เหตุการณ์ใน-นอกโลก VS ภัยธรรมชาติ และupdate พายุสุริยะ

Terror threats rising as FEMA orders $1 Billion in dehydrated food

Terror threats appear to be on the rise as FEMA has rushed a $1 Billion order of dehydrated food in the event of attacks on domestic targets in the US.

อเมริกากลัวภัยคุกคาม สั่งอาหารแห้งกักตุน มูลค่า 1 พันล้านเหรียญ

จากการสังเกต จะเห็นว่ามีผู้ผลิตอาหารแห้งรายใหญ่ในประเทศ ได้ลดการส่งอาหารให้ลูกค้ารายย่อย เพื่อผลิตอาหารส่ง FEMA เป็นมูลค่าถึงหนึ่งพันล้านดอลล่าร์

หนึ่งในผู้ผลิตอาหารแห้ง รายใหญ่ของประเทศ ได้ตัดยอดส่งไปยังลูกค้าต่างๆ ถึง 99% ไม่ใช่เพราะว่าเศรษฐกิจไม่ดี แต่ะเป็นพราะว่าเค้าไม่สามารถผลิตให้กับลูกค้าได้พอ
ทำไมหล่ะ เพราะว่า ทุกอย่างในโรงงานต้องเอาไปผลิตให้กับออร์เดอร์ใหญ่ของรัฐบาล

แล้วพวกเรารู้ได้อย่างไร เมื่อต้นเดือนนี้ FEMA (The Federal Emergency Management Agency) ได้สั่งให้มีการซื้ออาหารแห้งไว้ หรือ ย่อยว่า (Request for Proposal หรือ REP คือ อาหารที่มีเพียงพอใน 10 วัน สำหรับ 14 ล้านคน) นั่นคือ 420 ล้านมื้อ ทำไมอยู่ดีๆ ก็มาเพิ่มเป็น 420 ล้านมื้อหล่ะ เหมือนราวกับว่าเค้าตุนอาหารคล้ายๆ กับวันของ เรือโนอาห์ ใช่ไหม?

ชาวบ้านคิดว่าคงเกี่ยวข้องกับการทหาร หรือจะมีการก่อการร้าย
และได้ออกมาบอกถึงว่าน่าจะมีการระวังตัวเกี่ยวกับสิ่งที่จะเกิดขึ้นกับพื้นดินในอนาคตอันใกล้ เหตุการณ์ที่เกิดขึ้นทั่วโลก เช่น ผู้ชุมนุม น้ำมันราคาสูง ดอลล่าร์ราคาตก อาหารขาดแคลน และพวกวิกฤตพวกนี้น่าจะเกิดขึ้นจากภายในประเทศหรือนอกประเทศได้ทั้งนั้น

This is also coming on the heels of one of the largest terror drills performed by the US Navy on American soil, as Operation Solid Curtain is taking place this week.

In an article Tuesday from the Beaufort Observer, many of the largest suppliers of dehydrated foods in the country are dropping their distributors and customers to dedicate their resources to supplying a billion dollar FEMA request and purchase.

One of the nation's largest suppliers of dehydrated food has cut loose 99% of their dealers and distributors. And it's not because of the poor economy. It's because this particular industry leader can no longer supply their regular distribution channels.

Why not? Because they're using every bit of manufacturing capacity they have to fulfill massive new government contracts. Look, the government has always been a customer of the industry to some extent. But according to our sources, this latest development doesn't represent simply a change of vendor on the government's part. It's a whole new magnitude of business.
And that's not all.


Apparently, even though they've cut off their regular consumer markets, the industry leader I've just mentioned still can't produce enough survival food to meet the government's vast requirements.

How do we know? Earlier this month, FEMA (the Federal Emergency Management Agency) put out a Request for Proposal, or RFP, for even more dehydrated food. The RFP called for a 10-day supply of meals - for 14 million people. That's 420 million meals. Typically, FEMA maintains a stockpile of about 6 million meals. Why the sudden need to increase the stockpile by 420 million more? (And that's in addition to whatever our aforementioned industry leader is supplying.) It almost seems like they're trying to stock a modern day "Noah's Ark," doesn't it?
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Single functions or events such as FEMA requesting a purchase of survival food might not stand out as peculiar when it is their responsibility to ensure they are mission ready for unforseen events in the US, but couple this with other pieces of the puzzle, such as the Navy drill of Solid Curtain, which is intended for:

...nationwide "drill" involving all military, and it's a drill based on a severe terrorist attack.
​

and the public had best be aware of something major potentially occurring on our soil in the near future. Global events across the world such as the revolutions and protests, the rising spike in oil, the falling dollar, food shortages, and unrest in Wisconsin and Ohio, are bringing us to the point where crisis may take place, whether from domestic or foreign sources.


