Visualizzazione archivio di domenica, 9 gennaio AM

Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2022 Jan 09 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 09 Jan 2022 until 11 Jan 2022
Brillamenti solari

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

Geomagnetism

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

Protoni solari

Quiet

10cm fluxAp
09 Jan 2022115016
10 Jan 2022120013
11 Jan 2022122004

Bulletin

Solar activity was at very low levels. NOAA Active Region 2924 (Catania group 1) produced low-level B-class flares. NOAA AR 2925 (Catania group 2) was stable. A new region near the central meridian (NOAA AR 2926 N30E02) began to emerge but is magnetically simple. A returning active region has rotated onto the solar disk (S10E75) and has been numbered NOAA AR2927. Solar activity is expected to be at low levels with C-class flares possible and a slight chance of an M-class flare.

No Earth directed Coronal Mass Ejections (CMEs) have been observed in the available coronagraph data.

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 2MeV electron flux exceeded the 1000 pfu threshold and is expected to be below this threshold over the next 24 hours. The 24h electron fluence was at normal to moderate levels and is expected to be at normal levels over the next 24 hours.

The solar wind parameters showed the arrival of the expected High Speed Stream (HSS) from 17 UT Jan 08. The total magnetic field magnitude oscillated reached 20 nT with an extended period of negative Bz from 17 to 21 UT. The interplanetary magnetic field phi angle switched from the positive sector to the negative sector (directed towards from the Sun). The solar wind speed gradually increased from around 310 to 560 km/s. The solar wind speed is expected to continue to be enhanced on Jan 09 and Jan 10, as the Earth remains under the influence of the HSS.

Geomagnetic conditions were mostly quiet to unsettled with two periods of minor storm conditions (NOAA Kp=5) from 18 UT, due to the enhanced negative Bz ahead of the arrival of the HSS. Geomagnetic conditions are expected to be mostly unsettled with possible active intervals on Jan 09 and Jan 10, due the HSS influence.

Today's estimated international sunspot number (ISN): 056, based on 18 stations.

Solar indices for 08 Jan 2022

Wolf number Catania///
10cm solar flux102
AK Chambon La Forêt032
AK Wingst022
Estimated Ap020
Estimated international sunspot number051 - Based on 12 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 geomagnetica2025/04/04Kp5+ (G1)
Giorni senza macchie
Ultimo giorno senza macchie2022/06/08
Media mensile Numero di Macchie Solari
marzo 2025134.2 -20.4
aprile 2025148 +13.8
Ultimi 30 giorni130.9 -15.2

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