Monday, 24 June 2013

M2.9 Class Solar Flare Geomagnetic Storm HD

  


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Solar activity has been moderate with most activity detected around Sunspot 1778. This region is showing signs of growth and was responsible for an impulse M2.9 flare June 21st and again June 23 at 20:56 UTC Sunday evening and a C9.9 flare this morning at 11:32 UTC. All other regions remain fairly stable. Sunspot 1773 decayed to a spotless plage. Sunspots 1772 and 1776 continue to make their way towards the west limb. There will remain a chance for C-Class flares and perhaps another isolated M-Class event.
You can also visit me on my facebook at https://www.facebook.com/trudi.t.kay
Have a good day and thank you for watching.

Thursday, 6 June 2013

06 06 2013 The Best Solar Magnetic Tornado Observed HD

  
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This is one of the best solar tornadoes I have observed. SDO/NASA captured at various infrared 304 Ã…ngstrom. 171- 193 et al beginning June 3 to present June 6th 2013.
It is earth directed so whatever shock wave it will produce it is highly possible we will get a glancing blow around the 8th of June.
The auroras created from the shockwave should be beautiful as well as any possible sounds that are produced as the shockwave interacts with our geomagnetosphere causing a geomagnetic storm..
You all have a good week and weekend ahead and hope you catch some good aurora viewing.

Monday, 3 June 2013

A Special Presentation Geomagnetic/Radioactive Storms - 06 03 2013 HD




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On June 2nd at a high-speed (700 km/s) solar wind stream buffets Earth's magnetic field. The warning comes on the heels of a lengthy G2-class geomagnetic storm on May 31- and again June 1 sparked by the arrival of an interplanetary shock wave. The source of the shock is unknown. Although I do suspect it is from the coronal holes themselves. Current speculation focuses on a corotating interaction region (CIR)--that is, a shock-like transition zone between high- and low-speed solar wind streams. Whatever it was, the impact ignited some beautiful auroras,

June 1st, Northern Lights spilled across the Canadian border into more than a dozen US states, turning the sky purple and green as far south as Colorado and Nebraska. Subscribers to the Space Weather Alert System knew the storm was coming, but others were surprised:
Aurora Over Crater Lake National Park, OR
Taken by Brad Goldpaint on June 1, 2013 @ Crater Lake National Park, OR
Aurora
Taken by Robert Farrimond on May 31, 2013 @ Vantage, Washington

As solar maximum nears its peak we are anticipating whatever our heightened imagination can visualize.

Here is a little preview of the magnetic storm, solar flares at immense speed racing towards earth we can expect.

In which this event actually happened not too long ago last year in March 2012 with a CME at class M.8 (Understanding the Geomagnetic Storm)

more:  May/June 2013 Geomagnetic Storm Flareup

Tuesday, 14 May 2013

Solar Cycle 24 Delivers a Class X3.2 CME HD

  



The most powerful flare to date - Solar Maximum does not disappoint.
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Update from yesterdays class X1.7 and class X2.8 coronal ejection.
All other visible sunspot regions appear to be stable at this time. There will remain a chance for moderate M-Class solar flares and perhaps another isolated X-Class event within the next 24-48 hours, particularly around Sunspot 11748.

Monday, 13 May 2013

Class X1.7 & Class X2.8 CME ALERTS HD

  


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A sunspot on the sun's eastern limb is crackling with powerful X-class solar flares. It announced itself with an X1.7-class eruption on May 13th at 0217 UT, quickly followed by an X2.8-class flare at 1609 UT. These are the strongest flares of 2013, and they signal a significant uptick in solar activity. More eruptions are in the offing.
 ALERT: Type II Radio Emission
Begin Time: 2013 May 13 1557 UTC
Estimated Velocity: 949 km/s
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.

ALERT: Type IV Radio Emission
Begin Time: 2013 May 13 1557 UTC
Description: Type IV emissions occur in association with major eruptions on the sun and are typically associated with strong coronal mass ejections and solar radiation storms.

SUMMARY: 10cm Radio Burst
Begin Time: 2013 May 13 1553 UTC
Maximum Time: 2013 May 13 1601 UTC
End Time: 2013 May 13 1618 UTC
Duration: 25 minutes
Peak Flux: 520 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.

Sunday, 5 May 2013

Class M5.7 CME - M1.3 Flare Solar Magnetic Tornado HD



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Sunspot group AR1739, just now emerging over the sun's northeastern limb, erupted on May 3rd, producing an M5-class solar flare and a "solar tornado."  watch the plasma twist.
The explosion also hurled a bright coronal mass ejection (CME) into space:  Traveling almost 1300 km/s, the electrified cloud is expected to sweep past a couple of NASA spacecraft (EPOXI and Spitzer) on May 7th. No planets, however, were in the line of fire

Thursday, 2 May 2013

Class M1.1 CME and class C9.6 CME MONSTER FARSIDE ERUPTION HD



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Solar activity is now at moderate levels thanks to an isolated M1.1 Solar Flare around Sunspot 1731 in the northern hemisphere. A Coronal Mass Ejection (CME) is visible in the latest STEREO Ahead COR2 imagery. It appears that a majority of the plasma cloud was directed north of the Sun-Earth field.
Auroras this weekend.