Marko Rummelsburg
@markorummelsburg.bsky.social
41 followers 96 following 200 posts
Polymath, Space Weather Enthusiast, Berlin ☞ raumwetter.de #AuDHD 🏳️‍🌈
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markorummelsburg.bsky.social
Active Region 4246 should be taken seriously now. It is still growing and magnetically complex. If this development goes on, X-flares and/or major CMEs seem possible.
markorummelsburg.bsky.social
M1.9 flare from region 4246 with type III radio burst. An associated CME with possible earth-directed components is visible in STEREO-A COR2
markorummelsburg.bsky.social
Synoptic map of the Sun showing filaments, two large coronal holes and sunspot groups – with 4246 and 4248 having the highest potential for solar flares and coronal mass ejections.
markorummelsburg.bsky.social
Two days development of active sunspot region 4246: Increasing size, number of spots and complexity combined with an unusual north-south orientation
markorummelsburg.bsky.social
STEREO A shows an earth-directed CME, a faint partial Halo visible in SOHO/LASCO C2, possible directions for the plasma from the dimming region south of 4246 and a 400 km/s CME listed in DONKI
markorummelsburg.bsky.social
The sun was busy today, but as far as i can tell, no earth-directed solar storms were launched…
markorummelsburg.bsky.social
Growth of active sunspot region 4246 – potential CMEs likely to be deflected northwards
markorummelsburg.bsky.social
East limb of the sun – foreground: old region 4220 (new 4249) - behind: old regions 4214/4217 – Can they still make a difference?
markorummelsburg.bsky.social
The sun today: Mostly quiet

(SDO AIA 171 Å + SDO HMI Magnetogram)
markorummelsburg.bsky.social
The solar synoptic map shows a quiet sun with only a few small sunspot groups and a large coronal hole that crossed the central meridian. Its fast solar wind may arrive in 2-4 days and lead to increased geomagnetic activity.
markorummelsburg.bsky.social
Synoptic map of the sun: many filaments, mainly simple sunspot groups (active regions) and a large coronal hole near the central meridian
markorummelsburg.bsky.social
Bipolar ‘anemone active region’ AR4243 within a large coronal hole (CH85-), surrounded by a ring-shaped filament. On the left side (in the east), you can see how the fast solar wind escapes and wobbles along the magnetic field lines.
markorummelsburg.bsky.social
Active Region 4242 (what a name!) in the southeast has the potential to become a significant solar flare player
markorummelsburg.bsky.social
Synoptic map of the sun: coronal holes, filaments, sunspot groups (active regions)
markorummelsburg.bsky.social
2025-10-03 0500z - M1.5 flare, 2 eruptions, 2 CMEs, one heading NE, one heading toward earth, likely arrival around Oct 6
markorummelsburg.bsky.social
Four very active regions in the northeast of the sun.
markorummelsburg.bsky.social
Solar Synoptic Map: New Active Regions, Many Filaments, Large Coronal Holes
markorummelsburg.bsky.social
Did you know that our sun can do that? Sympathetic flaring between -90° and +90° (SDO AIA 94, 131, 171 Å)