Viewing archive of Friday, 17 April 2020

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2020 Apr 17 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 17 Apr 2020 until 19 Apr 2020
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
17 Apr 2020069007
18 Apr 2020068009
19 Apr 2020069008

Bulletin

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

The greater than 10 MeV proton flux and the greater than 2 MeV electron flux were at nominal values and are expected to remain so.

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

Solar wind speed was on a mostly declining trend, varying between 370 and 300 km/s and ending the period with low values around 310 km/s (DSCOVR). Bz varied between -4 and +3 nT, being mostly negative since 06UT. The direction of the interplanetary magnetic field (phi angle) was in a predominantly sunward orientation (negative sector).

Geomagnetic activity was at quiet levels, with an isolated unsettled episode recorded by Dourbes during the 15-18UT interval. Geomagnetic conditions are expected to be quiet to unsettled during the next few days.

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

Solar indices for 16 Apr 2020

Wolf number Catania///
10cm solar flux069
AK Chambon La Forêt007
AK Wingst006
Estimated Ap004
Estimated international sunspot number000 - Based on 34 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 (502.1 km/sec.)
The strength of the interplanetary magnetic field is moderate (10.25nT), the direction is North (0.51nT).
A southern hemisphere coronal hole was detected in an earth-facing position on Tuesday, 8 April 2025

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