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Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2019 Mar 21 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 21 Mar 2019 until 23 Mar 2019
Brillamenti solari

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

Geomagnetism

Quiet (A<20 and K<4)

Protoni solari

Quiet

10cm fluxAp
21 Mar 2019077004
22 Mar 2019078007
23 Mar 2019081007

Bulletin

There are two active regions on the visible solar disc. NOAA AR 2735 is decaying and has produced no activity in the past hours. On the other hand, the newly numbered NOAA AR 2736 (beta magnetic field configuration) has been more active producing numerous B-class flares and two C-class flares, the largest wass a C5.6 one peaking at 03:12 UT. This AR produced a faint CME yesterday directed mostly to the west, first seen at 18:24 UT on LASCO-C2, this CME is not expected to affect the Earth. Nevertheless, it had produced a larger CME earlier on March 20, first seen at 12:00 UT as an asymmetric full halo CME with the bulk of the material going to the northwest. Using LASCO-C2 and COR2 (beacon) images the speed of this CME was calculated to be 751 km/s, a flank of the CME is expected to hit the Earth on March 23.

Solar protons have remained at background levels over the past 24 hours.

The solar wind speed is at 350 km/s with interplanetary magnetic fields of 4 nT. Quiet conditions were observed in the past hours and the situation is not expected to change until the CME arrival on March 23.

Today's estimated international sunspot number (ISN): 040, based on 18 stations.

Solar indices for 20 Mar 2019

Wolf number Catania///
10cm solar flux077
AK Chambon La Forêt009
AK Wingst005
Estimated Ap004
Estimated international sunspot number036 - Based on 22 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 X2025/03/28X1.1
Ultimo brillamento M2025/04/01M2.5
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