SOLAR WATCH: Activity On The Sun Is At Very High Levels - Sunspot 1890 Explodes With Major X1.1 Solar Flare And CME; Not Strongly Geo-Effective; Small Earth-Directed Component, Glancing Blow On November 11th!

<div style="text-align: justify;"><b><span style="color: yellow;">November 08, 2013 - SUN </span></b>- Solar activity is again at high levels with a major X1.1 solar flare detected around sunspot 1890 at 04:26 UTC.<br /><br /><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://1.bp.blogspot.com/-6df1TfyGJ8A/Un0pkv_QF3I/AAAAAAABNf4/W2tciDXyE3k/s1600/xflare01.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://1.bp.blogspot.com/-6df1TfyGJ8A/Un0pkv_QF3I/AAAAAAABNf4/W2tciDXyE3k/s1600/xflare01.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;">NASA's Solar Dynamics Observatory recorded a flash of extreme UV radiation from the blast site.</td></tr></tbody></table><br /><br /><span style="color: yellow;"><b>X1.1 SOLAR FLARE:</b></span> Big sunspot AR1890 is crackling with strong flares. The latest, registered X1 on the Richter Scale of Flares.  This sunspot has a signature: It tends to produce very brief flares. The X1-flare was no exception as it lasted barely a minute. Brevity mitigates Earth-effects, so this intense flare was not strongly geoeffective--at least, not at first.<br /><br /><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://4.bp.blogspot.com/-Hmrmf1iA980/Un0pw0TYSeI/AAAAAAABNgA/0xYXAwBUtl8/s1600/xflare02.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://4.bp.blogspot.com/-Hmrmf1iA980/Un0pw0TYSeI/AAAAAAABNgA/0xYXAwBUtl8/s1600/xflare02.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;">SDO captures the X1.1 solar flare around sunspot 1890 and the <br />coronal mass ejection (CME) associated with the event.</td></tr></tbody></table><br /><br />The event was associated with a 10cm Radio Burst (TenFlare) measuring 1000 sfu, along with Type II and IV sweep frequency events. A CME became visible in LASCO C3 imagery, following the explosion, and appears that a majority of the plasma was directed to the south. <br /><br /><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://2.bp.blogspot.com/-fDCSlwtc4YY/Un0q-HzCMCI/AAAAAAABNgU/_hx1IP36mMc/s1600/sunspot1890a.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://2.bp.blogspot.com/-fDCSlwtc4YY/Un0q-HzCMCI/AAAAAAABNgU/_hx1IP36mMc/s1600/sunspot1890a.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;">Massive sunspot 1890 is an easy target for solar telescopes and Ron Cottrell sends us this nice <br />Calcium-K (CaK) image he captured yesterday at the Kitt Peak Observatory in Arizona.</td></tr></tbody></table><br /><br />There may be a small Earth directed component and the latest CME tracking model released by the Goddard Space Flight Center is showing a glancing blow impact possible by November 11th, possibly sparking polar geomagnetic storms.  <br /><br /><br /><span style="color: lime;"><b>WATCH:</b></span> Major X-Class Solar Flare - November 8, 2013. <br /><div style="text-align: center;"><br /><br /><iframe allowfullscreen="" frameborder="0" height="321" src="https://www.youtube.com/v/S4haCXBX4j0?showinfo=0&version=3" width="570"></iframe></div><br /><br /><br />It should also be noted that sunspot 1891 generated a moderate M2.3 flare at 09:28 UTC this morning.<br /><br /><br />More eruptions are in the offing. NOAA forecasters estimate a 60% chance of M-class solar flares and a 20% chance of X-flares on Nov. 8th.<br /><br /><br /><span style="color: yellow;"><b>SUNSPOTS:</b></span> Below is an updated look at the visible solar disk on Friday. Sunspot 1890 remains the largest visible Earth facing region and retains a delta configuration within the trailing section of the group. The active region will be in a near perfect geoeffective position over the next 3 days and is likely that future eruptions would be at least partially Earth directed. <br /><br /><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://3.bp.blogspot.com/-x5dhUMFxCcM/Un0qzH2n-II/AAAAAAABNgM/RgJza7YdWCk/s1600/sunspots.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://3.bp.blogspot.com/-x5dhUMFxCcM/Un0qzH2n-II/AAAAAAABNgM/RgJza7YdWCk/s1600/sunspots.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;"><span class="userContent">Visible solar disk. </span></td></tr></tbody></table><br /><br />Sunspot 1891 continues to possess a weak delta configuration and produced a moderate M2.3 solar flare at 09:28 UTC Friday morning. A new sunspot rotated into view off the east limb and should be numbered 1893 today. It appears to be stable with a simple magnetic layout. There will remain a chance for another isolated moderate to strong solar flare within the next 24 hours with 1890 being the most likely source. <br /><br /><br /><span style="color: yellow;"><b>CORONAL HOLE:</b></span> <span class="dailySunCaptionText">Solar wind flowing from the indicated coronal hole could reach Earth on Nov. 10-11. <br /></span><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://3.bp.blogspot.com/-K6Nwfh0xMIE/Un0r5otUpoI/AAAAAAABNgg/hdKEHjjfe-w/s1600/coronalhole.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://3.bp.blogspot.com/-K6Nwfh0xMIE/Un0r5otUpoI/AAAAAAABNgg/hdKEHjjfe-w/s1600/coronalhole.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;"><span class="dailySunCaptionText">Credit: SDO/AIA. </span></td></tr></tbody></table><br /><br /><br /><br />SOURCES: <a href="http://www.spaceweather.com/"><span style="color: orange;"><b>Space Weather</b></span></a> | <a href="http://www.youtube.com/user/SolarWatcher?feature=watch"><span style="color: orange;"><b>Solar Watcher</b></span></a> | <a href="http://www.solarham.net/"><span style="color: orange;"><b>Solar Ham</b></span></a>.<br /><br /><br /></div>

