Viewing archive of Thursday, 22 October 2020

Solar activity report

Report of Solar-Geophysical Activity 2020 Oct 22 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 296 Issued at 2200Z on 22 Oct 2020

IA. Analysis of Solar Active Regions and Activity from 21-2100Z to 22-2100Z

Solar activity has been at very low levels for the past 24 hours. There are currently 1 numbered sunspot regions on the disk.
IB. Solar Activity Forecast
Solar activity is expected to be very low on days one, two, and three (23 Oct, 24 Oct, 25 Oct).
IIA. Geophysical Activity Summary 21-2100Z to 22-2100Z
The geomagnetic field has been at quiet to unsettled levels for the past 24 hours. Solar wind speed reached a peak of 410 km/s at 21/2132Z. Total IMF reached 8 nT at 22/0455Z. The maximum southward component of Bz reached -5 nT at 22/1157Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 168 pfu.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at quiet to minor storm levels on day one (23 Oct) and quiet to active levels on days two and three (24 Oct, 25 Oct).
III. Event Probabilities 23 Oct to 25 Oct
Class M01%01%01%
Class X01%01%01%
Proton01%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       22 Oct 075
  Predicted   23 Oct-25 Oct 075/075/075
  90 Day Mean        22 Oct 072

V. Geomagnetic A Indices
  Observed Afr/Ap 21 Oct  007/007
  Estimated     Afr/Ap 22 Oct  010/012
  Predicted    Afr/Ap 23 Oct-25 Oct  015/020-013/015-012/015

VI. Geomagnetic Activity Probabilities 23 Oct to 25 Oct
A. Middle Latitudes
Active40%40%35%
Minor storm30%25%20%
Major-severe storm10%05%05%
B. High Latitudes
Active05%10%10%
Minor storm25%25%30%
Major-severe storm65%65%50%

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, Yellowknife, NT
A transequatorial coronal hole was detected in an earth-facing position on Monday, 24 March 2025

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Monday, 24 March 2025
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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13:55 UTC - Coronal hole

A transequatorial coronal hole is facing Earth. Enhanced solar wind could arrive in ~3 days

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02:45 UTC - Geomagnetic activity

Active geomagnetic conditions (Kp4) Threshold Reached: 02:33 UTC

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