Viewing archive of Sunday, 5 June 2016

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2016 Jun 05 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 05 Jun 2016 until 07 Jun 2016
Solar flares

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

Geomagnetism

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

Solar protons

Quiet

10cm fluxAp
05 Jun 2016080021
06 Jun 2016075019
07 Jun 2016075010

Bulletin

Solar activity once more was very low. No active regions are visible. No flares or CMEs were observed. The solar activity is expected to remain low for the next 48 hours.

Solar wind observations indicate the presence of a co-rotating interaction region (CIR) preceding a coronal hole high speed stream. The magnitude of the interplanetary magnetic field abruptly increased around 6h30 UT to a maximum of 16 nT, with a varying Bz. The solar wind speed (currently 430 km/s) and temperature are also increasing. Geomagnetic conditions were mainly quiet, but indicate the starting influence of the solar wind disturbance (local K at Dourbes and NOAA estimated Kp currently are at K=4). Geomagnetic conditions up to minor storm levels (K=5) can occur within the next 24 to 48 hours.

Today's estimated international sunspot number (ISN): 000, based on 27 stations.

Solar indices for 04 Jun 2016

Wolf number Catania///
10cm solar flux080
AK Chambon La Forêt007
AK Wingst004
Estimated Ap003
Estimated international sunspot number000 - Based on 17 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

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