เหตุการณ์ใน-นอกโลก VS ภัยธรรมชาติ และupdate พายุสุริยะ

Some Comets like it Hot

<table class="table_generic center" summary="media files table" style="vertical-align: baseline; font-weight: normal; font-style: normal; font-size: 13px; outline-width: 0px; outline-style: initial; outline-color: initial; padding-top: 0px; padding-right: 0px; padding-bottom: 0px; padding-left: 0px; margin-top: 0px; margin-right: auto !important; margin-bottom: 0px; margin-left: auto !important; border-top-width: 0px; border-right-width: 1px; border-bottom-width: 1px; border-left-width: 0px; border-style: initial; border-color: initial; border-image: initial; float: none; overflow-x: hidden; overflow-y: hidden; border-collapse: collapse; border-bottom-style: solid; border-bottom-color: rgb(204, 204, 204); border-right-style: solid; border-right-color: rgb(204, 204, 204); color: rgb(0, 0, 0); font-family: Arial, Helvetica, sans-serif; font-variant: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-align: -webkit-auto; 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); width: 450px; " border="1" cellpadding="0" cellspacing="0"><tbody style="vertical-align: baseline; font-weight: inherit; font-style: inherit; font-size: 13px; outline-width: 0px; outline-style: initial; outline-color: initial; padding-top: 0px; padding-right: 0px; padding-bottom: 0px; padding-left: 0px; margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; border-top-width: 0px; border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-style: initial; border-color: initial; border-image: initial; "><tr style="vertical-align: baseline; font-weight: inherit; font-style: inherit; font-size: 13px; outline-width: 0px; outline-style: initial; outline-color: initial; padding-top: 0px; padding-right: 0px; padding-bottom: 0px; padding-left: 0px; margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; border-top-width: 0px; border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-style: initial; border-color: initial; border-image: initial; "><td style="vertical-align: top; font-weight: inherit; font-style: inherit; font-size: 13px; outline-width: 0px; outline-style: initial; outline-color: initial; padding-top: 5px; padding-right: 5px; padding-bottom: 5px; padding-left: 5px; margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; border-top-width: 1px; border-right-width: 0px; border-bottom-width: 0px; border-left-width: 1px; border-style: initial; border-color: initial; border-image: initial; text-align: center; border-top-style: solid; border-top-color: rgb(204, 204, 204); border-left-style: solid; border-left-color: rgb(204, 204, 204); ">[ame="http://www.youtube.com/watch?v=w75lBn1QIaI"]Play ScienceCast Video[/ame]</td><td style="vertical-align: top; font-weight: inherit; font-style: inherit; font-size: 13px; outline-width: 0px; outline-style: initial; outline-color: initial; padding-top: 5px; padding-right: 5px; padding-bottom: 5px; padding-left: 5px; margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; border-top-width: 1px; border-right-width: 0px; border-bottom-width: 0px; border-left-width: 1px; border-style: initial; border-color: initial; border-image: initial; text-align: center; border-top-style: solid; border-top-color: rgb(204, 204, 204); border-left-style: solid; border-left-color: rgb(204, 204, 204); ">Join Mailing List</td></tr></tbody></table>Jan. 12, 2012: Comets are icy and fragile. They spend most of their time orbiting through the dark outskirts of the solar system safe from destructive rays of intense sunlight. The deepest cold is their natural habitat.
Last November amateur astronomer Terry Lovejoy discovered a different kind of comet. The icy fuzzball he spotted in the sky over his backyard observatory in Australia was heading almost directly for the sun. On Dec. 16<sup style="vertical-align: baseline; font-weight: inherit; font-style: inherit; font-size: 0.8em; outline-width: 0px; outline-style: initial; outline-color: initial; padding-top: 0px; padding-right: 0px; padding-bottom: 0px; padding-left: 0px; margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-left: 0px; border-top-width: 0px; border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-style: initial; border-color: initial; border-image: initial; bottom: 0.5em; position: relative; ">th</sup>, less than three weeks after he found it, Comet Lovejoy would swoop through the sun’s atmosphere only 120,000 km above the stellar surface.
Astronomers soon realized a startling fact: Comet Lovejoy likes it hot.
"Terry found a sungrazer," says Karl Battams of the Naval Research Lab in Washington DC. "We figured its nucleus was about as wide as two football fields—the biggest such comet in nearly 40 years.”



