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Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2018 Sep 09 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 09 Sep 2018 until 11 Sep 2018
Brillamenti solari

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

Geomagnetism

Minor storm expected (A>=30 or K=5)

Protoni solari

Quiet

10cm fluxAp
09 Sep 2018069008
10 Sep 2018069013
11 Sep 2018069034

Bulletin

Solar activity was at very low levels. Small and inactive sunspot region NOAA 2721 is still present on the solar disk. No earth-directed coronal mass ejections (CMEs) were observed in the available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels. A trans-equatorial positive polarity coronal hole (CH) has finished its transit over the Central Meridian.

Solar activity is expected to remain at very low levels.

Solar wind speed varied between 360 and 430 km/s, ending the period near 370 km/s (DSCOVR). Bz varied mostly between -4 and +3 nT, ending the period at +6 nT. The direction of the interplanetary magnetic field was variable.

Quiet to unsettled geomagnetic conditions were observed. Mostly quiet geomagnetic conditions are expected with a chance on an unsettled episode until the arrival of the co-rotating interaction region (CIR) and wind stream from the positive polarity CH, late on 10 or on 11 September. This may result in minor storming conditions.

Today's estimated international sunspot number (ISN): 015, based on 21 stations.

Solar indices for 08 Sep 2018

Wolf number Catania///
10cm solar flux069
AK Chambon La Forêt009
AK Wingst005
Estimated Ap005
Estimated international sunspot number016 - Based on 23 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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