Visualizzazione archivio di mercoledì, 2 febbraio AM

Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2022 Feb 02 1247 UTC

SIDC Forecast

Valid from 1230 UTC, 02 Feb 2022 until 04 Feb 2022
Brillamenti solari

Quiet conditions (<50% probability of C-class flares)

Geomagnetism

Quiet (A<20 and K<4)

Protoni solari

Quiet

10cm fluxAp
02 Feb 2022129013
03 Feb 2022131012
04 Feb 2022130013

Bulletin

Solar activity was low over the past 24 hours. Active Region 2939 (Catania sunspot group 22, Mag. configuration: beta) has been most active, producing a C9.0 flare, peaking on Feb 01 22:23UT. This was associated with a dimming. Over the next 24 hours, C-class flares can be expected with a possibility of M-class flares and a slight chance of X-class flares.

Of the Coronal Mass Ejections observed, none is currently expected to have an Earth-directed component.

The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours, depending flaring activity. The greater than 2 MeV electron flux exceeded the 1000 pfu alert threshold on Feb 01 13:38UT, until 22:34UT. It is expected to remain about threshold in the next 24 hours. The 24h electron fluence was at moderate levels and is expected to be about moderate levels during the next period. Over the past 24 hours, a shock was detected in solar wind data on Feb 01 21:41UT, due to the arrival of the CME taking place on Jan 29 23:36UT. The solar wind speed jumped from 400 to 470 km/s. The magnetic field magnitude jumped from 5 to 12 nT. Bz attained a southward peak reaching -11nT. Since then, the total magnetic field has decreased to 8 nT while Bz has a value of +3nT. The solar wind speed has remained slightly enhanced. The interplanetary magnetic field phi angle was predominantly in the positive sector sector (directed way from the Sun), with slight variations associated with the impact of the CME. Over the next 24 hours, we expect that impact to dissipate further. An equatorial negative polarity coronal hole is at central meridian and the associated high speed stream can be expected Feb 05.

Geomagnetic conditions were quiet to unsettled over the past 24 hours, with an active period on Feb 02 00:00 to 03:00UT (NOAA Kp and K-BEL=4). Geomagnetic conditions are expected to be quiet to unsettled over the next 24 hours due to the expected CME influence.

Today's estimated international sunspot number (ISN): 077, based on 12 stations.

Solar indices for 01 Feb 2022

Wolf number Catania///
10cm solar flux129
AK Chambon La Forêt020
AK Wingst006
Estimated Ap006
Estimated international sunspot number083 - Based on 18 stations

Noticeable events summary

DayBeginMaxFineLocStrengthOP10cmCatania/NOAARadio burst types
Nessuna

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

Tutti gli orari in UTC

<< Vai alla pagina della panoramica giornaliera

Ultime notizie

Supporta SpaceWeatherLive.com!

Molte persone vengono su SpaceWeatherLive per seguire l'attività del Sole o sapere se ci sia la possibilità di vedere l'aurora, ma a maggior traffico corrispondono costi maggiori. Considerate una donazione se vi piace SpaceWeatherLive così che possiamo mantenere online il sito web!

Dona SpaceWeatherLive Pro
Supporta SpaceWeatherLive con il nostro merchandise
Dai un'occhiata al nostro merchandise

Notizie sul meteo spaziale

Ultimo brillamento X2025/03/28X1.1
Ultimo brillamento M2025/04/01M2.5
Ultima tempesta geomagnetica2025/03/27Kp5 (G1)
Giorni senza macchie
Ultimo giorno senza macchie2022/06/08
Media mensile Numero di Macchie Solari
marzo 2025134.2 -20.4
aprile 2025143 +8.8
Ultimi 30 giorni129.8 -16.3

Questo giorno nella storia*

Brillamenti solari
12001X1.21
22001M7.3
32001M4.52
42013M3.28
52004M2.47
DstG
11993-165G3
21968-112G3
31978-109G1
41984-108G2
51989-101G2
*dal 1994

Social networks