Comet Lovejoy at sunrise on Dec. 25, 2011. Wayne England took the picture from Poocher Swamp, west of Bordertown, South Australia. [more]

Sungrazing comets aren't a new thing. In fact, the orbiting Solar and Heliospheric Observatory (SOHO) watches one fall toward the sun and evaporate every few days. These frequent kamikaze comets, known as “Kreutz sungrazers,” are thought to be splinters of a giant comet that broke apart hundreds of years ago. Typically they measure about 10 meters across, small, fragile, and easily vaporized by solar heat.

Based on its orbit, Comet Lovejoy was surely a member of the same family—except it was 200 meters wide instead of the usual 10. Astronomers were eager to see such a whopper disintegrate. Even with its extra girth, there was little doubt that it would be destroyed.

When Dec. 16th came, however, "Comet Lovejoy shocked us all," says Battams. "It survived, and even flourished.”

Images from NASA's Solar Dynamics Observatory showed the comet vaporizing furiously as it entered the sun's atmosphere--apparently on the verge of obliteration—yet Comet Lovejoy was still intact when it emerged on the other side. The comet had lost its tail during the fiery transit--a temporary setback. Within hours, the tail grew back, bigger and brighter than before.

"It's fair to say we were dumbfounded," says Matthew Knight of the Lowell Observatory and the Johns Hopkins Applied Physics Lab. "Comet Lovejoy must have been bigger than we thought, perhaps as much as 500 meters wide."

That would make it the biggest sungrazer since Comet Ikeya-Seka almost 40 years ago. With a tail that stretched halfway across the sky, Ikeya-Seki was actually visible in broad daylight after it passed through the sun's atmosphere in October 1965. In Japan, where observers spotted the over-heated comet only 1/2 degree from the sun, it was described as 10 times brighter than the Full Moon.

Comet Lovejoy wasn't that bright, but it was still amazing. Only a few days after it left the sun, the comet showed up in the morning skies of the southern hemisphere. Observers in Australia, South America, South Africa, and New Zealand likened it to a search light beaming up from the east before dawn. The tail lined up parallel to the Milky Way and, for a few days, made it seem that we lived in a double-decker galaxy.


This sequence of images, gathered by an extreme UV telescope onboard NASA's STEREO-B spacecraft, shows Comet Lovejoy's tail wiggling wildly in transit through the solar corona. [animation]

Astronauts on the International Space Station also witnessed the comet. ISS Commander Dan Burbank, who has seen his share of wonders, even once flying directly through the Northern Lights onboard the space shuttle, declared Comet Lovejoy “the most amazing thing I have ever seen in space.”

An armada of spacecraft including SOHO, the Solar Dynamics Observatory, NASA's twin STEREO probes, Japan’s Hinode spacecraft, and Europe's Proba2 microsatellite recorded the historic event.
"We've collected a mountain of data," says Knight. "But there are some things we're still having trouble explaining."

For instance, what made Lovejoy's tail wiggle so wildly when it entered the solar corona? Perhaps it was in the grip of the sun's powerful magnetic field.

What caused Lovejoy to lose its tail inside the sun's atmosphere—and then regain it later? “This is one of the biggest mysteries to me,” says Battams.
And then there is the ultimate existential puzzle: How did Comet Lovejoy survive at all?
As January unfolds, the “Comet that liked it Hot” is returning to the outer solar system, still intact, leaving many mysteries behind. “It’ll be back in about 600 years,” says Knight. “Maybe we will have figured them out by then.”

