Viewing archive of Saturday, 26 September 2020

Solar activity report

Report of Solar-Geophysical Activity 2020 Sep 26 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 270 Issued at 2200Z on 26 Sep 2020

IA. Analysis of Solar Active Regions and Activity from 25-2100Z to 26-2100Z

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C1 event observed at 26/0038Z from Region 2773 (N27E18). There are currently 0 numbered sunspot regions on the disk.
IB. Solar Activity Forecast
Solar activity is expected to be very low with a slight chance for a C-class flare on days one, two, and three (27 Sep, 28 Sep, 29 Sep).
IIA. Geophysical Activity Summary 25-2100Z to 26-2100Z
The geomagnetic field has been at quiet to minor storm levels for the past 24 hours. Solar wind speed reached a peak of 585 km/s at 26/1707Z. Total IMF reached 9 nT at 26/1135Z. The maximum southward component of Bz reached -8 nT at 26/1202Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 3802 pfu.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at quiet to minor storm levels on days one and two (27 Sep, 28 Sep) and unsettled to major storm levels on day three (29 Sep).
III. Event Probabilities 27 Sep to 29 Sep
Class M01%01%01%
Class X01%01%01%
Proton01%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       26 Sep 073
  Predicted   27 Sep-29 Sep 072/072/072
  90 Day Mean        26 Sep 070

V. Geomagnetic A Indices
  Observed Afr/Ap 25 Sep  017/018
  Estimated     Afr/Ap 26 Sep  018/025
  Predicted    Afr/Ap 27 Sep-29 Sep  013/018-015/022-028/040

VI. Geomagnetic Activity Probabilities 27 Sep to 29 Sep
A. Middle Latitudes
Active40%45%30%
Minor storm25%25%40%
Major-severe storm05%05%25%
B. High Latitudes
Active10%05%05%
Minor storm25%20%15%
Major-severe storm60%65%80%

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

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