Visualizzazione archivio di mercoledì, 4 maggio AM

Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2022 May 04 1243 UTC

SIDC Forecast

Valid from 1230 UTC, 04 May 2022 until 06 May 2022
Brillamenti solari

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

Geomagnetism

Quiet (A<20 and K<4)

Protoni solari

Quiet

10cm fluxAp
04 May 2022118008
05 May 2022123007
06 May 2022128007

Bulletin

Solar flaring activity was high over the past 24 hours. An X1.1 flare was observed from beyond the east limb, peaking at 13:25UT. This region, which is just rotating onto the disk, also produced an M5.3 flare at 00:19UT. In addition, there was an M5.7 flare with a peak time of 08:59UT that originated from NOAA Active Region (AR) 3004. The rest of the regions were relatively quiet and stable. The flaring activity is expected to be at moderate levels with C-class flares expected, M-class flares probable and X-class flares possible.

There was a small dimming associated with the M5.7 flare originating from NOAA AR 3004. Given the location of the region near the central meridian, any associated eruption could impact Earth. Further analysis of any associated eruption will be given when the coronagraph data become available. No other 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 exceed threshold over the next 24 hours. The 24h electron fluence was at normal to moderate levels and is expected to be at normal to moderate levels over the next 24 hours.

The solar wind speed (as recorded by ACE) decreased from values around 440 to near 350 km/s. The total magnetic field magnitude fluctuated around 4 nT. The interplanetary magnetic field phi angle was predominantly in the negative sector (directed towards the Sun). The solar wind speed is expected to continue to gradually decrease and reflect a slow solar wind regime for the next 48 hours.

Geomagnetic conditions were quiet to unsettled. Geomagnetic conditions are expected to be quiet over the next 48 hours.

Today's estimated international sunspot number (ISN): 080, based on 16 stations.

Solar indices for 03 May 2022

Wolf number Catania130
10cm solar flux114
AK Chambon La Forêt009
AK Wingst007
Estimated Ap006
Estimated international sunspot number084 - Based on 30 stations

Noticeable events summary

DayBeginMaxFineLocStrengthOP10cmCatania/NOAARadio burst types
03130913251331S16E05X1.1SF96/3004
04000800190025----M5.3--/----
04084508590910S16W08M5.71N3296/3004

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