Coronal Hole Coronal Mass Ejections Earthquakes Electric Universe Farside Region Filament Eruption Geomagnetic Storms Magnetic Fields Solar Eruptions Solar Flares Solar Watch Sun Sunspot 1890 SOLAR WATCH: Activity On The Sun Is At Very High Levels - Sunspot 1890 Explodes With Major X1.1 Solar Flare And CME; Not Strongly Geo-Effective; Small Earth-Directed Component, Glancing Blow On November 11th!

November 08, 2013 - SUN - Solar activity is again at high levels with a major X1.1 solar flare detected around sunspot 1890 at 04:26 UTC. NA...

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SOLAR WATCH: X3-Class Solar Flare Caused A Very Rare 'Magnetic Crochet' - Radiation Surge In The Ionization Of Earth's Upper Atmosphere Resulted In A Disturbance Of The Planet's Magnetic Field!

<div style="text-align: justify;"><b><span style="color: yellow;">November 07, 2013 - SUN </span></b>- On November 5th at 22:12 UT, the magnetic canopy of sunspot AR1890 erupted, producing a brief but intense <a href="http://www.spaceweather.com/glossary/flareclasses.html?PHPSESSID=ee7hdf8djak6haorfbqhqvo0f0">X3-class</a> solar flare. NASA's Solar Dynamics Observatory recorded the extreme ultraviolet flash:<br /><br /><br /><div class="separator" style="clear: both; text-align: center;"><a href="http://1.bp.blogspot.com/-R9CMKA54Xew/UnuVUsiMWLI/AAAAAAABNWo/XuBHGmmT-xI/s1600/xflare.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="http://1.bp.blogspot.com/-R9CMKA54Xew/UnuVUsiMWLI/AAAAAAABNWo/XuBHGmmT-xI/s1600/xflare.jpg" /></a></div><br /><br />Radiation from the flare caused a surge in the ionization of Earth's upper atmosphere--and this led to a rare magnetic crochet. Alexander Avtanski observed the effect using a homemade magnetometer in San Jose, California. A magnetic crochet is a disturbance in Earth's magnetic field caused by electrical currents flowing in air 60 km to 100 km above our heads. Unlike geomagnetic disturbances that arrive with CMEs days after a flare, a magnetic crochet occurs while the flare is in progress. They tend to occur during fast impulsive flares like this one.<br /><br />More eruptions are in the offing. NOAA forecasters estimate a 45% chance of M-class solar flares and a 10% chance of X-flares on November 7th. <br /><br />AR1890, one of the biggest sunspots of the current solar cycle, has turned almost directly toward Earth. This raises the possibility of geoeffective eruptions in the days ahead. NOAA forecasters estimate a 45% chance of M-class flares and a 10% chance of X-flares on November 7th. <br /><br /><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://2.bp.blogspot.com/-S4wPo_Erywc/UnuWmpcz9EI/AAAAAAABNW0/LxDCYaTOzok/s1600/sunspots.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://2.bp.blogspot.com/-S4wPo_Erywc/UnuWmpcz9EI/AAAAAAABNW0/LxDCYaTOzok/s1600/sunspots.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;">Visible Solar Disk.</td></tr></tbody></table><br /><br /><br />The Sun has erupted more than two dozen times over the past ten days, sending solar material and radiation through space.