Viewing archive of Thursday, 20 August 2020

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2020 Aug 20 1243 UTC

SIDC Forecast

Valid from 1230 UTC, 20 Aug 2020 until 22 Aug 2020
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
20 Aug 2020071008
21 Aug 2020071008
22 Aug 2020071002

Bulletin

The solar activity was low over the past 24 hours. The X-ray flux was low and reached B-class level. For the next 24 hours the solar activity is expected to remain low.

No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraphic imagery.

The greater than 10 MeV proton flux was at background levels over the past 24 hours. It is expected to stay at background levels for the next 24 hours. The greater than 2 MeV electron flux was at nominal levels over the past 24 hours and is expected to remain so over the next 24 hours.

The speed of the solar wind varied between 305 and 340 km/s (DSCOVR), while its density slightly increased. The polarity of the Interplanetary Magnetic Field (IMF) was predominantly oriented away the Sun (phi angle in the positive sector), apart from 4-8UT when it was on the negative sector. Bz fluctuated between -2 and +2 nT. The magnitude of the magnetic field varied between 0 and 4 nT. Over the next 24 hours, there is a chance to see the combined effects of the wind associated with the CME on Aug 16th and the Coronal Hole (CH) at central meridial on Aug 17th can be anticipated to have an impact, which sould be followed by the HSS of the CH from Aug 19th.

The geomagnetic conditions were quiet to unsettled. The values registered for the past 24 hours were 0-3 for K Dourbes and 0-1for NOAA Kp. Unsettled to active conditions, are expected for the next 24 hours.

Today's estimated international sunspot number (ISN): 012, based on 18 stations.

Solar indices for 19 Aug 2020

Wolf number Catania///
10cm solar flux071
AK Chambon La Forêt006
AK Wingst005
Estimated Ap006
Estimated international sunspot number014 - Based on 30 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

Tórshavn
Trondheim
The solar wind speed is currently moderately high (571.1 km/sec.)

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