Terror alerts have been raised by FEMA in the past month, and this new special order of dehydrated food, at the magnitude of $1 Billion dollars in taxpayer money, should be a call for everyone to prepare on your own for any potential crisis.

อ้างอิง
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หน่วยงานรับมือภัยฉุกเฉินสหรัฐสั่งอาหารแห้งมูลค่าหนี่งพันล้านดอล์ล่าร์

• 
• djmoder

สหรัฐเตรียมสั่งอาหารแห้งจำนวนมากถึงหนึ่งพันล้านเหรียญเตรียมรับมือกรณีฉุกเฉิน เกี่ยวกับก่อการร้าย? หรือภัยพิบัติ?
Terror threats rising as FEMA orders $1 Billion in dehydrated food - National Finance Examiner | Examiner.com
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อะไรที่กำลังพุ่งชนโลก

What's Hitting Earth?

March 1, 2011: Every day about 100 tons of meteoroids -- fragments of dust and gravel and sometimes even big rocks – enter the Earth's atmosphere. Stand out under the stars for more than a half an hour on a clear night and you'll likely see a few of the meteors produced by the onslaught. But where does all this stuff come from? Surprisingly, the answer is not well known.



Now NASA is deploying a network of smart cameras across the United States to answer the question, What's Hitting Earth?

Did that meteor you saw blazing through the sky last night come from the asteroid belt? Was it created in a comet's death throes? Or was it a piece of space junk meeting a fiery demise?


"When I get to work each morning and power up my computer, there's an email waiting with answers," says William Cooke, head of NASA's Meteoroid Environment Office. "And I don't have to lift a finger, except to click my mouse button."



A Southern Delta Aquarid fireball streaks over one of the network cameras in July 2010: movie.



Groups of smart cameras in the new meteor network triangulate the fireballs' paths, and special software¹ uses the data to compute their orbits and email Cooke his morning message.


"If someone calls me and asks 'What was that?' I'll be able to tell them. We'll have a record of every big meteoroid that enters the atmosphere over the certain parts of the U.S. Nothing will burn up in those skies without me knowing about it!"


In other U.S. meteor networks, someone has to manually look at all the cameras' data and calculate the orbits – a painstaking process.




The orbit of the Southern Delta Aquarid meteor (red) was a good match to that of the parent comet (blue).



"With our network, our computers do it for us – and fast," says Cooke.



The network's first three cameras, each about the size of a gumball machine, are already up and running. Cooke's team will soon have 15 cameras deployed east of the Mississippi River, with plans to expand nationwide². Cooke is actively seeking schools, science centers, and planetaria willing to host his cameras. Criteria are listed in the notes at the end of this story.


In addition to tracking fireballs and their orbits, Cooke's system gives him other valuable information.


"It provides data on meteor speed as a function of size – and this is critical to calibrating the models we use in designing spacecraft."


Meteorite hunters will reap benefits too. By determining a bright fireball's trajectory through the atmosphere, the network's software can calculate whether it will plunge to Earth and pinpoint the impact location fairly precisely.
"And when we collect the meteorite chunks, we'll know their

source. I could be holding a piece of Vesta in my hand.³ It would be like a free sample return mission!"


Opportunities like that, however, will be rare. "Most meteorites fall in the ocean, lakes, forests, farmer's fields, or the Antarctic," says Rhiannon Blaauw, who assists Cooke. "And the majority of those meteorites will never be found. But our system will help us track down more of them."




NASA's Smart Meteor Network is catching more than fireballs. In this movie, a bird stops to rest on one of the cameras in Georgia. Apparently, spiders like the cameras, too.



All cameras in the network send their fireball information to

Cooke and to a public website, fireballs.ndc.nasa.gov.