<br /><br />Scientists at NASA say more solar flares may be coming as Sun nears the highest peak of its 11-year activity rotation. The shooting radiation towards the Earth could potentially play havoc with global communications. <br /><br />Since October 23, the Sun has sent out 24 medium-strength M-class solar flares, and four X-class flares – the most powerful kind. As Sun is heading towards the peak of its 11-year cycle, a period known as the solar maximum, this should not be unusual. <br /><br />The solar flare that erupted on October 30, Friday was the fourth intense one the sun has emitted since October 23. According to NASA, October 23rd solar flare peaked at 5:54 p.m. ET. It was classified as a X2.3 class flare, big enough to disrupt satellites nearly 100 million miles away and more intense than the ones emitted the previous Friday. Those were classified at X1.7 and X2.1. <br /><br />These two solar flares were also the most intense kind emitted by the sun,that can cause a temporary radio blackout. The U.S. National Oceanic and Atmospheric Administration issued four radio blackout warnings during that time after solar weather suddenly turned turbulent. <br /><br />Radiation from solar flares cannot penetrate the atmosphere of the Earth to harm life on the ground, but when strong enough it can interrupt the atmosphere in the ionosphere, where GPS and radio signals travel. <br /><br />Solar flares occur when energy stored in magnetic fields twisted across the surface of the Sun is suddenly released. They can also cause aurora. Storms are rare during solar minimum, but as the sun nears solar maximum, large storms occur several times per year. <br /><br />The storm that was most intense between Oct. 29 and 31, 2003 caused some scary sun-spawned havoc both on the Earth and above it, officials with United States Geological Survey explained in a statement.<br /><br />SOURCES: <a href="http://www.spaceweather.com/"><span style="color: orange;"><b>Space Weather</b></span></a> | <a href="http://truthdive.com/2013/11/05/28-solar-flares-erupted-from-sun-in-a-week-more-on-the-way.html"><span style="color: orange;"><b>Truth Dive</b></span></a>.<br /><br /> <br /><br /></div>

Coronal Hole Coronal Mass Ejections Earthquakes Electric Universe Farside Region Filament Eruption Geomagnetic Storms Magnetic Fields Solar Eruptions Solar Flares Solar Watch Sun Sunspot 1890 SOLAR WATCH: X3-Class Solar Flare Caused A Very Rare 'Magnetic Crochet' - Radiation Surge In The Ionization Of Earth's Upper Atmosphere Resulted In A Disturbance Of The Planet's Magnetic Field!

November 07, 2013 - SUN - On November 5th at 22:12 UT, the magnetic canopy of sunspot ...

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SOLAR WATCH: Activity On The Sun Increases - Sunspot 1890 Erupts With Major X3.3 Solar Flare And Coronal Mass Ejection; THIRD LARGEST Event In Terms Of Peak X-Ray Flux During Solar Cycle 24; Impulsive Event Directed South And Away From Earth!