Author:Dr. Tony Phillips| Production editor: Dr. Tony Phillips | Credit: Science@NASA​

 

FARSIDE ERUPTION: Today, Jan. 12th, between 10:00 and 1300 UT, NASA's STEREO-Behind spacecraft observed a significant eruption on the farside of the sun. Although the blast was eclipsed by the edge of the solar disk, it nevertheless produced a long-duration X-ray flare (C3-class) detectable from Earth. A movie from NASA's Solar Dynamics Observatory shows some of the debris flying over the NE limb:


การระเบิดของดวงอาทิตย์ด้านที่ไม่ตรงกับโลก: วันที่ 12 มกราคม เวลาประมาณ 10-13 UT (ห้าโมงเย็น-สองทุ่ม เวลาไทย) ดาวเทียม STEREO behind ได้จับเห็นการระเบิดครั้งสำคัญที่ดวงอาทิตย์ด้านที่ไม่ตรงกับโลก และ การระเบิดถูกปิดโดยจานที่บังแสงดวงอาทิตย์ไว้ ถึงอย่างไรก็ตามมันทำให้เกิด x-ray flare เป็นเวลานนานมาก ตรวจจับได้จากโลก และในวิดีโอก็จะเห็นว่าบางส่วนของการระเบิดได้วิ่งผ่านไปทางตะวันออกเฉียงเหนือของดวงอาทิตย์


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The blast site is not far behind the eastern limb, and it is only ~two days away from rotating onto the Earthside of the sun.



จุดของการระเบิดครั้งนี้ ไม่ได้ไปหลังดวงอาทิตย์มากนัก และก็แค่สองวันที่จุดตรงนี้จะหันมายังโลก



By this weekend, we'll get a direct look at the active region. Perhaps it will break the recent string of mostly quiet days and low solar activity. Solar flare alerts: text, voice.



SpaceWeather.com -- News and information about meteor showers, solar flares, auroras, and near-Earth asteroids

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Small Flare, Big Show:
Even small solar flares can put on nice light shows. This C1.5 solar flare early Thursday morning around Sunspot 1391 was captured by SDO in the movie below.

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Solar Update:
Sunspot 1393 is now located on the western limb and out of direct Earth view. Solar activity did drop to very low levels, however that may change in the upcoming days.


An active region looks to be hiding on the northeast limb and will soon begin to rotate into direct Earth view. An explosion this morning produced a Coronal Mass Ejection (CME) off the limb that registered as a very long duration C-Class flare. Click HERE for a movie.




จุดดับ 1391 - ตั้งอยูบน N12 ของดวงอาทิตย์
ลองมาดูบนโลก ถ้าตรงกับไทยนี่จะกินพื้นที่ใดบ้าง
ประมาณเพชรบุรี ประจวบ (ด้านตะวันตก)
ชลบุรี ระยอง จันทบุรี ตราด (ด้านตะวันออก)

คาดว่าอาจมีน้ำมาเยอะ(หรือแผ่นดินไหว) -->คาดการณ์

Sunspots and active regions

The following regions with sunspots can be now observed on the Sun's surface
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</td> </tr> <tr> <th width="1%"> Group number </th> <th width="10%"> Sunspots Location on the Sun </th> <th width="11%"> The number of spots in the group </th> <th width="20%"> The classification by the Zurich's modified system </th> <th width="30%"> Area (millions of shares of the solar hemisphere) </th> <th width="9%"> Group length (in degrees) </th> <th width="16%"> Carrington Longitude (in degrees) </th> <th class="last" width="1%"> Group's magnet type </th> </tr> <tr class="separator_1"> <td>
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</td> </tr> <tr> <td nowrap="nowrap"> № 1391 </td> <td> N12 W51 </td> <td class="center"> 11 </td> <td class="center"> Cao </td> <td class="center"> 0180 </td> <td class="center"> 09 </td> <td class="center"> 011 </td> <td class="center"> Beta </td> </tr> <tr class="separator_1"> <td>
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</td> </tr> <tr> <td nowrap="nowrap"> № 1395 </td> <td> N21 E07 </td> <td class="center"> 02 </td> <td class="center"> Hsx </td> <td class="center"> 0070 </td> <td class="center"> 01 </td> <td class="center"> 313 </td> <td class="center"> Alpha </td> </tr> <tr class="separator_1"> <td>
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</td> </tr> <tr> <td nowrap="nowrap"> № 1396 </td> <td> N25 E32 </td> <td class="center"> 02 </td> <td class="center"> Bxo </td> <td class="center"> 0010 </td> <td class="center"> 03 </td> <td class="center"> 287 </td> <td class="center"> Beta </td> </tr> </tbody></table> Coordinates and other characteristics of active regions are issued for January 13, 2012 00:31 UT

