Visualizzazione archivio di mercoledì, 28 aprile AM

Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2021 Apr 28 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 28 Apr 2021 until 30 Apr 2021
Brillamenti solari

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

Geomagnetism

Quiet (A<20 and K<4)

Protoni solari

Quiet

10cm fluxAp
28 Apr 2021078006
29 Apr 2021078007
30 Apr 2021077014

Bulletin

X-ray flux has remained below C level throughout the period. All three regions on disc remained stable or in decay. In particular the trailing edge of Catania group 91 (NOAA region 2821) seems to be dissolving. X-ray flux is likely to remain below C level though an isolated C-flare is not unlikely.

No new Earth directed CMEs have been detected. Regarding the April 26 filament eruption and associated CME reported yesterday: SoHO/LASCO C2 coronagraph data now show more clearly (though faint) the CME propagating towards the South-South-West with an angular width of under 90 degrees. Nevertheless, combined with the STEREO A observations which clearly display an equatorial component, it is not excluded that Earth may see part of the passing magnetic cloud. If it reaches Earth it should be expected late on May 1.

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. The greater than 2 MeV electron flux remained under the 1000 pfu event threshold. The 24h electron fluence was at normal levels but rising. As Solar wind enhancements are now dying out, the electron fluence is expected to remain at normal levels during next days.

From just before midnight, Solar wind parameters finally showed the expected return to slow Solar wind conditions. Solar wind speed meanwhile dropped to around 375km/s while total magnetic field remained under 5nT with an unremarkable Bz component and a phi angle indicating magnetic field orientation mostly towards the Sun. By end of April 30, start of May 1 we may see Solar wind perturbations due to a combination of enhanced speed associated to the positive polarity coronal hole currently transiting the central meridian, and magnetic field perturbations due to passing magnetic clouds from first the April 25 CME and later the April 26 CME. Though likelihood and confidence for the CME arrivals is low.

Geomagnetic conditions were quiet (local K Dourbes and NOAA Kp 0-2). Geomagnetic conditions are expected to be quiet to unsettled until at least late April 30.

Today's estimated international sunspot number (ISN): 044, based on 16 stations.

Solar indices for 27 Apr 2021

Wolf number Catania///
10cm solar flux079
AK Chambon La Forêt006
AK Wingst007
Estimated Ap007
Estimated international sunspot number053 - Based on 30 stations

Noticeable events summary

DayBeginMaxFineLocStrengthOP10cmCatania/NOAARadio burst types
Nessuna

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

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Notizie sul meteo spaziale

Ultimo brillamento X2026/03/30X1.5
Ultimo brillamento M2026/04/04M7.6
Ultima tempesta geomagnetica2026/04/02Kp6- (G2)
Giorni senza macchie
Ultimi 365 giorni3 giorni
20263 giorni (3%)
Ultimo giorno senza macchie2026/02/24
Media mensile Numero di Macchie Solari
marzo 202685.9 +7.7
aprile 2026141 +55.1
Ultimi 30 giorni95.4 +31.2

Questo giorno nella storia*

Brillamenti solari
12002M8.82
22026M7.6
31999M6.76
42001M2.91
52003M2.74
DstG
11979-202G3
21988-133G3
31984-120G4
42004-117G2
51994-111G3
*dal 1994

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