<div style="text-align: justify;"><span style="color: yellow;"><b><b><span style="color: yellow;">November 05, 2013 - SUN </span></b></b></span>- Earth-orbiting satellites have just detected an X3-class solar flare.<br /><br /><span style="color: yellow;"><b>X3.3 SOLAR FLARE:</b></span> A very rapid solar flare measuring X3.3 was detected around sunspot 1890 at 22:12 UTC. <br /><br />The event was accompanied by a 10cm Radio Burst (TenFlare) measuring 400 sfu and a Type II Sweep Frequncy Event with a velocity of 1380 km/s. <br /><br /><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://2.bp.blogspot.com/-1UliQM7zfvQ/UnmZKhYdUpI/AAAAAAABNIM/eOso-wO--lU/s1600/xflare01.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://2.bp.blogspot.com/-1UliQM7zfvQ/UnmZKhYdUpI/AAAAAAABNIM/eOso-wO--lU/s1600/xflare01.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;">NASA's Solar Dynamics Observatory recorded the extreme ultraviolet flash.</td></tr></tbody></table><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://1.bp.blogspot.com/-I8WV1ym2WBw/UnmZKlPSIcI/AAAAAAABNIQ/ufQuW-AcG_c/s1600/xflare02.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://1.bp.blogspot.com/-I8WV1ym2WBw/UnmZKlPSIcI/AAAAAAABNIQ/ufQuW-AcG_c/s1600/xflare02.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;"><span class="userContent">Attached image by the Solar Dynamics Observatory (SDO) captures an impusive X3.3 solar flare.</span></td></tr></tbody></table><br /><br /><span style="color: lime;"><b>WATCH:</b></span> Major X3.3 Solar Flare - November 5, 2013.  <br /><div style="text-align: center;"><br /><br /><iframe allowfullscreen="" frameborder="0" height="321" src="https://www.youtube.com/v/rk2BlkuEufQ?showinfo=0&version=3" width="570"></iframe></div><br /><br /><br />Although this flare was intense, it was also very brief. This will mitigate any Earth effects. For instance, any radio blackouts caused by ionization of Earth's upper atmosphere will likely be short-lived.<br /><br /><br /><div class="separator" style="clear: both; text-align: center;"><a href="http://3.bp.blogspot.com/-EfOIErAnnZ8/Unmf5q1w-VI/AAAAAAABNJY/P_Dn3THugP0/s1600/goes.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="http://3.bp.blogspot.com/-EfOIErAnnZ8/Unmf5q1w-VI/AAAAAAABNJY/P_Dn3THugP0/s1600/goes.jpg" /></a></div><br /><br />The X3.3 event comes in as the third (3rd) largest flare in terms of peak X-Ray flux during the current solar cycle 24. <br /><br /><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://1.bp.blogspot.com/-HiX9jlJ-cLg/UnmZyYbfg_I/AAAAAAABNIc/x6Y_CLyLhO0/s1600/xflare03.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://1.bp.blogspot.com/-HiX9jlJ-cLg/UnmZyYbfg_I/AAAAAAABNIc/x6Y_CLyLhO0/s1600/xflare03.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;"><span class="userContent">X3.3 solar flare. Image: SDO.</span></td></tr></tbody></table><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://1.bp.blogspot.com/-C22pDq5umAU/UnmZzD7kA1I/AAAAAAABNIk/O746rDOEgY0/s1600/xflare04.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://1.bp.blogspot.com/-C22pDq5umAU/UnmZzD7kA1I/AAAAAAABNIk/O746rDOEgY0/s1600/xflare04.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;"><span class="userContent">The major X3.3 solar flare was the third largest flare event in terms of peak X-Ray<br /> flux during the current Solar Cycle 24.</span></td></tr></tbody></table><br /><br /><span style="color: yellow;"><b>CME:</b></span> Although the event was very impulsive, a coronal mass ejection (CME) is now visible in the latest LASCO C2 imagery. So far it looks to be directed mostly towards the south and away from Earth. <br /><br /><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://2.bp.blogspot.com/-F-EyRaDZC0g/Unmed3MvttI/AAAAAAABNJQ/o3vJu5gtWrA/s1600/cme.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://2.bp.blogspot.com/-F-EyRaDZC0g/Unmed3MvttI/AAAAAAABNJQ/o3vJu5gtWrA/s1600/cme.