Viewing archive of Sunday, 13 September 2020

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2020 Sep 13 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 13 Sep 2020 until 15 Sep 2020
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
13 Sep 2020069003
14 Sep 2020070003
15 Sep 2020070003

Bulletin

The Sun was spotless. Solar activity was at very low levels and is expected to remain so.

The greater than 10 MeV proton flux was at nominal levels and is expected to remain so. The greater than 2 MeV electron flux exceeded the 1000 pfu alert threshold, with a maximum of 1467 pfu at 16:10UT. The electron flux is expected to be at nominal levels, with a small chance to reach moderate levels.

No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery.

Solar wind speed varied between 310 and 350 km/s (DSCOVR). Bz varied between -5 and +4 nT. The direction of the interplanetary magnetic field (phi angle) was mostly away from the Sun (positive sector).

Geomagnetic activity was at quiet levels and expected to remain so, an isolated unsettled interval not excluded.

Today's estimated international sunspot number (ISN): 000, based on 13 stations.

Solar indices for 12 Sep 2020

Wolf number Catania///
10cm solar flux069
AK Chambon La Forêt010
AK Wingst006
Estimated Ap006
Estimated international sunspot number000 - Based on 27 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, Iqaluit, NU
Nuuk
Reykjavik
The solar wind speed is currently moderately high (516.6 km/sec.)
A southern hemisphere coronal hole was detected in an earth-facing position on Tuesday, 8 April 2025

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