The EUI telescope on Solar Orbiter is getting its first glimpses of the poles of the Sun.
SIDC News
The earth environment was under the influence of a solar wind stream from an equatorial coronal hole from 8 till 10 March.
Late on 24 February, a filament erupted from behind the Sun's southwest limb. This eruption was associated with a long-duration M-class flare, a minor proton event, and a truly impressive coronal mass ejection.
PROBA-3 took a snapshot of a star field – in the very first image captured by the mission’s coronagraph ASPIICS.
The STCE's SC25 Tracking page has been updated to reflect the latest evolution of some critical space weather parameters for the ongoing solar cycle 25 (SC25).
JSWSC has opened a new Topical Issue "Space Climate: Solar Extremes, Long-Term Variability, and Impacts on Earth's System".
From behind the northwest solar limb, NOAA 14001 produced an X2.0 flare on 23 February.
The fleet of solar satellites recorded several impressive solar eruptions and CMEs during the first few days of February.
Preliminary, non-operational images of the GOES-19 coronagraph CCOR-1 are available at the NOAA/SWPC's testbed, in anticipation of GOES-19 becoming fully operational on 4 April.
From 28 January onwards, a cluster of sunspots started to rotate over the northeast solar limb. It was responsible for several medium-sized solar flares.
A million km long filament has been transiting the solar disk during the last 2 weeks.