Viewing archive of Tuesday, 1 May 2007

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 2007 May 01 2203 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 121 Issued at 2200Z on 01 May 2007

IA. Analysis of Solar Active Regions and Activity from 30-2100Z to 01-2100Z

Solar activity was very low. Only low level B-class flares were observed. Region 953 (S12W04) has decreased in area to around 440 millionths and has weakened to a beta-gamma magnetic class.
IB. Solar Activity Forecast
Solar activity is expected to be very low to low with a slight chance for an M-flare from Region 953.
IIA. Geophysical Activity Summary 30-2100Z to 01-2100Z
The geomagnetic field was quiet to unsettled. An isolated active period was observed at the Boulder Magnetometer between 01/0600 - 0900 UTC. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels again today.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be mostly quiet for the forecast period (02 - 04 May).
III. Event Probabilities 02 May to 04 May
Class M10%10%05%
Class X01%01%01%
Proton01%01%01%
PCAFGreen
IV. Penticton 10.7 cm Flux
  Observed       01 May 086
  Predicted   02 May-04 May  085/085/080
  90 Day Mean        01 May 074
V. Geomagnetic A Indices
  Observed Afr/Ap 30 Apr  013/020
  Estimated     Afr/Ap 01 May  008/008
  Predicted    Afr/Ap 02 May-04 May  005/005-005/005-005/005
VI. Geomagnetic Activity Probabilities 02 May to 04 May
A. Middle Latitudes
Active15%15%15%
Minor storm05%05%05%
Major-severe storm01%01%01%
B. High Latitudes
Active20%15%15%
Minor storm10%05%05%
Major-severe storm01%01%01%

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