width="100%"> <tbody><tr> <td>[​IMG]</td> </tr> </tbody></table> [​IMG] <table border="0" cellpadding="0" cellspacing="0" width="100%"> <tbody><tr> <td>[​IMG]</td> </tr> </tbody></table> Returning sunspot AR1429 is just a shadow of its former self, having decayed substantially during its two week trip around the backside of the sun. Credit: SDO/HMI
     
    Falkman, 31 มีนาคม 2012

    #1839
  20. Falkman

    Falkman พลังจิตนานาชาติ ทีมงาน ผู้ดูแลเว็บบอร์ด

    วันที่สมัครสมาชิก:
    3 กรกฎาคม 2006
    โพสต์:
    19,726
    ค่าพลัง:
    +77,791
    จับตาการเรียงตัวของดาวเคราะห์ช่วงวันที่ 1 ถึง 30 เมษายน คศ 2012 : update 2 เมษายน 1:15 UTC

    [​IMG]

    Submitted by Administration on Sun, 2012-04-01 07:00
    ช่วงเวลา: Sun, 2012-04-01 - Mon, 2012-04-30

    [​IMG]

    ในครั้งนี้เราจะมาสังเกตการณ์การเรียงตัวของดาวเคราะห์ และอิทธิพลของปรากฏการณ์นี้ต่อปฏิกริยาของดวงอาทิตย์และการเปลี่ยนแปลงทาง สภาพอากาศบนโลก ซึ่งทางเวปได้ทำการทดลองมาเป็นเวลานานและได้พบความสัมพันธ์ที่สามารถนำมาใช้ คาดการณ์การเปลี่ยนแปลงของโลกได้ ซึ่งพบว่าปรากฏการณ์มีคุณสมบัติหลายๆอย่างตรงกับการคุณสมบัติของการเปลียน แปลงทางพลังงานไฟฟ้า

    ในช่วงเวลานี้จะมีแนวการเรียงตัวของดาวเคราะห์ที่สำคัญสองช่วงได้แก่ใน วันที่ 15 เมษายน และ ระหว่างวันที่ 18-20 เมษายน ซึ่งคาดว่าจะมีการเปลี่ยนแปลงทางธรรมชาติย่างมีนัยสำคัญสูงโดยเฉพาะปฏิกริยา ดวงอาทิตย์ และจะมีภัยพิบัติเกิดขึ้นเป็นพิเศษในบางพื้นที่บนโลกในช่วงวันดังกล่าวและ หลังจากนั้น นอกจากเรื่องของภัยพิบัติทางธรรมชาติแล้ว พลังงานพายุสุริยะยังสามารถส่งผลกระทบต่อสุขภาพของมนุษย์ได้อีกด้วย ดังนั้นผู้ที่ร่างกายไม่แข็งแรงโปรดรักษาสุขภาพในช่วงวันดังกล่าวเป็นพิเศษ เพื่อลดโอกาสการเจ็บป่วย

    อ้างอิง: จับตาการเรียงตัวของดาวเคราะห์ช่วงวันที่ 1 ถึง 30 เมษายน คศ 2012 : update 2 เมษายน 1:15 UTC | Truth4Thai.org


    <TABLE style="WIDTH: 443pt; BORDER-COLLAPSE: collapse" border=0 cellSpacing=0 cellPadding=0 width=590><COLGROUP><COL style="WIDTH: 86pt; mso-width-source: userset; mso-width-alt: 3660" width=114><COL style="WIDTH: 195pt; mso-width-source: userset; mso-width-alt: 8320" width=260><COL style="WIDTH: 162pt; mso-width-source: userset; mso-width-alt: 6912" width=216><TBODY><TR style="HEIGHT: 15pt" height=20><TD style="BORDER-BOTTOM: #f0f0f0; BORDER-LEFT: #f0f0f0; BACKGROUND-COLOR: transparent; WIDTH: 443pt; HEIGHT: 15pt; BORDER-TOP: #f0f0f0; BORDER-RIGHT: #f0f0f0; mso-ignore: colspan" class=xl91 height=20 width=590 colSpan=3 align=left>ตารางสรุปปรากฏการณ์ดาวเคราะห์เรียงตัวและการเปลี่ยนแปลงต่อโลกในช่วงนี้

