Space weather only #AuDHD https://xitter.cf/t.co/oLIp56qfhZ

Berlin
Joined February 2011
Three sunspot groups, some magnetic flux is emerging; still a chance of isolated M-class flares…
Solar Synoptic Map - 3 active regions on the visible solar disk: 4560 simple bipolar; 4557 slowly growing, quite stable; 4551 confined M1.68 solar flare ≈0900 UTC, no CME ('solar storm') - coronal hole CH04+: elevated chances of aurora from 19 Oct, SWPC: G1 watch 19/20 Oct
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Solar Synoptic Map - 3 active regions on the visible solar disk: 4560 simple bipolar; 4557 slowly growing, quite stable; 4551 confined M1.68 solar flare ≈0900 UTC, no CME ('solar storm') - coronal hole CH04+: elevated chances of aurora from 19 Oct, SWPC: G1 watch 19/20 Oct
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A solar filament dissipated without erupting
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A filament (or prominence) eruption occurred early on 17 October 2026 UTC day at/behind the southeastern limb of the Sun. Quite a large CME ('solar storm', not heading towards Earth) was produced. (SDO AIA 304, AIA 171, AIA 193 Running Difference)
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The Sun in extreme ultraviolet (AIA, SDO satellite) - region 4551 (S) looks stable - ongoing flux emergence in region 4557 (N) - wobbly filament north of 4551 - (+) polarised coronal hole crossed the central meridian
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Region 4551 recorded in Nagoya, i assume with H-alpha filter, very pretty with many small flares and a dense filament connecting the leading and trailing section.
10/15 名古屋の太陽 動画編(81/288) AR4551付近。小規模ながら11:07にC2.9, 11:17にC1.9のフレアが発生しています。10:26~1分間隔 120分間 30fps 全球動画から切り取り
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Slowly growing sunspot groups 4557 (N) and 4451 (S) with some low level C-class flare activity (SDO HMI, SDO AIA 94, PFSS field lines, GOES X-ray flux long)
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Streamer Blowout a.k.a. Balloon CME from the southwestern limb of the Sun. The streamer is generated by a large negative coronal hole in the southern hemisphere and the positively polarised coronal hole near the south pole of the Sun.
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A positively polarised coronal hole is approaching the central meridian of the Sun. That could mean there is an Increased chance of aurora in a week or so, especially at higher latitudes.
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Growing sunspot group 4551 is showing increasing complexity and an increasing risk for stronger solar flares.
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A large filament is lifting off on the Sun’s northern hemisphere. Most likely, the associated CME ('solar storm') is not earth-directed. (SDO AIA 304, SDO AIA 171/193/211 tricolor base difference)
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Crazy filament launch just now from the Sun's northern hemisphere. This isn't Earth directed, but wow how about some eye candy this morning! Super pretty stuff.
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Solar Synoptic Map - W ➡️ half of the ☀️ disk dominated by (–) polarised coronal holes - connection to 1 of them, ≈600 km/s near 🌎 - limited geoeffectiveness: wrong polarity - sunspot group 4551: new spot 👀 - new spots in NE ↖️ 👀 - waiting for filament eruptions ☀️->🌎
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Another possibly earth-directed filament eruption occurred on the southern hemisphere of the Sun. (SDO AIA 304, SDO AIA 171/193/211 tricolor base difference, GOES X-ray flux long, e-Callisto radiogram)
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Large filament eruption north of the large southern coronal hole. Possibly earth-directed. We'll have to wait for coronagraph imagery…
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CCOR1 looks promising with one shock to the east but also one to the west, possibly caused by the area that produced the fast CME that hit us recently
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2026-10-10: Coronal mass ejection towards NW↗️ after M6.4 solar flare with fast earth-directed shock (360° halo, 1500 km/s). Shock arrival possible late on 11 October, early on 12 October (UTC day), uncertain. CME core will only graze or rather miss us.
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With a current plasma density of < 1 p/ccm near earth there is hardly any material that could be shocked
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Marko Rummelsburg retweeted
A decent aurora tonight here in Pilsen region, Czechia 💃
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