Viewing archive of Thursday, 19 April 2018

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2018 Apr 19 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 19 Apr 2018 until 21 Apr 2018
Solar flares

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

Geomagnetism

Active conditions expected (A>=20 or K=4)

Solar protons

Quiet

10cm fluxAp
19 Apr 2018071007
20 Apr 2018073016
21 Apr 2018072007

Bulletin

During last 24 hours only few low B-class were reported. All flaring activity originated from the active region which is rotating from the behind of the East solar limb. This active region might be the source of B-class and isolated C-class flares in the coming hours. The coronagraph images do not show signatures of a possibly Earth directed CME. The solar protons remain at the background level.

The solar wind speed is about 280 km/s and the interplanetary magnetic field magnitude is rather low with the value of about 2 nT. The increase of the solar wind speed, associated with equatorial coronal hole which reached central meridian on April 16 is expected later today, or tomorrow morning. The geomagnetic conditions are presently quiet. We expect quiet to unsettled conditions later today and possibly active geomagnetic conditions tomorrow.

Today's estimated international sunspot number (ISN): 007, based on 27 stations.

Solar indices for 18 Apr 2018

Wolf number Catania///
10cm solar flux071
AK Chambon La Forêt010
AK Wingst006
Estimated Ap006
Estimated international sunspot number000 - Based on 29 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

Fairbanks, AK
The solar wind speed is currently moderately high (625.3 km/sec.)

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