Daily Sun: 12 Jan 12 <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> All of these sunspots have simple, quiet magnetic fields. The chance of flares is low. Credit: SDO/HMI

 

12-13 มกราคม ดวงอาทิตย์-โลก-ดวงจันทร์
ดวงอาทิตย์-โลก-ศุกร์
ดวงอาทิตย์-โลก-ดาวเสาร์
ดวงอาทิตย์-วีนัส-ดาวเสาร์
- และพายุสุริยะจะส่งผลกระทบต่อโลกในระหว่างวันที่ 15-17 มกราคม



จับตาการเรียงตัวของดาวเคราะห์ช่วงวันที่ 25 ธันวาคม 2011 ถึง 18 มกราคม 2012 : update 11 มกราคม 3:03 UTC | Truth4Thai.org

 

[ame=http://www.youtube.com/watch?v=ZJsCz0eIMN0]Major ALERT Massive HAARP Ring Australian NT - YouTube[/ame]

 

[ame=http://www.youtube.com/watch?v=iDfwHU7Cw6g]Conspiracy Theory W/ Jesse Ventura: HAARP [Season 1, Episode 1] (Full Length • HD) - YouTube[/ame]

 

January 14, 2012

Diagram of the solar flare activity

X-ray emission of the Sun from 13.01.2012 to 14.01.2012 (GOES-15)


Solar flares today

Today, 3 solar flares were observed:

<table class="table_4" width="750" cellpadding="0" cellspacing="0"><tbody><tr> <th width="1%"> </th> <th width="1%" align="left"> </th> <th>Active region</th> <th>Begin, UT</th> <th>Max, UT</th> <th>End, UT</th> </tr> <tr> <td nowrap="nowrap"></td> <td align="left" nowrap="nowrap">Flare of class C2.1</td> <td class="center">1396</td> <td class="center">03:19:00</td> <td class="center">03:35:00</td> <td class="center">04:03:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td> </tr> <tr> <td nowrap="nowrap"></td> <td align="left" nowrap="nowrap">Flare of class C4.1</td> <td class="center">0</td> <td class="center">12:00:00</td> <td class="center">12:09:00</td> <td class="center">12:20:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td> </tr> <tr> <td nowrap="nowrap"></td> <td align="left" nowrap="nowrap">Flare of class M1.4</td> <td class="center">0</td> <td class="center">13:14:00</td> <td class="center">13:18:00</td> <td class="center">13:20:00</td></tr></tbody></table>

 

M-FLARE: Today at 1318 UT, Earth-orbiting satellites detected an M1-class solar flare (SDO movie). The source is a new sunspot emerging over the sun's northeastern limb.

 

CORONAL HOLE: NASA's Solar Dynamics Observatory is monitoring a dark gash in the sun's atmosphere--a coronal hole. It's the dark vertical feature in this extreme UV image taken on Jan. 13th:​

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Coronal holes are places where the sun's magnetic field opens up and allows the solar wind to escape. This yawning hole is about 120,000 km wide and more than a million km long. Solar wind flowing from its UV-dark abyss will reach Earth on Jan. 16th or 17th, possibly sparking auroras for high-latitude sky watchers.

