Viewing archive of Thursday, 13 October 2022

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2022 Oct 13 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 13 Oct 2022 until 15 Oct 2022
Solar flares

M-class flares expected (probability >=50%)

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
13 Oct 2022141007
14 Oct 2022138007
15 Oct 2022136007

Bulletin

There are four active regions on the visible disc. The X-ray background is on the C-level. NOAA AR 3112 produced an M1.5 flare peaking at 00:19 UT. More M-class flares can be expected for the next 24 hours.

No Earth-directed coronal mass ejections (CMEs) were detected in the available coronagraph imagery over the past 24 hours.

The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux was above the 1000 pfu threshold but has decreased below it in the last hours. It is expected to remain so in the coming 24 hours. The 24h electron fluence was at moderate levels in the past 24 hours and is expected to remain so in the next 24 hours.

The solar wind speed at the Earth has decreased in the last 24 hours to about 310 km/s. The interplanetary magnetic field magnitude has been around 5 nT. In the next 24 hours, similar conditions are expected.

Geomagnetic conditions were quiet to unsettled (Kp up to 2 and K_Dourbes up to 3). Similar conditions are expected for the next 24 hours.

Today's estimated international sunspot number (ISN): 082, based on 11 stations.

Solar indices for 12 Oct 2022

Wolf number Catania///
10cm solar flux141
AK Chambon La Forêt013
AK Wingst007
Estimated Ap006
Estimated international sunspot number099 - Based on 18 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types
12235400190037----M1.555/3112

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

All times in UTC

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