Viewing archive of Thursday, 29 March 2001

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 2001 Mar 29 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 088 Issued at 2200Z on 29 Mar 2001

IA. Analysis of Solar Active Regions and Activity from 28-2100Z to 29-2100Z

Solar activity was high. Region 9393 (N17W18) produced an X1/1N event at 29/1015Z. This event had an associated Type IV radio sweep, a tenflare of 4700 sfu, and a full halo CME was reported from LASCO/SOHO imagery. This earth-directed CME occurred at approximately 29/1030Z. Region 9393 also produced numerous minor M-class events during the period. Region 9393 has shown slight growth in area since yesterday and is currently over 2400 millionths in white light. No new regions were numbered today.
IB. Solar Activity Forecast
Solar activity is expected to be high. Region 9393 still has the best potential to produce a major flare.
IIA. Geophysical Activity Summary 28-2100Z to 29-2100Z
The geomagnetic field was quiet to minor storm. The greater than 10 MeV protons crossed the 10 pfu event threshold at 29/1635Z and has not yet peaked (highest flux observed so far was 18 pfu at 29/2050Z).
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to increase during the first day of the period to active to major storms levels due to a CME passage. The passage of a faster CME, from the X1 event today, may occur later on the first day. With the passage of the second CME, conditions are expected to be at active to major storm levels with isolated severe conditions possible. During the last half of the period, conditions are expected to decrease to unsettled to active conditions. CME passage could increase the strength and duration of the 10 MeV proton event currently in progress. Another proton event is possible, and likely stronger, if Region 9393 produces another major flare as it transits the solar western hemisphere.
III. Event Probabilities 30 Mar to 01 Apr
Class M80%80%80%
Class X30%30%30%
Proton99%30%30%
PCAFyellow
IV. Penticton 10.7 cm Flux
  Observed       29 Mar 262
  Predicted   30 Mar-01 Apr  260/255/250
  90 Day Mean        29 Mar 163
V. Geomagnetic A Indices
  Observed Afr/Ap 28 Mar  019/031
  Estimated     Afr/Ap 29 Mar  020/025
  Predicted    Afr/Ap 30 Mar-01 Apr  045/050-045/050-025/030
VI. Geomagnetic Activity Probabilities 30 Mar to 01 Apr
A. Middle Latitudes
Active30%20%40%
Minor storm40%50%30%
Major-severe storm20%25%15%
B. High Latitudes
Active20%10%30%
Minor storm40%40%40%
Major-severe storm30%40%20%

All times in UTC

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