Coronal holes คือ พื้นที่ที่สนามแม่หล็กเปิดและทำให้พายุสุริยะเล็ดลอดออกมาได้ มันอ้าประมาณ กว้าง 120,000 กิโลเมตร และยาวถึง 1 ล้านกิโลมตร พายุสุริยะจะมาถึงโลกประมาณ 16-17 มกรา



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

 

ดาวเทียมรัสเซียตกมหาสมุทรอินเดียพรุ่งนี้

ดาวเทียมรัสเซียตกมหาสมุทรอินเดียพรุ่งนี้​

(14 ม.ค.) นายสุรพงษ์ โตวิจักษณ์ชัยกุล รัฐมนตรีว่าการกระทรวงการต่างประเทศ เปิดเผยว่า จากกรณีมีกระแสข่าวว่า ดาวเทียมของรัสเซียหลุดวงโคจรและมีแนวโน้มจะตกลงสู่พื้นโลก คาดว่าแถบประเทศอินเดีย บังกลาเทศ พม่า และไทยนั้น

ล่าสุดได้รับรายงานยืนยันจากทางการรัสเซียมาแล้วว่า ดาวเทียมโฟโบส-กรันท์ (Phobos-Grunt) จะตกลงสู่มหาสมุทรอินเดีย และจะไม่ทำให้ภาคพื้นดินได้รับความเสียหายแต่อย่างใด ดังนั้นในวันพรุ่งนี้ (15 ม.ค.) ประเทศไทย อาจจะเห็นเป็นเพียงลำแสงพุ่งผ่านแต่ไม่มีความเสียหายเกิดขึ้น และไม่มีการยิงจรวดจากประเทศใดๆ ทั้งสิ้นขอให้ประชาชนอย่าตกใจกับลำแสงดังกล่าว - สำนักข่าวไทย

ที่มา

 

Daily Sun: 15 Jan 12 <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> New sunspots 1401 and 1402 pose a threat for M-class solar flares. Credit: SDO/HMI
<table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> Sunspot number: 145

จุดดับพุ่งกระฉูด :boo:

 

ACTIVE SUNSPOTS: Crackling with C-class solar flares, a pair of active sunspots is emerging over the sun's northeastern limb. NASA's Solar Dynamics Observatory photographed the pair during the early hours of Jan. 15th:​

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These sunspots have the potential for strong eruptions. Sunspot 1401 produced an M1-flare on Jan. 14th. Two days earlier, while it was still on the farside of the sun, sunspot 1402 produced a partially-eclipsed flare of uncertain magnitude that created waves of ionization in the atmosphere over Europe.


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NOAA forecasters estimate a 30% chance of more M-flares during the next 24 hours. Solar flare alerts: text, voice.



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

 

<table cellpadding="0" cellspacing="0"><tbody><tr><td background="graphics/middle.jpg" width="25">
</td> <td background="graphics/back7.jpg" valign="top" width="540">
<table cellpadding="2" width="540"><tbody><tr><td background="graphics/back5.jpg" width="540"><center>Latest Solar News and Updates </center></td></tr></tbody></table> C-Class Solar Flares / Solar Update
01/16/2012 by Kevin VE3EN at 04:10 UTC
Comment on Message Board

Long Duration C-Class Flare: A long duration C6 class solar flare is in progress around Sunspot 1402 in the northeast quadrant. A Coronal Mass Ejection (CME) is now seen in the latest Lasco images, however it appears that it will be directed to the north and east. Stay tuned for more updates.

http://www.solarham.com/





</td></tr></tbody></table>
จุดดับ 1402 ระเบิดและมี CME มาทางโลก ออกไปทางเหนือและตะวันออก
ตอนนี้จุดดับ № 1402 N27 E64 อยู่ตรง 27 องศาเหนือ (ค่อนไปทางเหนือๆ ขึ้นไปจากไทย)

 