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;"><span class="userContent"> Visible CME in the LASCO C2 image.</span></td></tr></tbody></table><br /><br /><b>ALERT:</b> Type II Radio Emission<br />Begin Time: 2013 Nov 05 2216 UTC<br />Estimated Velocity: 1380 km/s<br />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.<br /><br /><b>SUMMARY:</b> 10cm Radio Burst<br />Begin Time: 2013 Nov 05 2212 UTC<br />Maximum Time: 2013 Nov 05 2212 UTC<br />End Time: 2013 Nov 05 2214 UTC<br />Duration: 2 minutes<br />Peak Flux: 400 sfu<br />Latest Penticton Noon Flux: 149 sfu<br />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.<br /><br /><br /><span style="color: yellow;"><b>SUNSPOTS:</b></span> One of the biggest sunspots of the current solar cycle emerged over the sun's eastern limb three days ago and now it is turning toward Earth. <br /><br /><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://1.bp.blogspot.com/-ETUYR9o2Rzc/UnmbsfBVt6I/AAAAAAABNIw/Cav33UFfMK4/s1600/sunspots.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://1.bp.blogspot.com/-ETUYR9o2Rzc/UnmbsfBVt6I/AAAAAAABNIw/Cav33UFfMK4/s1600/sunspots.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;">Image: SDO/HMI</td></tr></tbody></table><br /><br />This movie from NASA's Solar Dynamics Observatory shows the approach of sunspot AR1890:<br /><br /><br /><br /><div class="separator" style="clear: both; text-align: center;"><a href="http://4.bp.blogspot.com/-BdCHcPzTAAk/UnmcQ3kO_SI/AAAAAAABNI4/voj7YRVGPXM/s1600/ar1890anim.gif" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="415" src="http://4.bp.blogspot.com/-BdCHcPzTAAk/UnmcQ3kO_SI/AAAAAAABNI4/voj7YRVGPXM/s640/ar1890anim.gif" width="570" /></a></div><br /><br /><br />AR1890 has an unstable 'beta-gamma-delta' magnetic field that harbors energy for strong explosions. NOAA forecasters estimate a 45% chance of M-class solar flares and a 10% chance of X-flares on Nov. 5th. <br /><br /><br /><span style="color: yellow;"><b>CORONAL HOLE:</b></span> <span class="dailySunCaptionText">Solar wind flowing from the indicated coronal hole could reach Earth on Nov. 7-8. </span><br /><br /><br /><table align="center" cellpadding="0" cellspacing="0" class="tr-caption-container" style="margin-left: auto; margin-right: auto; text-align: center;"><tbody><tr><td style="text-align: center;"><a href="http://2.bp.blogspot.com/-QHw6vFVvMiU/UnmcZZr_fLI/AAAAAAABNJA/WiErqjrBrEI/s1600/coronalhole.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><img border="0" src="http://2.bp.blogspot.com/-QHw6vFVvMiU/UnmcZZr_fLI/AAAAAAABNJA/WiErqjrBrEI/s1600/coronalhole.jpg" /></a></td></tr><tr><td class="tr-caption" style="text-align: center;"><span class="dailySunCaptionText">Image: SDO/AIA. </span></td></tr></tbody></table><br /><br /><br />Stay tuned for more updates.<br /><br /><br />SOURCES: <a href="http://spaceweather.com/"><span style="color: orange;"><b>Space Weather</b></span></a> | <a href="http://solarham.net/"><span style="color: orange;"><b>Solar Ham</b></span></a><a href="http://www.youtube.com/user/SolarWatcher?feature=watch"><span style="color: orange;"><b></b></span></a>. <br /><br /><br /><br /><br /></div>

Coronal Hole Coronal Mass Ejections Earthquakes Electric Universe Farside Region Filament Eruption Geomagnetic Storms Magnetic Fields Solar Eruptions Solar Flares Solar Watch Sun Sunspot 1890 SOLAR WATCH: Activity On The Sun Increases - Sunspot 1890 Erupts With Major X3.3 Solar Flare And Coronal Mass Ejection; THIRD LARGEST Event In Terms Of Peak X-Ray Flux During Solar Cycle 24; Impulsive Event Directed South And Away From Earth!

November 05, 2013 - SUN - Earth-orbiting satellites have just detected an X3-class solar flare. X3.3 SOLAR FLARE: A very rapid solar flare ...

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