Solar atmosphere constantly changes. The changes could be large as during the last week M-class flare, or they could be relative small. Watch filament near the North polar region (upper part of image) slowly rising and then erupting. LASCO coronagraphs do not seem to show a clear signature of a CME eruption associated with this partial filament eruption.
Subscribe to:
Post Comments (Atom)
GONG operations during U.S. government shutdown
During U.S. government shutdown, GONG will continue regular operations. The data will be provided both for the operational space weather f...
-
GONG/Learmonth (Australia) took observations of a large two-ribbon flare, which was the source of Earth-directed halo Coronal Mass Ejectio...
-
Here is the road timeline (as of 28-Mar-2025): 1. RFP released from DOT to the 2 down-selected and qualified vendors: Mid-April 2. Bids b...
-
The 246th AAS meeting (joint with the Laboratory Astrophysics and Solar Physics Divisions) took place the of week 8-12 June 2025 in Anchorag...
No comments:
Post a Comment