Visualizzazione archivio di venerdì, 20 settembre AM

Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2024 Sep 20 1231 UTC

SIDC Forecast

Brillamenti solari

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

Geomagnetism

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

Protoni solari

Quiet

10cm fluxAp
20 Sep 2024160006
21 Sep 2024158012
22 Sep 2024158007

Solar Active Regions and flaring

Solar flaring activity over the past 24 hours remained at low levels with background C-class flaring. There are six numbered regions on the visible solar disc with NOAA AR 3828 (beta-gamma- delta) growing to become the largest and most complex region. Most of the flaring activity was produced by NOAA AR 3824 (beta-gamma) from the west limb, NOAA AR 3825 (beta-gamma) and NOAA AR 3829 (beta). The solar flaring activity is likely to be predominantly at low levels over the coming days with 40% chances of M-class flares and 5% chances for isolated X-class flaring.

Espulsioni di massa coronale

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

Vento solare

Over the past 24 hours the solar wind parameters (ACE and DSCOVR) remained slightly perturbed. The interplanetary magnetic field reached 9.1 nT with Bz as low as - 8.7 nT. The solar wind velocity varied in the range of 340 km/s to 499 km/s. The B field phi angle was in the positive sector (directed away from the Sun). The solar wind conditions are expected to continue to be slightly perturbed in the upcoming days under the possible influence of mild high speed stream.

Geomagnetism

The geomagnetic conditions over the past 24 hours were quiet to active. Mostly quiet to unsettled geomagnetic conditions with isolated active periods are expected over the next days.

Proton flux levels

Over the past 24 hours the greater than 10 MeV GOES proton flux has been at nominal levels and is expected to remain so over the next 24 hours.

Electron fluxes at geostationary orbit

The greater than 2 MeV electron flux as measured by GOES 18 has exceeded the 1000 pfu threshold over the past 24 hours and is expected to exceed the threshold over the next 24 hours. The 24h electron fluence was at nominal levels and is expected to be at the border of nominal to moderate levels in the next 24 hours.

Today's estimated international sunspot number (ISN): 126, based on 15 stations.

Solar indices for 19 Sep 2024

Wolf number Catania183
10cm solar flux161
AK Chambon La Forêt017
AK Wingst016
Estimated Ap017
Estimated international sunspot number110 - Based on 29 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 M2025/04/05M1.0
Ultima tempesta geomagnetica2025/04/06Kp5 (G1)
Giorni senza macchie
Ultimo giorno senza macchie2022/06/08
Media mensile Numero di Macchie Solari
marzo 2025134.2 -20.4
aprile 2025148.7 +14.5
Ultimi 30 giorni132.7 -9.9

Questo giorno nella storia*

Brillamenti solari
12006M1.39
22002M1.38
31997C9.01
42002C8.7
52002C6.29
DstG
12000-292G4
21995-149G4
31977-95G3
41989-85G1
51960-76G1
*dal 1994

Social networks