Viewing archive of Wednesday, 10 March 2021

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2021 Mar 10 1316 UTC

SIDC Forecast

Valid from 1230 UTC, 10 Mar 2021 until 12 Mar 2021
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
10 Mar 2021085005
11 Mar 2021084007
12 Mar 2021082010

Bulletin

The new region, Catania group 78 (NOAA 2808), produced a C1.6 flare in the last 24 hours and has now fully turned to the Earth-facing solar hemisphere. Further C-level flare activity might take place in the next 24 hours.

No Earth-directed Coronal Mass Ejections (CMEs) have been observed in coronagraph data.

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 peaked over the 1000 pfu event threshold during its diurnal maximum and maybe do so again today. The 24h electron fluence reached moderate levels and is expected to drop slowly over the next days.

A low latitude corona hole of negative polarity in the southern hemisphere is now crossing the solar central meridian.

The solar wind continued to decline from the enhanced solar wind conditions. The solar wind speed is at 400 km/s and is expected to decline further during the next 24 hours. The magnetic field strength is below 5 nT and is expected to remain weak. The magnetic field was directed away from the Sun and is expected to remain largely so. Solar wind conditions are expected to further decay slowly over the next day. The corona hole crossing that crossed the solar meridian in the last 24 hours, is expected to effect the solar wind conditions in approximately 3 days. The sector boundary crossing ahead of it is expected on 12 March followed by an increase in the magnetic field strength.

Geomagnetic conditions were quiet to unsettled (both NOAA Kp and local K Dourbes had values 0-3). They are expected to remain quiet to unsettled for the next 24 to 48 hours. An increased level is expected afterwards due to the expected sector boundary crossing and enhanced solar wind conditions.

Today's estimated international sunspot number (ISN): 015, based on 13 stations.

Solar indices for 09 Mar 2021

Wolf number Catania025
10cm solar flux084
AK Chambon La Forêt005
AK Wingst003
Estimated Ap002
Estimated international sunspot number018 - Based on 17 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types
None

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

All times in UTC

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G3 - Strong geomagnetic storm

Observed Kp: 7
Threshold reached: 19:32 UTC

Current data suggests there is a high possibility for aurora to appear at the following high latitude regions in the near future

Kuopio
Arkhangelsk

Current data suggests there is a moderate possibility for aurora to appear at the following middle latitude regions in the near future

Helsinki, Tampere, Turku
Petrozavodsk, Syktyvkar

Current data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future

Copenhagen
Tallinn
Riga
Perm, Saint Petersburg, Surgut, Yaroslavl
Malmö, Stockholm
The strength of the interplanetary magnetic field is moderate (13.94nT), the direction is North (13.19nT).
The Disturbance Storm Time index predicts strong storm conditions right now (-144nT)

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