Viewing archive of Monday, 1 June 2020

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2020 Jun 01 1233 UTC

SIDC Forecast

Valid from 1230 UTC, 01 Jun 2020 until 03 Jun 2020
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
01 Jun 2020070007
02 Jun 2020070008
03 Jun 2020070007

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 flux071
AK Chambon La Forêt008
AK Wingst004
Estimated Ap003
Estimated international sunspot number/// - Based on /// 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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Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future

Gillam, MB, Yellowknife, NT

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