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Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2020 Jun 08 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 08 Jun 2020 until 10 Jun 2020
Brillamenti solari

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

Geomagnetism

Quiet (A<20 and K<4)

Protoni solari

Quiet

10cm fluxAp
08 Jun 2020073010
09 Jun 2020073010
10 Jun 2020073007

Bulletin

Active Region NOAA 2765 produced a few B flares in the past 24 hours. The chance for a C flare in the next 24 hours, especially from NOAA 2765, is estimated at 30%.

No Earth-directed Coronal Mass Ejections (CMEs) were observed in available coronagraphic imagery.

The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours.

Solar wind speed near Earth as registered by DSCOVR increased from about 340 to 500 km/s in the past 24 hours, with current values around 475 km/s. This is probably related to patchy extensions of the northern coronal hole. The Interplanetary Magnetic Field (IMF) was oriented predominantly away from the Sun, and its magnitude varied between about 0 and 13 nT, with current values of around 3 nT. Bz was below -5 nT between 17:30 and 19:15 UT on June 7. Enhanced solar wind conditions are expected in the next 24 hours.

Quiet to unsettled geomagnetic conditions (K Dourbes between 1 and 3; NOAA Kp between 1 and 4) were registered in the past 24 hours. Quiet to unsettled geomagnetic levels (K Dourbes < 4) are expected on June 8, 9 and 10, with a chance for isolated active intervals (K Dourbes = 4).

Today's estimated international sunspot number (ISN): 016, based on 20 stations.

Solar indices for 07 Jun 2020

Wolf number Catania///
10cm solar flux073
AK Chambon La Forêt020
AK Wingst012
Estimated Ap011
Estimated international sunspot number015 - Based on 26 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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