    </TD></TR></TBODY></TABLE>​

    <TABLE style="WIDTH: 393pt; BORDER-COLLAPSE: collapse" border=0 cellSpacing=0 cellPadding=0 width=524><COLGROUP><COL style="WIDTH: 76pt; mso-width-source: userset; mso-width-alt: 3225" width=101><COL style="WIDTH: 155pt; mso-width-source: userset; mso-width-alt: 6630" width=207><COL style="WIDTH: 162pt; mso-width-source: userset; mso-width-alt: 6912" width=216><TBODY><TR style="HEIGHT: 14.4pt" height=19><TD style="BORDER-BOTTOM: black 1pt solid; BORDER-LEFT: black 1pt solid; BACKGROUND-COLOR: #c2d69a; WIDTH: 76pt; HEIGHT: 14.4pt; BORDER-TOP: black 1pt solid; BORDER-RIGHT: black 0.5pt solid" class=xl89 height=19 width=101>วันที่</TD><TD style="BORDER-BOTTOM: black 1pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: #c2d69a; WIDTH: 155pt; BORDER-TOP: black 1pt solid; BORDER-RIGHT: black 0.5pt solid" class=xl90 width=207>ปรากฏการณ์</TD><TD style="BORDER-BOTTOM: black 1pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: #c2d69a; WIDTH: 162pt; BORDER-TOP: black 1pt solid; BORDER-RIGHT: black 1pt solid" class=xl91 width=216>วันสังเกตผลกระทบต่อโลก</TD></TR><TR style="HEIGHT: 13.8pt" height=18><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black 1pt solid; BACKGROUND-COLOR: transparent; WIDTH: 76pt; HEIGHT: 13.8pt; BORDER-TOP: #f0f0f0; BORDER-RIGHT: black 0.5pt solid" class=xl73 height=18 width=101>3 เมย</TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 155pt; BORDER-TOP: #f0f0f0; BORDER-RIGHT: black 0.5pt solid" class=xl70 width=207>ดวงอาทิตย์-โลก-ดวงจันทร์</TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 162pt; BORDER-TOP: #f0f0f0; BORDER-RIGHT: black 1pt solid" class=xl71 width=216>2-4 เมย</TD></TR><TR style="HEIGHT: 13.8pt" height=18><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black 1pt solid; BACKGROUND-COLOR: transparent; WIDTH: 76pt; HEIGHT: 13.8pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl74 height=18 width=101>5 เมย</TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 155pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl66 width=207>ดวงอาทิตย์ดาวพุธดาวพฤหัส</TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 162pt; BORDER-TOP: black; BORDER-RIGHT: black 1pt solid" class=xl67 width=216>10-11 เมย</TD></TR><TR style="HEIGHT: 27.6pt" height=37><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black 1pt solid; BACKGROUND-COLOR: transparent; WIDTH: 76pt; HEIGHT: 27.6pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl74 height=37 width=101>7-13 เมย</TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 155pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl66 width=207></TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 162pt; BORDER-TOP: black; BORDER-RIGHT: black 1pt solid" class=xl67 width=216>มีความน่าจะเป็นที่มีพายุสุริยะส่งผลต่อโลกในวันที่ 14-16 เมย</TD></TR><TR style="HEIGHT: 14.4pt" height=19><TD style="BORDER-BOTTOM: #f0f0f0; BORDER-LEFT: black 1pt solid; BACKGROUND-COLOR: red; WIDTH: 76pt; HEIGHT: 14.4pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl76 height=19 width=101>15 เมย</TD><TD style="BORDER-BOTTOM: #f0f0f0; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 155pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl77 width=207>ดวงอาทิตย์โลกดาวเสาร์</TD><TD style="BORDER-BOTTOM: #f0f0f0; BORDER-LEFT: black; BACKGROUND-COLOR: red; WIDTH: 162pt; BORDER-TOP: black; BORDER-RIGHT: black 1pt solid" class=xl92 width=216>15, 17-19 