Het archief bekijken van donderdag 13 oktober 2022

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2022 Oct 13 1231 UTC

SIDC Prognose

Zonnevlammen

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

Geomagnetisme

Quiet (A<20 and K<4)

Proton Flux monitor

Quiet

	10cm flux	Ap
13 Oct 2022	141	007
14 Oct 2022	138	007
15 Oct 2022	136	007

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.

Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 082, gebaseerd op 11 stations.

Zon indexen voor 12 Oct 2022

Wolfgetal Catania	///
10cm zonneflux	141
AK Chambon La Forêt	013
AK Wingst	007
Geschatte Ap	006
Geschat internationaal zonnevlekkengetal	099 - Gebaseerd op 18 stations

Overzicht opvallende gebeurtenissen

Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive

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