Solar wind
speed: 365.7 km/sec
density: 10.8 protons/cm³
explanation | more data
Updated: Today at 0523 UT

ความหนาแน่นของ proton เพิ่มขึ้นสูง

 

เรื่องเก่ามาเล่าใหม่

มาดูเรื่องจุดดับกัน

September 7, 2011

Diagram of the solar flare activity

X-ray emission of the Sun from 06.09.2011 to 07.09.2011 (GOES-15)


Solar flares today

Today, 3 solar flares were observed:

<table class="table_4" cellpadding="0" cellspacing="0" width="750"> <tbody><tr> <th width="1%"> </th> <th width="1%" align="left"> </th> <th>Active region</th> <th>Begin, UT</th> <th>Max, UT</th> <th>End, UT</th> </tr> <tr> <td nowrap="nowrap"></td> <td nowrap="nowrap" align="left">Flare of class C3.0</td> <td class="center">0</td> <td class="center">19:55:00</td> <td class="center">20:06:00</td> <td class="center">20:19:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td> </tr> <tr> <td nowrap="nowrap"></td> <td nowrap="nowrap" align="left">Flare of class C1.6</td> <td class="center">1283</td> <td class="center">22:13:00</td> <td class="center">22:18:00</td> <td class="center">22:26:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td> </tr> <tr> <td nowrap="nowrap"></td> <td nowrap="nowrap" align="left">Flare of class X1.8</td> <td class="center">1283</td> <td class="center">22:32:00</td> <td class="center">22:38:00</td> <td class="center">22:44:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td> </tr> </tbody></table>
Solar flares yesterday

Yesterday, 2 solar flares were observed:

<table class="table_4" cellpadding="0" cellspacing="0" width="750"><tbody><tr> <th width="1%"> </th> <th width="1%" align="left"> </th> <th>Active region</th> <th>Begin, UT</th> <th>Max, UT</th> <th>End, UT</th> </tr> <tr> <td nowrap="nowrap"></td> <td nowrap="nowrap" align="left">Flare of class M5.3</td> <td class="center">1283</td> <td class="center">01:35:00</td> <td class="center">01:50:00</td> <td class="center">02:05:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td> </tr> <tr> <td nowrap="nowrap"></td> <td nowrap="nowrap" align="left">Flare of class X2.1</td> <td class="center">1283</td> <td class="center">22:12:00</td> <td class="center">22:20:00</td> <td class="center">22:24:00</td></tr></tbody></table>
สังเกตว่า จุดดับ 1283 ที่จะทำให้เกิด x-class (ระเบิดระดับรุนแรง) ได้คือ มี Group's magnet type = Beta-Gamma-Delta

