Viewing archive of Monday, 26 September 2022

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2022 Sep 26 1310 UTC

SIDC Forecast

Valid from 1230 UTC, 26 Sep 2022 until 28 Sep 2022
Solar flares

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

Geomagnetism

Active conditions expected (A>=20 or K=4)

Solar protons

Quiet

10cm fluxAp
26 Sep 2022130010
27 Sep 2022129014
28 Sep 2022129007

Bulletin

Solar flaring activity was at low levels. The largest flare was a C4.7 flare, associated with Catania group 47 (NOAA AR 3107), peaking on September 26 at 09:11 UT. Other low level C-class flares were produced by Catania group 48 (NOAA active region 3110) and by Catania group 35 (NOAA active region 3102) from beyond the limb. Catania group 48 and Catania group 47 are the most complex region on disk. Solar flaring activity is expected to be at low levels, with C-class flares still likely and a remaining small chance for M-class flare from Catania group 48 and Catania group 47.

No new Earth directed Coronal Mass Ejections (CMEs) were detected in the available coronagraph imagery.

In the past 24 hours the greater than 10 MeV proton flux was very slightly enhanced but well below the minor storm warning threshold. The greater than 10 MeV proton flux is expected to remain below the radiation storm threshold over the next 24 hours. The greater than 2 MeV electron flux above the 1000 pfu threshold for a short period and is expected to cross the threshold again in the coming 24 hours. The 24h electron fluence was at normal to moderate levels over the past 24 hours. The 24h electron fluence is expected to increase to moderate levels in the next 24 hours.

Solar wind speed displayed a declining trend with values decreasing from 400-300 km/s. The interplanetary magnetic field had a magnitude of between 1 and 6.5nT and a minimum Bz of -4nT. Slow solar wind conditions are expected on September 26. From September 27, possible glancing blows from the September 23 CMEs may blend into the expected high speed stream expected from the extension of the southern polar coronal hole, which crossed the central meridian on September 23.

Geomagnetic conditions were quiet to (NOAA Kp 0-2, local K-Dourbes 0-2). Initially quiet to unsettled conditions are expected on September 26. Early September 27, active periods likely with the expected perturbed solar wind conditions.

Today's estimated international sunspot number (ISN): 122, based on 11 stations.

Solar indices for 25 Sep 2022

Wolf number Catania///
10cm solar flux135
AK Chambon La Forêt010
AK Wingst007
Estimated Ap006
Estimated international sunspot number129 - Based on 22 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 Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!

Donate SpaceWeatherLive Pro
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Latest alerts

Get instant alerts!

Space weather facts

Last X-flare2025/03/28X1.1
Last M-flare2025/04/01M2.5
Last geomagnetic storm2025/03/27Kp5 (G1)
Spotless days
Last spotless day2022/06/08
Monthly mean Sunspot Number
February 2025154.6 +17.6
April 2025147 -7.6
Last 30 days129.8 -18.9

This day in history*

Solar flares
12001X1.77
22017M8.35
31999M6.2
42001M3.57
52017M1.81
DstG
11979-168G4
21960-151G3
31992-105G2
42004-104G2
51994-103G3
*since 1994

Social networks