Teachers can contact Cooke at William.J.Cooke@nasa.gov to request teacher workshop slides containing suggestions for classroom use of the data. Students can learn to plot fireball orbits and speeds, where the objects hit the ground, how high in the atmosphere the fireballs burn up, etc.


Cooke gives this advice to students and others who want to try meteor watching on their own:
"Go out on a clear night, lie flat on your back, and look straight up. It will take 30 to 40 minutes for your eyes to become light adapted, so be patient. By looking straight up, you may catch meteor streaks with your peripheral vision too. You don't need any special equipment -- just your eyes."

 

ตอนนี้พายุสุริยะปาเข้้าไป 703.4 km/sec

<table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> Solar wind
speed: 703.4 km/sec
density: 0.1 protons/cm³
explanation | more data
Updated: Today at 0314 UT <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> X-ray Solar Flares
6-hr max: C1 1957 UT Mar01
24-hr: C6 0414 UT Mar01
explanation | more data
Updated: Today at: 2359 UT <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> Daily Sun: 01 Mar 11 <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> Growing sunspot 1164 (movie) has a complex "beta-gamma" magnetic field that harbors energy 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: 72
What is the sunspot number?
Updated 28 Feb 2011

Spotless Days
Current Stretch: 0 days
2011 total: 1 day (2%)
2010 total: 51 days (14%)
2009 total: 260 days (71%)
Since 2004: 820 days
Typical Solar Min: 486 days
Updated 28 Feb 2011

The Radio Sun
10.7 cm flux: 96 sfu
explanation | more data
Updated 28 Feb 2011
<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> Current Auroral Oval: ​

​

<table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/POES <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> Planetary K-index
Now: Kp=[FONT=Arial, Helvetica, sans-serif] 4 [/FONT] unsettled
24-hr max: Kp= 6 storm
explanation | more data
<table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> Interplanetary Mag. Field
B_total: 4.0 nT
B_z: 0.4 nT south
explanation | more data
Updated: Today at 0316 UT <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> Coronal Holes: 01 Mar 10 <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> A solar wind stream flowing from the indicated coronal hole should reach Earth on March 3rd or 4th. Credit: SDO/AIA. <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> <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td width="76%">SPACE WEATHER
NOAA Forecasts</td> <td valign="top" width="24%">

​

</td> </tr> </tbody></table> <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> Updated at: 2011 Mar 01 2200 UTC <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> <table height="80" width="100%" bgcolor="#FFFFF0" border="1" cellpadding="0" cellspacing="0"> <tbody><tr> <td width="40%">

FLARE​

</td> <td width="30%">

0-24 hr​

</td> <td width="30%">

24-48 hr​

</td> </tr> <tr> <td>

CLASS M​

</td> <td>

35 %​

</td> <td>

35 %​

</td> </tr> <tr> <td>

CLASS X​

</td> <td>

05 %​

</td> <td>

05 %​

</td> </tr> </tbody></table> <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> Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> Updated at: 2011 Mar 01 2200 UTC <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> Mid-latitudes <table height="100" width="100%" bgcolor="#FFFFF0" border="1" cellpadding="0" cellspacing="0"> <tbody><tr> <td width="40%">
</td> <td width="30%">

0-24 hr​

</td> <td width="30%">

24-48 hr​

</td> </tr> <tr> <td>

ACTIVE​

</td> <td>

30 %​

</td> <td>

30 %​

</td> </tr> <tr> <td>

MINOR​

</td> <td>

15 %​

</td> <td>

15 %​

</td> </tr> <tr> <td>

SEVERE​

</td> <td>

01 %​

</td> <td>

01 %​

</td> </tr> </tbody></table> <table width="100%" border="0" cellpadding="0" cellspacing="0"> <tbody><tr> <td></td> </tr> </tbody></table> High latitudes <table height="100" width="100%" bgcolor="#FFFFF0" border="1" cellpadding="0" cellspacing="0"><tbody><tr> <td width="40%">
</td> <td width="30%">

0-24 hr​

</td> <td width="30%">

24-48 hr​

</td> </tr> <tr> <td>

ACTIVE​

</td> <td>

40 %​

</td> <td>

40 %​

</td> </tr> <tr> <td>

MINOR​

</td> <td>

20 %​

</td> <td>

20 %​

</td> </tr> <tr> <td>

SEVERE​

</td> <td>

05 %​

</td> <td>

05 %​

</td></tr></tbody></table>

 