Sunspots and active regions

The following regions with sunspots can be now observed on the Sun's surface
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</td> </tr> <tr> <th width="1%"> Group number </th> <th width="10%"> Sunspots Location on the Sun </th> <th width="11%"> The number of spots in the group </th> <th width="20%"> The classification by the Zurich's modified system </th> <th width="30%"> Area (millions of shares of the solar hemisphere) </th> <th width="9%"> Group length (in degrees) </th> <th width="16%"> Carrington Longitude (in degrees) </th> <th class="last" width="1%"> Group's magnet type </th> </tr> <tr class="separator_1"> <td>
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</td> </tr> <tr> <td nowrap="nowrap"> № 1277 </td> <td> N18 W93 </td> <td class="center"> 01 </td> <td class="center"> Hsx </td> <td class="center"> 0060 </td> <td class="center"> 02 </td> <td class="center"> 299 </td> <td class="center"> Alpha </td> </tr> <tr class="separator_1"> <td>
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</td> </tr> <tr> <td nowrap="nowrap"> № 1281 </td> <td> S18 W51 </td> <td class="center"> 02 </td> <td class="center"> Bxo </td> <td class="center"> 0010 </td> <td class="center"> 03 </td> <td class="center"> 258 </td> <td class="center"> Beta </td> </tr> <tr class="separator_1"> <td>
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</td> </tr> <tr> <td nowrap="nowrap"> № 1283 </td> <td> N14 W18 </td> <td class="center"> 23 </td> <td class="center"> Eai </td> <td class="center"> 0200 </td> <td class="center"> 12 </td> <td class="center"> 224 </td> <td class="center"> Beta-Gamma-Delta </td> </tr> <tr class="separator_1"> <td>
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</td> </tr> <tr> <td nowrap="nowrap"> № 1287 </td> <td> S31 E25 </td> <td class="center"> 05 </td> <td class="center"> Cso </td> <td class="center"> 0100 </td> <td class="center"> 08 </td> <td class="center"> 181 </td> <td class="center"> Beta </td> </tr> <tr class="separator_1"> <td>
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</td> </tr> <tr> <td nowrap="nowrap"> № 1288 </td> <td> N19 E20 </td> <td class="center"> 01 </td> <td class="center"> Axx </td> <td class="center"> 0000 </td> <td class="center"> 00 </td> <td class="center"> 186 </td> <td class="center"> Alpha </td> </tr> <tr class="separator_1"> <td>
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</td> </tr> <tr> <td nowrap="nowrap"> № 1289 </td> <td> N24 E78 </td> <td class="center"> 01 </td> <td class="center"> Hsx </td> <td class="center"> 0190 </td> <td class="center"> 03 </td> <td class="center"> 129 </td> <td class="center"> Alpha </td> </tr> </tbody></table> Coordinates and other characteristics of active regions are issued for September 07, 2011 00:31 UT



Solar flares today

Today, 5 solar flares were observed:

<table class="table_4" cellpadding="0" cellspacing="0" width="750"><tbody><tr> <th width="1%"> </th> <th width="1%" align="left"> </th> <th>Active region</th> <th>Begin, UT</th> <th>Max, UT</th> <th>End, UT</th> </tr> <tr> <td nowrap="nowrap"></td> <td nowrap="nowrap" align="left">Flare of class C1.0</td> <td class="center">1302</td> <td class="center">02:46:00</td> <td class="center">02:52:00</td> <td class="center">02:58:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td> </tr> <tr> <td nowrap="nowrap"></td> <td nowrap="nowrap" align="left">Flare of class C7.7</td> <td class="center">1305</td> <td class="center">03:37:00</td> <td class="center">04:00:00</td> <td class="center">04:13:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td> </tr> <tr> <td nowrap="nowrap"></td> <td nowrap="nowrap" align="left">Flare of class C3.4</td> <td class="center">1307</td> <td class="center">18:42:00</td> <td class="center">18:47:00</td> <td class="center">18:53:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td> </tr> <tr> <td nowrap="nowrap"></td> <td nowrap="nowrap" align="left">Flare of class M1.0</td> <td class="center">1305</td> <td class="center">18:55:00</td> <td class="center">19:06:00</td> <td class="center">19:15:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td> </tr> <tr> <td nowrap="nowrap"></td> <td nowrap="nowrap" align="left">Flare of class C1.1</td> <td class="center">1302</td> <td class="center">20:37:00</td> <td class="center">20:42:00</td> <td class="center">20:48:00</td> </tr> <tr> <td colspan="6" style="height:8px;">
</td></tr></tbody></table>ถ้าเป็น Beta-Gamma ก็มีโอกาสเกิดระเบิดที่เป็นระดับปานกลาง M-Class ๆได้

เพราะฉะนั้นคาดว่าจุดดับใหญ่ 7 จุดที่พระอาจารย์รัตน์บอก น่าจะเป็นจุดดับที่มี Group's magnet type = Beta-Gamma-Delta

ดังนั้นเราต้องมาดูว่า ไอ้เจ้า Group's magnet type = Beta-Gamma-Delta เกิดขึั้นเมื่อไหร่พร้อมกัน 7 จุด ก็น่าจะเป็นสัญญาณบ่งบอกอะไรได้บ้างแล้ว