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Daily bulletin on solar and geomagnetic activity from the SIDC

Випущено: 2020 Jun 01 1233 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
01 Jun 2020	070	007
02 Jun 2020	070	008
03 Jun 2020	070	007

Bulletin

Solar X ray flux remained below B level throughout the period. The region in the northern hemisphere, responsible for the M1 flare a few days ago, had decayed to plage and remained quiescent, although it remains to be watched. Overall probability for flaring is low.

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 was in a near nominal regime. Solar wind speed was around 400 km/s and total magnetic field around 4nT with the magnetic field phi angle stable in the negative sector. We are expecting near nominal conditions to continue over the next 48 hours.

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

Today's estimated international sunspot number (ISN): 006, based on 30 stations.

Solar indices for 31 May 2020

Wolf number Catania	///
10cm solar flux	071
AK Chambon La Forêt	008
AK Wingst	004
Estimated Ap	003
Estimated international sunspot number	/// - Based on /// stations

Noticeable events summary

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

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