Space Weather Today
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Solar wind
speed: 593.3 km/sec
density: 0.23 protons/cm3
Updated: Today at 1051 UT

X-ray Solar Flares
6-hr max: M1 1726 UT May24
24-hr: M1 1726 UT May24
Updated: Today at: 2255 UT
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A SOLAR STORM AND THE PLEIADES: Before the launch of the Solar and Heliospheric Observatory (SOHO) in 1995, astronomers had never seen anything like this. Behold, a solar storm passing directly in front of the Pleiades:

https://spaceweather.com/images2023/24may23/pleaides_anim_strip2_opt2.gif

SOHO recorded this rare conjunction on May 21st. An erupting filament of magnetism near the sun's north pole propelled the CME into space just as the Seven Sisters were passing by. Electra, Taygete, Maia, Celaeno, Alcyone, Sterope, and Merope spent nearly three hours shining through the translucent solar storm.

When SOHO left Earth almost 30 years ago, it carried the first realtime coronagraph into space. Coronagraphs are devices that create an artificial eclipse, blocking the glare of the sun to reveal nearby stars, planets, and comets. No telescope on Earth could see something as faint as the Pleiades only a few degrees from the sun, but SOHO does it all the time.
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THE CALM BEFORE THE STORM? Giant sunspot AR3311 has been relatively calm for the past 48 hours. It might be the calm before the storm. The sunspot has an unstable 'beta-gamma-delta' magnetic field that harbors energy for strong X-class solar flares. NOAA forecasters estimate a 10% chance of an X-flare on May 24th.
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Solar wind
speed: 439.2 km/sec
density: 0.14 protons/cm3
Updated: Today at 0317 UT

X-ray Solar Flares
6-hr max: C2 1447 UT May27
24-hr: M1 2303 UT May26
Updated: Today at: 1520 UT
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FARSIDE SUNSPOT: There's a sunspot on the farside of the sun so large, it is affecting the way the whole sun vibrates. Helioseismic maps reveal the active region about 10 days away from turning toward Earth. This could herald a period of geoeffective solar activity in June.
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ELLERMAN BOMBS: At the beginning of the week, sunspot AR3315 didn't exist. Now it is the biggest and most dangerous sunspot on the solar disk. Maximilian Teodorescu photographed the fast-growing active region yesterday and found it crackling with bomb-blasts:

https://spaceweather.com/images2023/27may23/ebombs_strip.jpg

These are Ellerman bombs--magnetic explosions about one-millionth as powerful as true solar flares. A handful are circled above for reference. They are named after physicist Ferdinand Ellerman who studied the tiny blasts in the early 20th century. Of course, "tiny" is relative. A single Ellerman bomb releases about 1026 ergs of energy--equal to about 100,000 World War II atomic bombs.

Explosions like these are a sign of magnetic complexity in a sunspot. Opposite polarities bump together, reconnect, and--boom. A full-fledged flare may not be far behind.
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Solar wind
speed: 382.3 km/sec
density: 0.79 protons/cm3
Updated: Today at 0316 UT

X-ray Solar Flares
6-hr max: C2 1437 UT May29
24-hr: C2 0729 UT May29
Updated: Today at: 1520 UT
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Solar wind
speed: 383.0 km/sec
density: 1.68 protons/cm3
Updated: Today at 0817 UT

X-ray Solar Flares
6-hr max: C6 1650 UT May30
24-hr: M1 1338 UT May30
Updated: Today at: 2020 UT
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SUBSIDING CHANCE OF FLARES: Dangerous sunspot AR3315 became less dangerous today. Its magnetic field has decayed, losing the delta configuration that gave it potential energy for X-class solar flares. Lesser M-class flares are still possible, though, with NOAA estimating a 40%-chance of M-flares on May 30th.
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Solar wind
speed: 379.6 km/sec
density: 6.08 protons/cm3
Updated: Today at 0332 UT

X-ray Solar Flares
6-hr max: M1 1226 UT May31
24-hr: M1 0438 UT May31
Updated: Today at: 1535 UT
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MINOR GEOMAGNETIC STORM WATCH: NOAA forecasters say that minor G1-class geomagnetic storms are possible on June 2nd when a stream of solar wind is expected to hit Earth's magnetic field. The gaseous material is flowing from a pair of holes in the sun's atmosphere.
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