Tag Archives: Solar Flares

Solar Flare

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SOLSTICE SOLAR FLARE: This morning, June 21st at 03:16 UT, the sun itself marked the solstice with an M2-class solar flare from sunspot AR1777. NASA’s Solar Dynamics Observatory photographed the extreme ultraviolet flash and a plume of material flying out of the blast site:

As sunspots go, AR1777 is neither large nor apparently menacing, yet it has been crackling with flares for days. Before it rotated over the sun’s eastern limb on June 20th, it unleashed a series of farside flares and CMEs. Today’s explosion was not Earth directed, but future explosions could be as the sun’s rotation continues to turn AR1777 toward our planet. NOAA forecasters estimate a 30% chance of M-flares and a 5% chance of X-flares during the next 24 hours.

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6/5 Solar Activity

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SOLAR FLARE AND CME: Southern sunspot AR1762 erupted today, June 5th, producing a long-duration M1-class solar flare that peaked around 0900 UT. The explosion hurled a right coronal mass ejection (CME) into space, shown here in a coronagraph image from the Solar and Heliospheric Observatory:

Because the sunspot is approaching the sun’s southwestern limb, the blast was not squarely Earth-directed. In fact, it might miss us altogether. Stay tuned for further analysis of the trajectory of the CME.

Meanwhile, more eruptions could be in the offing. AR1762 has a ‘beta-gamma-delta’ magnetic field that harbors energy for X-flares much stronger than the M1-class event that occured this morning.

fr/spaceweather.com

Two New Sunspots

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TWO NEW SUNSPOTS: On Friday they didn’t exist. On Saturday they are big sunspots. Today, sunspots AR1726 and AR1727 are rapidly emerging in the sun’s northern hemisphere. The larger of the two, AR1726, contains nearly a dozen dark cores and spans 125,000 km from end to end. Click to view a 24-hour movie recorded by NASA’s Solar Dynamics Observatory:

AR1726 is the fastest-growing and, so far, the most active. It is crackling with C-class flares and seems capable of producing even stronger M-class eruptions. Because of the sunspot’s central location on the solar disk, any explosions this weekend will be Earth-directed.

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On Budding Sunspots

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VERY SPOTTED SUN: Solar activity is still relatively low, but the appearance of the sun suggests the quiet might not last. Over the weekend, a profusion of new sunspot groups peppered the solar disk with dark cores–each one a potential source of eruptions. NOAA forecasters estimate a 35% chance of M-class flares and a 5% chance of X-flares during the next 24 hours. Solar flare alerts: text, voice.

There are so many spots on the sun, even a jumbo jet cannot hide them:

Raffaello Lena took the picture on January 5 not far from the international airport in Rome, Italy. “An animation of the flyby is available here,” he says.

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More Solar Eruptions

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SLOW ERUPTION: The magnetic canopy of a sunspot group just over the sun’s southwestern limb slowly erupted on Oct. 28th. When the hours-long eruption was over, this bright arcade formed over the blast site, marking the location where the explosion occured:

Arcade loops appear after many solar flares. It is how the magnetic fields of sunspots settle down after a significant eruption. This particular eruption hurled a massive CME into space, but Earth was not in the line of fire.

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The SUn’s Magnetic Froth

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MAGNETIC FROTH: Sunspot AR1598 has quieted down since unleashing an X1-class solar flare on Oct. 23rd. It might be the calm before the storm. The sunspot is still large and apparently potent, as shown in this image captured by amateur astronomer Sergio Castillo of Inglewood,California:

Castillo used a telescope capped with a “Calcium K” filter tuned to the light of ionized calcium atoms in the sun’s lower atmosphere. Calcium K filters highlight the bright magnetic froth that sometimes forms around a sunspot’s dark core. AR1598 is very frothy indeed.

Magnetic froth does not necessarily herald an explosion, but it does guarantee a photogenic sunspot

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Ongoing Geo-Magnetic Storm

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GEOMAGNETIC STORM UNDERWAY: A G1-class geomagnetic storm is underway on Oct. 13th. Reports of bright auroras have been received from Scandinavia, Greenland, Canada and several northern-tier US states. Colin Chatfield sends this picture from Saskatoon, Saskatchewan:

“This is from my backyard around 5:00a.m. this morning,” says Chatfield. “Never have I seen the auroras so bright, especially from within the city. They were astounding, with purple visible to the naked eye.”

The ongoing storm was triggered by a knot of south-pointing magnetism from the sun. During the early hours of Oct. 13th, the knot bumped into Earth’s magnetic field, opening a crack in our planet’s magnetosphere. Solar wind poured in to fuel the auroras.

More auroras are in the offing. NOAA forecasters estimate a 40% chance of strong polar geomagnetic storms on Oct. 14th when a solar wind stream is expected to blow past Earth

from:    spaceweather.com

New Sunspot Activity

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ADVANCING SUNSPOTS: For the past two weeks, solar activity has been relatively low. Now, a change is in the offing. The farside of the sun is peppered with sunspots, and some of them are beginning to turn toward Earth. NASA’s Solar Dynamics Observatory photographed this pair of active regions advancing over the eastern limb during the early hours of Oct. 11th:

Underlying each nest of glowing magnetic loops is a dark sunspot that poses a threat for solar flares. NOAA forecasters estimate a 40% chance of M-class solar flares and a 5% chance of X-flares during the next 24 hours.

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