เมย</TD></TR><TR style="HEIGHT: 14.4pt" height=19><TD style="BORDER-BOTTOM: black 2pt double; BORDER-LEFT: black 1pt solid; BACKGROUND-COLOR: #d99795; WIDTH: 76pt; HEIGHT: 56.4pt; BORDER-TOP: black 2pt double; BORDER-RIGHT: black 0.5pt solid" class=xl80 height=74 rowSpan=4 width=101>17-20 เมย</TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: #d99795; WIDTH: 155pt; BORDER-TOP: black 2pt double; BORDER-RIGHT: black 0.5pt solid" class=xl81 width=207>ดวงอาทิตย์ โลกดวงจันทร์</TD><TD style="BORDER-BOTTOM: black 2pt double; BORDER-LEFT: black 0.5pt solid; BACKGROUND-COLOR: #d99795; WIDTH: 162pt; BORDER-TOP: black 2pt double; BORDER-RIGHT: black 1pt solid" class=xl82 rowSpan=4 width=216>17-20 เมย, 22-25 เมย</TD></TR><TR style="HEIGHT: 13.8pt" height=18><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: #d99795; WIDTH: 155pt; HEIGHT: 13.8pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl84 height=18 width=207>ดวงอาทิตย์ ดาวพุธดาววีนัส</TD></TR><TR style="HEIGHT: 13.8pt" height=18><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: #d99795; WIDTH: 155pt; HEIGHT: 13.8pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl84 height=18 width=207>ดวงอาทิตย์วีนัสทางช้างเผือก</TD></TR><TR style="HEIGHT: 14.4pt" height=19><TD style="BORDER-BOTTOM: black 2pt double; BORDER-LEFT: black; BACKGROUND-COLOR: #d99795; WIDTH: 155pt; HEIGHT: 14.4pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl87 height=19 width=207>ดวงอาทิตย์ดาวพุธ ทางช้างเผือก</TD></TR><TR style="HEIGHT: 14.4pt" height=19><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black 1pt solid; BACKGROUND-COLOR: transparent; WIDTH: 76pt; HEIGHT: 14.4pt; BORDER-TOP: #f0f0f0; BORDER-RIGHT: black 0.5pt solid" class=xl78 height=19 width=101>24 เมย</TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 155pt; BORDER-TOP: #f0f0f0; BORDER-RIGHT: black 0.5pt solid" class=xl70 width=207>ดวงอาทิตย์โลกดวงจันทร์</TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 162pt; BORDER-TOP: #f0f0f0; BORDER-RIGHT: black 1pt solid" class=xl79 width=216>23-24 เมย</TD></TR><TR style="HEIGHT: 13.8pt" height=18><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black 1pt solid; BACKGROUND-COLOR: transparent; WIDTH: 76pt; HEIGHT: 13.8pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl74 height=18 width=101>28 เมย</TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 155pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl66 width=207>ดวงอาทิตย์ดาวพุธดาวเสาร์</TD><TD style="BORDER-BOTTOM: black 0.5pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; WIDTH: 162pt; BORDER-TOP: black; BORDER-RIGHT: black 1pt solid" class=xl67 width=216>1-2 พค</TD></TR><TR style="HEIGHT: 14.4pt" height=19><TD style="BORDER-BOTTOM: black 1pt solid; BORDER-LEFT: black 1pt solid; BACKGROUND-COLOR: transparent; HEIGHT: 14.4pt; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl75 height=19></TD><TD style="BORDER-BOTTOM: black 1pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; BORDER-TOP: black; BORDER-RIGHT: black 0.5pt solid" class=xl68></TD><TD style="BORDER-BOTTOM: black 1pt solid; BORDER-LEFT: black; BACKGROUND-COLOR: transparent; BORDER-TOP: black; BORDER-RIGHT: black 1pt solid" class=xl69></TD></TR></TBODY></TABLE>

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    แนวดาวเรียงตัววันที่ 15-17 เมษายน
     
    Falkman, 2 เมษายน 2012

    #1840
หน้า 92 ของ 233

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