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Daily bulletin on solar and geomagnetic activity from the SIDC

Випущено: 2020 Jun 07 1231 UTC

SIDC Forecast

Сонячні спалахи

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

Geomagnetism

Quiet (A<20 and K<4)

Сонячні протони

Quiet

	10cm flux	Ap
07 Jun 2020	072	010
08 Jun 2020	072	013
09 Jun 2020	072	007

Bulletin

Solar X-ray flux remained below C level throughout the period. NOAA region 2765 remained fairly inactive producing just some minor B flares. C flares from this region are possible but not very probable.

There were no Earth directed Coronal Mass Ejections (CMEs) observed in coronagraph data.

The greater than 10 MeV proton flux levels were at background values and are expected to continue to be at background level. The greater than 2 MeV electron flux has been nominal over the past days.

Solar wind speed showed originally a minor decreasing trend reaching under 300 km/s around 6UT before showing a steady increase to around 350km/s presently. The total magnetic field was around or below 5nT with a variable Bz component. The magnetic field phi angle was variable but predominantly in the negative sector. Solar wind conditions may become slightly more enhanced but should overall remain close to nominal.

Geomagnetic conditions were quiet (NOAA Kp and local K Dourbes 0-2). Geomagnetic conditions are expected to be quiet to unsettled over the next 48 hours.

Today's estimated international sunspot number (ISN): 015, based on 16 stations.

Solar indices for 06 Jun 2020

Wolf number Catania	///
10cm solar flux	072
AK Chambon La Forêt	007
AK Wingst	003
Estimated Ap	003
Estimated international sunspot number	014 - Based on 32 stations

Noticeable events summary

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

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