[FONT=Arial, Helvetica, sans-serif]GEOMAGNETIC STORM: [/FONT]A solar wind stream hit Earth's magnetic field during the early hours of March 1st, sparking a day-long magnetic storm that is subsiding but perhaps not over yet. In recent hours, spotters have reported auroras over Northern Ireland, Scotland, Latvia, Norway, and Sweden. High-latitude sky watchers in North America should be alert for green lights as night falls across their continent. Stay tuned! [Aurora alerts: phone, text]


NASA space physicist James Spann sends this picture from Poker Flats, Alaska, where he is attending a scientific conference to study auroras:

Photo details: Nikon D700 with 14-24mm lens at f/3.5, exposure of 25 seconds at 14 mm, ISO 1000​

"This is the first time I have seen the aurora borealis in person," says Spann who lives in Alabama. "It was fantastic--the greatest light show on Earth. It was cold (<-20 F) outside but worth every minute of exposure and lost sleep. I am afraid now that I have been ruined for life since my first personal viewing of the aurora was so amazing."


As a researcher he also appreciated the greater meaning of the display: "This is the most obvious and accessible evidence of the connectivity that Earth has with our star the sun. Witnessing the connectivity first-hand was particularly special to me."

 

เป็นไปได้อย่างสููง

 

Researchers Crack the Mystery of the Missing Sunspots

March 2, 2011: In 2008-2009, sunspots almost completely disappeared for two years. Solar activity dropped to hundred-year lows; Earth's upper atmosphere cooled and collapsed; the sun’s magnetic field weakened, allowing cosmic rays to penetrate the Solar System in record numbers. It was a big event, and solar physicists openly wondered, where have all the sunspots gone?
Now they know. An answer is being published in the March 3rd edition of Nature.
In this artistic cutaway view of the sun, the Great Conveyor Belt appears as a set of black loops connecting the stellar surface to the interior. Credit: Andrés Muñoz-Jaramillo of the Harvard CfA.

"Plasma currents deep inside the sun interfered with the formation of sunspots and prolonged solar minimum," says lead author Dibyendu Nandi of the Indian Institute of Science Education and Research in Kolkata. "Our conclusions are based on a new computer model of the sun's interior."

For years, solar physicists have recognized the importance of the sun's "Great Conveyor Belt." A vast system of plasma currents called ‘meridional flows’ (akin to ocean currents on Earth) travel along the sun's surface, plunge inward around the poles, and pop up again near the sun's equator. These looping currents play a key role in the 11-year solar cycle. When sunspots begin to decay, surface currents sweep up their magnetic remains and pull them down inside the star; 300,000 km below the surface, the sun’s magnetic dynamo amplifies the decaying magnetic fields. Re-animated sunspots become buoyant and bob up to the surface like a cork in water—voila! A new solar cycle is born.
For the first time, Nandi’s team believes they have developed a computer model that gets the physics right for all three aspects of this process--the magnetic dynamo, the conveyor belt, and the buoyant evolution of sunspot magnetic fields.
"According to our model, the trouble with sunspots actually began in back in the late 1990s during the upswing of Solar Cycle 23," says co-author Andrés Muñoz-Jaramillo of the Harvard-Smithsonian Center for Astrophysics. "At that time, the conveyor belt sped up."
The fast-moving belt rapidly dragged sunspot corpses down to sun's inner dynamo for amplification. At first glance, this might seem to boost sunspot production, but no. When the remains of old sunspots reached the dynamo, they rode the belt through the amplification zone too hastily for full re-animation. Sunspot production was stunted.
Sunspot cycles over the last century. The blue curve shows the cyclic variation in the number of sunspots. Red bars show the cumulative number of sunspot-less days. The minimum of sunspot cycle 23 was the longest in the space age with the largest number of spotless days. Credit: Dibyendu Nandi et al.

