Viewing archive of Friday, 27 September 2002

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 2002 Sep 27 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 27 Sep 2002

IA. Analysis of Solar Active Regions and Activity from 26-2100Z to 27-2100Z

Solar activity was moderate during the past 24 hours. Region 134 (N11E38) showed a marked increase in flare productivity during the past 24 hours, including two M-class events. The first was an M1/Sf at 1312 UTC and the second was an M1/Sf at 1942 UTC. Coronagraph data show a relatively narrow CME off the northeast limb in association with the first M-class event. Insufficient data were available at forecast issue time to make any CME association with the second M-class event. Analysis of the Region 134 shows the development of a small delta configuration along an east-west inversion line, and observations indicate the build up of magnetic shear in this part of the region. The only other flare-producing region on the disk was Region 132 (N19W65), which managed to produce a couple C-class subflares, but appeared to be in a state of decline. New Region 135 (S26E06) emerged on the disk today as a simple D-type sunspot group.
IB. Solar Activity Forecast
Solar activity is expected to be low to moderate. There is a fair chance for additional M-class events from Region 134, and there is a slight chance that Region 132 may produce an isolated M-class event as well.
IIA. Geophysical Activity Summary 26-2100Z to 27-2100Z
The geomagnetic field has been quiet to unsettled during the past 24 hours.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be quiet to unsettled for the next 24-36 hours. An increase to unsettled to slightly active is expected late on the second day and should last through the third day in response to a favorably positioned coronal hole.
III. Event Probabilities 28 Sep to 30 Sep
Class M50%50%50%
Class X05%05%05%
Proton05%05%05%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       27 Sep 152
  Predicted   28 Sep-30 Sep  150/145/140
  90 Day Mean        27 Sep 179
V. Geomagnetic A Indices
  Observed Afr/Ap 26 Sep  003/008
  Estimated     Afr/Ap 27 Sep  005/008
  Predicted    Afr/Ap 28 Sep-30 Sep  005/008-010/012-015/015
VI. Geomagnetic Activity Probabilities 28 Sep to 30 Sep
A. Middle Latitudes
Active15%35%35%
Minor storm10%15%20%
Major-severe storm05%05%10%
B. High Latitudes
Active20%30%40%
Minor storm15%20%25%
Major-severe storm05%15%20%

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

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