Viewing archive of Friday, 19 February 2021

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2021 Feb 19 1241 UTC

SIDC Forecast

Valid from 1230 UTC, 19 Feb 2021 until 21 Feb 2021
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 Feb 2021070007
20 Feb 2021071021
21 Feb 2021072007

Bulletin

The solar activity has been quiet over the past 24 hours. The sunspot (Catania 72, NOAA-AR 2802) that emerged yesterday has already decayed. The new unipolar sunspot (Catania 73) is visible close to the east limb of the solar disc, however, no significant flaring activity was recorded. The solar activity is expected to remain at low levels for the next 24 hours with small chances of C-class flare from the newly emerged sunspot.

No Earth-directed coronal mass ejections was observed in the available coronagraph imagery.

The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux remained under the 1000 pfu threshold and is expected to remain so in the next 24 hours.

Over the past 24 hours, the solar wind speed ranged between 360 km/s and 390 km/s. The total magnetic field was below 5 nT, it then starts to increase on February 19 around 05:00 UTC up to the current value of 8 nT. The Bz component fluctuated between -7.3 nT and 7.5 nT. The high-speed streams associated with the equatorial coronal hole (negative magnetic polarity and facing Earth on February 18) is expected to impact the solar wind environment near Earth in about 1-2 days.

The geomagnetic conditions over the past 24 hours were quiet. The conditions are expected to remain mostly quiet with possible short periods of unsettled conditions in response to the slightly enhancement of the interplanetary magnetic field and possible prolonged period of southward directed Bz component.

Today's estimated international sunspot number (ISN): 011, based on 12 stations.

Solar indices for 18 Feb 2021

Wolf number Catania013
10cm solar flux071
AK Chambon La Forêt006
AK Wingst///
Estimated Ap004
Estimated international sunspot number011 - Based on 16 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

Arkhangelsk, Vorkuta
The maximum X-ray flux of the past two hours is:
C8.08

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