Later, in the 2000s, according to the model, the Conveyor Belt slowed down again, allowing magnetic fields to spend more time in the amplification zone, but the damage was already done. New sunspots were in short supply. Adding insult to injury, the slow moving belt did little to assist re-animated sunspots on their journey back to the surface, delaying the onset of Solar Cycle 24.
"The stage was set for the deepest solar minimum in a century," says co-author Petrus Martens of the Montana State University Department of Physics.
Colleagues and supporters of the team are calling the new model a significant advance.
"Understanding and predicting solar minimum is something we’ve never been able to do before---and it turns out to be very important," says Lika Guhathakurta of NASA’s Heliophysics Division in Washington, DC.
Three years ago on March 2, 2008, the face of the sun was featureless--no sunspots. Credit: SOHO/MDI

While Solar Max is relatively brief, lasting a few years punctuated by episodes of violent flaring, over and done in days, Solar Minimum can grind on for many years. The famous Maunder Minimum of the 17^th century lasted 70 years and coincided with the deepest part of Europe's Little Ice Age. Researchers are still struggling to understand the connection.
One thing is clear: During long minima, strange things happen. In 2008-2009, the sun’s global magnetic field weakened and the solar wind subsided. Cosmic rays normally held at bay by the sun’s windy magnetism surged into the inner solar system. During the deepest solar minimum in a century, ironically, space became a more dangerous place to travel. At the same time, the heating action of UV rays normally provided by sunspots was absent, so Earth’s upper atmosphere began to cool and collapse. Space junk stopped decaying as rapidly as usual and started accumulating in Earth orbit. And so on….
Nandi notes that their new computer model explained not only the absence of sunspots but also the sun’s weakened magnetic field in 08-09. "It's confirmation that we’re on the right track."
Next step: NASA’s Solar Dynamics Observatory (SDO) can measure the motions of the sun’s conveyor belt—not just on the surface but deep inside, too. The technique is called helioseismology; it reveals the sun’s interior in much the same way that an ultrasound works on a pregnant woman. By plugging SDO’s high-quality data into the computer model, the researchers might be able to predict how future solar minima will unfold. SDO is just getting started, however, so forecasts will have to wait.
Indeed, much work remains to be done, but, says Guhathakurta, "finally, we may be cracking the mystery of the spotless sun."
Credits: This research was funded by NASA’s Living With a Star Program and the Department of Science and Technology of the Government of India.

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

 

อ้างอิง

ไม่ลองไปดู ตำแหน่งดาว วันที่ 15 มีนาคม 2554 ด้วยหละครับ คล้ายๆ กันเลย ระดับ 9+ มาแน่ๆ




Posted by 3eye on Sun, 2011-02-27 14:19


กำลังเตรียมอยู่ครับ

โดยรวมคิดว่าคงจะมีอะไรรุนแรงเหมือนกันครับ โดยเฉพาะในช่วงปลายเดือนมีนาคม







Posted by Administration on Mon, 2011-02-28 09:33

 

น้ำมาเยอะเลย

 

[FONT=Arial, Helvetica, sans-serif]SUNSPOT SUNSET: [/FONT]The sun isn't blank any more. Just look at the sunset. Photographer Jens Hackmann sends this example from Weikersheim, Germany, on March 1st:


จุดดับของดวงอาทิตย์: พระอาทิตย์ไม่ได้ว่างๆ ต่อไปแล้ว เมื่อมองดูพระอาทิตย์ตก มีคนถ่ายได้ที่เยอรมันนี วันที่ 1 มีนา 11

​

"Because of high moisture in the air, the sunset was spectacular--and then it got even better," he says. "As the sun sank toward the treeline, sunspot 1164 popped into view." Hackmann's two-minute movie of the "sunspot sunset" is a [ame="http://www.youtube.com/watch?v=LFdRFp5yetQ"]must-see[/ame].

The primary dark core of sunspot 1164 is three times wider than Earth itself. This makes it an easy target for backyard telescopes equipped with solar filters. Moreover, the sunspot's magnetic field is unstable and harbors energy for X-class solar flares. The next sunspot sunset could be a lively one! Stay tuned.

