Viewing archive of Tuesday, 23 December 2025

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2025 Dec 23 1252 UTC

SIDC Forecast

Solar flares

C-class flares expected, (probability >=50%)

Geomagnetism

Minor storm expected (A>=30 or K=5)

Solar protons

Quiet

10cm fluxAp
23 Dec 2025135024
24 Dec 2025133026
25 Dec 2025131027

Solar Active Regions and flaring

Solar flaring activity was low over the past 24 hours, with only C-class flares identified. The largest flare was a C8.6 flare (SIDC Flare 6479) peaking on December 22 at 22:31 UTC, which was produced by SIDC Sunspot Group 735 (NOAA Active Region 4317). During the flare, the source region (SIDC Sunspot Group 735) of the flare had beta configuration of its photospheric magnetic field. A total of 7 numbered sunspot groups were identified on the disk over the past 24 hours. SIDC Sunspot Group 731 (NOAA Active Region 4316) has the most complex magnetic configuration (Beta-Gamma) and was growing over the past 24 hours. Solar flaring activity is expected to be low to moderate over the next 24 hours, with C-class flares expected and a chance for M-class flares.

Coronal mass ejections

A coronal mass ejection (CME) was observed on SOHO/LASCO-C2 images around 10:36 UTC on Dec 22, which is possibly asscoiated with a filament eruption around 09:00 UTC on the SE quadrant (S02 E37) of the Sun. It has a projected speed of about 400 km/s and a projected width of about 90 deg. A glancing blow, associated with this CME, may be expected at the Earth on Dec 25-26. No other Earth-directed CMEs were detected in the available coronagraph observations during last 24 hour.

Solar wind

Earth is still inside a fast solar wind stream, with the continuous arrival of high speed streams (HSSs) from the elongated, posiitve polarity, recurrent coronal hole (SIDC Coronal Hole 128) which started to cross the central meridian on Dec 20. The solar wind speed ranged from 620 km/s to 865 km/s. The interplanetary magnetic field ranged between 4 nT and 8 nT, and the North- South component (Bz) ranged betweeen -7 nT and 6 nT. In the next 24 hours, enhanced solar wind conditions are expected to continue with the further arrival of HSSs from the same coronal hole.

Geomagnetism

Geomagnetic conditions were globally at unsettled to minor storm conditions (NOAA Kp 3 to 5), and locally over Belgium at quiet to minor storm conditions (K BEL 2 to 5) during the past 24 hours, possibly as the result of the ongoing influence of high speed streams (HSS) from the southern, positive polarity, recurrent coronal hole (SIDC Coronal Hole 128). We expect unsettled to minor storm conditions (K 3 to 5) in the next 24 hours, possibly with the further arrival of HSSs from the same coronal hole.

Proton flux levels

The greater than 10 MeV GOES proton flux was below the threshold level over the past 24 hours and it is expected to remain so for the next 24 hours.

Electron fluxes at geostationary orbit

Over the past 24 hours, the greater than 2 MeV electron flux, as measured by GOES-18 satellite, exceeded above the 1000 pfu threshold level around 16:40 UTC on Dec 22, dropped below the threshold level arouond 03:00 UTC on Dec 23, and it is above threshold level since 09:20 UTC on Dec 23. The greater than 2 MeV electron flux, as measured by GOES-19 satellite, increased and exceed the threshold level from 14:40 UTC to 19:30 UTC on Dec 22. It was in response to the high speed streams (HSS) from the southern, positive polarity, recurrent coronal hole (SIDC Coronal Hole 128) which started to cross the central meridian from Dec 20. The electron flux is expected to remain above this alert level during most of the next period. The 24h electron fluence is presently at normal level, and it is expected to remain normal to moderate level in the coming 24 hours.

Today's estimated international sunspot number (ISN): 111, based on 03 stations.

Solar indices for 22 Dec 2025

Wolf number Catania///
10cm solar flux133
AK Chambon La Forêt038
AK Wingst029
Estimated Ap029
Estimated international sunspot number081 - Based on 09 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types
None

Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive

All times in UTC

<< Go to daily overview page

Latest news

Support SpaceWeatherLive.com!

A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!

No Ads on SWL Pro!
No Ads on SWL Pro! Subscriptions
Donations
Support SpaceWeatherLive.com! Donate
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Latest alerts

Get instant alerts!

Space weather facts

Last X-flare2026/07/04X1.3
Last M-flare2026/07/12M1.19
Last geomagnetic storm2026/07/04Kp7+ (G3)
Spotless days
Last 365 days3 days
20263 days (2%)
Last spotless day2026/02/24
Monthly mean Sunspot Number
June 202694.4 -7.1
July 202674.8 -19.6
Last 30 days87 -20.2

This day in history*

Solar flares
12002X2.61
22023M5.7
32000M4.77
42000M4.39
52002M3.24
DstG
11959-183G4
21961-105G4
31980-80G3
41991-78G1
51982-73G1
*since 1994

Aurora on this day in history

No observations submitted for this day in history. If you've observed the aurora and you have some amazing photos to show off, submit your observations now!
Submit your aurora observation

Social networks