Visualizzazione archivio di domenica, 29 agosto AM

Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2021 Aug 29 1257 UTC

SIDC Forecast

Valid from 1230 UTC, 29 Aug 2021 until 31 Aug 2021
Brillamenti solari

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

Geomagnetism

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

Protoni solari

Quiet

10cm fluxAp
29 Aug 2021091008
30 Aug 2021091016
31 Aug 2021090008

Bulletin

During last 24 hours six B-class and three C-class flares were reported. The strongest reported flare was the C8.1 flare (peaked at 10:03 UT this morning) originating from the Catania sunspot group 32 (NOAA AR 2860) which is maintaining the beta-gamma configuration of its photospheric magnetic field. We expect similar level of the flaring activity to continue in the coming hours. From the presently available data it is not clear if the C8.1 flare was associated with the wide CME. More will be reported when data become available. The large filament eruption from the northern hemisphere (at about 15:00 UT on August 28) and close to the central meridian does not seem to be associated with the CME observed in the presently available coronagraph data. The CME associated with that filament eruption would be possibly Earth directed. The M4.7 flare (peaked at 06:11 UT on August 28) was associated with the partial halo CME (first time seen in the SOHO/LASCO C2 field of view at about 07:48 UT) that could arrive to Earth on September 2.

The greater than 10 MeV proton flux was at background levels and we expect it will remain so in the next 24 hours. The greater than 2 MeV electron flux crossed the 1000 pfu threshold at about 03:20 UT today and it is above the threshold since then. We expect such level to remain in the coming hours. The 24h electron fluence is at moderate levels and we expect it will stay so in the coming 24 hours.

The solar wind speed is presently about 390 km/s and the interplanetary magnetic field magnitude is about 2 nT. In the morning of August 30 we can expect arrival of the halo CME (first observed in the SOHO LASCO C2 field of view at about 19:00 UT on April 26) that could induce active geomagnetic conditions. During last 24 hours the geomagnetic conditions were unsettled to quiet. We can expect such a geomagnetic conditions to persist in the coming hours.

Today's estimated international sunspot number (ISN): 047, based on 14 stations.

Solar indices for 28 Aug 2021

Wolf number Catania///
10cm solar flux090
AK Chambon La Forêt013
AK Wingst017
Estimated Ap018
Estimated international sunspot number070 - Based on 25 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 giorni130.4 -16.1

Questo giorno nella storia*

Brillamenti solari
12002M8.82
21999M6.76
32001M2.91
42003M2.74
52001M2.31
DstG
11979-202G3
21988-133G3
31984-120G4
42004-117G2
51994-111G3
*dal 1994

Social networks