Viewing archive of Friday, 4 March 2022

Solar activity report

Report of Solar-Geophysical Activity 2022 Mar 04 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 63 Issued at 2200Z on 04 Mar 2022

IA. Analysis of Solar Active Regions and Activity from 03-2100Z to 04-2100Z

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C3 event observed at 03/2155Z from Region 2958 (N17E11). There are currently 5 numbered sunspot regions on the disk.
IB. Solar Activity Forecast
Solar activity is likely to be low with a slight chance for an M-class flare on days one, two, and three (05 Mar, 06 Mar, 07 Mar).
IIA. Geophysical Activity Summary 03-2100Z to 04-2100Z
The geomagnetic field has been at quiet to unsettled levels for the past 24 hours. Solar wind speed reached a peak of 484 km/s at 04/1041Z. Total IMF reached 8 nT at 04/0042Z. The maximum southward component of Bz reached -5 nT at 04/1717Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 234 pfu.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at quiet to active levels on days one, two, and three (05 Mar, 06 Mar, 07 Mar).
III. Event Probabilities 05 Mar to 07 Mar
Class M20%20%20%
Class X01%01%01%
Proton01%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       04 Mar 113
  Predicted   05 Mar-07 Mar 115/117/117
  90 Day Mean        04 Mar 106

V. Geomagnetic A Indices
  Observed Afr/Ap 03 Mar  003/004
  Estimated     Afr/Ap 04 Mar  012/017
  Predicted    Afr/Ap 05 Mar-07 Mar  011/012-011/012-011/012

VI. Geomagnetic Activity Probabilities 05 Mar to 07 Mar
A. Middle Latitudes
Active30%30%30%
Minor storm10%10%10%
Major-severe storm01%01%01%
B. High Latitudes
Active15%15%15%
Minor storm30%30%30%
Major-severe storm40%40%40%

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

Rovaniemi, Sodankylä, Utsjoki
Reykjavik
Kirkenes, Tromsø
Murmansk
Kiruna
A transequatorial coronal hole was detected in an earth-facing position on Monday, 24 March 2025

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Latest alerts

Coronal hole faces Earth

The anticipated strong G3 geomagnetic storm watch never materialized as the coronal mass ejection that was supposed to arrive early yesterday didn't arrive until today just past midnight UTC. The impact was very lackluster with the Bt (total strength of the IMF) increasing to a moderate 15nT at best and the solar wind speed reaching just 420km/s. A far cry from the anticipated 700 to 800km/s. That once again goes to show how hard it is to forecast space weather events and any resulting geomagnetic conditions. We remain under the influence of the CME and high latitude sky watchers should remain alert for some nice aurora displays but middle latitude sky watchers will probably have to wait for the next opportunity. 

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