Viewing archive of Tuesday, 6 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 06 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.comJoint USAF/NOAA Report of Solar and Geophysical Activity
SDF Number 065 Issued at 2200Z on 06 Mar 2001
IA. Analysis of Solar Active Regions and Activity from 05-2100Z to 06-2100Z
Solar activity has been low. The largest event of the
day was an optically uncorrelated C6 flare at 06/1013 UTC.
SOHO/LASCO data suggest an association with the most energetic phase
of a CME observed off the west limb, though not appearing
earth-directed. Several lesser C-class events occurred throughout
the day, with three observed from Region 9368 (N25W08), which
underwent some growth in spot count and areal coverage, but without
significant change in magnetic complexity. Region 9371 (N20W64)
exhibited similar growth, but produced only two subfaint optical
flares without notable x-ray enhancements. Region 9370 showed some
increase in size and complexity, but has remained quiet so far,
along with the other numbered regions on the disk.
IB. Solar Activity Forecast
Solar activity is expected to be
predominantly low for the next three days, though a chance for
isolated moderate (weak M-class) activity exists principally for
Region 9368.
IIA. Geophysical Activity Summary 05-2100Z to 06-2100Z
The geomagnetic field has been quiet to unsettled. Solar wind speed
remains somewhat elevated, but recent effects from a coronal hole
high speed stream appear to have waned over the course of the day.
IIB. Geophysical Activity Forecast
The geomagnetic field is
expected to be quiet to unsettled, with isolated active conditions
possible for the next 24 hours, until coronal hole effects have
completely subsided. Mainly quiet to unsettled conditions are
expected thereafter for the remainder of the forecast period.
III. Event Probabilities 07 Mar to 09 Mar
Class M | 30% | 30% | 30% |
Class X | 01% | 01% | 01% |
Proton | 01% | 01% | 01% |
PCAF | green
|
IV. Penticton 10.7 cm Flux
Observed 06 Mar 158
Predicted 07 Mar-09 Mar 162/165/165
90 Day Mean 06 Mar 162
V. Geomagnetic A Indices
Observed Afr/Ap 05 Mar 019/018
Estimated Afr/Ap 06 Mar 008/008
Predicted Afr/Ap 07 Mar-09 Mar 008/008-007/005-005/005
VI. Geomagnetic Activity Probabilities 07 Mar to 09 Mar
A. Middle Latitudes |
Active | 20% | 15% | 15% |
Minor storm | 05% | 01% | 01% |
Major-severe storm | 01% | 01% | 01% |
B. High Latitudes |
Active | 25% | 15% | 15% |
Minor storm | 10% | 01% | 01% |
Major-severe storm | 01% | 01% | 01% |
All times in UTC
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