Viewing archive of Wednesday, 21 May 2008

Solar activity report

Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Report of Solar-Geophysical Activity 2008 May 21 2203 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 142 Issued at 2200Z on 21 May 2008

IA. Analysis of Solar Active Regions and Activity from 20-2100Z to 21-2100Z

Solar activity was very low. The visible disk is spotless.
IB. Solar Activity Forecast
Solar activity is expected to be very low.
IIA. Geophysical Activity Summary 20-2100Z to 21-2100Z
The geomagnetic field was mostly unsettled. An isolated active period was observed at 21/0300 - 0600Z. Solar wind speed increased gradually from approximately 450 km/s to values ranging between 550 - 620 km/s. The solar wind signatures were consistent with a high speed stream from a coronal hole.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be unsettled with a chance for isolated active periods for the next three days (22 - 24 May) due to persistent effects from the high speed stream.
III. Event Probabilities 22 May to 24 May
Class M01%01%01%
Class X01%01%01%
Proton01%01%01%
PCAFGreen
IV. Penticton 10.7 cm Flux
  Observed       21 May 069
  Predicted   22 May-24 May  068/068/068
  90 Day Mean        21 May 071
V. Geomagnetic A Indices
  Observed Afr/Ap 20 May  007/010
  Estimated     Afr/Ap 21 May  015/015
  Predicted    Afr/Ap 22 May-24 May  008/015-008/010-008/010
VI. Geomagnetic Activity Probabilities 22 May to 24 May
A. Middle Latitudes
Active25%25%25%
Minor storm10%10%10%
Major-severe storm01%01%01%
B. High Latitudes
Active40%40%40%
Minor storm20%20%20%
Major-severe storm10%10%10%

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

Norilsk, Vorkuta
The solar wind speed is currently moderately high (553.5 km/sec.)
The direction of the interplanetary magnetic field is slightly South (-5.62nT).
A southern hemisphere coronal hole was detected in an earth-facing position on Tuesday, 8 April 2025

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