จุดดับหลัก จุด 1164 มีความกว้างกว่าโลกเราสามเท่า ทำให้มันง่ายต่อการมองเห็นจากกล้องดูดาวหลังบ้าน และสนามแม่เหล็กของจุดดับไม่เสถียรและทำให้เกิดการระเบิดระดับ x จุดดับต่อไปอาจจะเป็นจุดมีชีวิตชีวาจับตาไว้ให้ดี

 

อ้างอิง



วันที่ 3 มีนาคม เราสังเกตเห็นแนว Active region และ จุุดดับ 1164 เข้ามาเรียงตัวกับโลกอย่างชัดเจน และยังมีการจำลองทิศทาง CME ที่เกิดจากวันที่ 2 มีนาคม ซึ่งดาดว่าจะถึงโลกในวันที่ 6 มีนาคม เวลาประมาณ 12-18 UTC

www.truth4thai.org/sites/default/files/CME Mar 2 11.gif

หมายเหตุ 12-18 UTC = ทุ่มหนึ่งถึงตีหนึ่งวันอาทิตย์ที่ 6 เมืองไทย

 

<table class="tbis" align="center" border="0" cellpadding="3" cellspacing="0" width="840"> <tbody><tr class="tbis1" bgcolor="#336699"><td width="20%" nowrap="nowrap">วัน-เวลา *ประเทศไทย</td> <td align="center" width="10%" nowrap="nowrap">ขนาด</td> <td align="center" width="10%" nowrap="nowrap">Latitude</td> <td align="center" width="7%" nowrap="nowrap">Longitude</td> <td align="center" width="13%" nowrap="nowrap">Phase</td> <td width="" nowrap="nowrap">บริเวณที่เกิด</td> </tr> <tr class="tbis3"> <td valign="top">2554-03-04 08:06:10</td> <td align="center" valign="top">2.3</td> <td align="center" valign="top">14.84</td> <td align="center" valign="top">99.13</td> <td align="center" valign="top">7</td> <td valign="top">บ้านนาสวน อำเภอศรีสวัสติ์ </td></tr></tbody> </table>

 

Sunspots + CME / RSS Feed Widget Box
03/03/2011 by Kevin VE3EN at 22:10 UTC
Comment on Message Board Solar Update - Sunspots continue to pop up in various locations on the sun. Currently Sunspot 1164 in the north and 1166 which rotated into view on the eastern limb remain the largest regions. A new sunspot that formed between 1164 and 1166 was numbered 1167. Several C-Class flares took place during the day on Thursday and there will continue to be a chance for an M-Class event.



Small CME - A small and possibly earth directed Coronal Mass Ejection (CME) is seen in the latest Lasco C2 movie. The latest SWPC update lists a slight chance for major geomagnetic storming at high latitudes by March 6.


CME อันเล็ก ที่ตรงมายังโลก สามารถมองเห็นได้จากดาวเทียม
มีโอกาสเล็กน้อยที่จะมี พายุแม่เหล็กโลกใหญ่ ที่ขั้วโลกเหนือ วันที่ 6 มีนานี้



RSS Feed Widget Box - Would you like to add a SolarCycle24.com RSS feed widget box to your website? M6MOF created one and you can find it HERE.



Sunspots (Thursday)

 

[FONT=Arial, Helvetica, sans-serif]FARSIDE ACTIVITY: [/FONT]This morning, March 4th, NASA spacecraft detected an explosion just behind the sun's eastern limb. STEREO-B recorded a flash of extreme UV radiation while SOHO observed a massive cloud billowing into space: movie. The blast was not Earth-directed, but future blasts could be as the active region turns toward our planet in the days ahead.

การระเบิดของพระอาทิตย์ด้านตรงกันข้ามกับโลก: วันที่ 4 มีนาคม ดาวเทียมได้ดักเจอการระเบิดของพระอาทิตย์ด้านที่ไกลจากโลก ตรงฝั่งตะวันออก. ดาวเทียม Stereo-B บันทึกถึง มีการส่งรังสี UV ออกมาอย่างมากๆ ขณะที่ ดาวเทียม SOHO สังเกตเห็นกลุ่มควันขนาดมหึมาพ่นออกมาในอวกาศ (ดูจากรุปด้านล่าง) แต่การระเบิดไม่ได้ตรงมาตรงโลก แต่ในอนาคตไม่แน่ เพราะว่าเจ้าจุดตรงที่ระเบิดใหญ่นี้มันต้องหันหน้ามาทางโลก ในไม่กี่วันข้างหน้านี้แล้ว