Viewing archive of Tuesday, 3 March 1998

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 1998 Mar 03 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 062 Issued at 2200Z on 03 MAR 1998

IA. Analysis of Solar Active Regions and Activity from 02-2100Z to 03-2100Z

SOLAR ACTIVITY WAS LOW. REGION 8171 (S23W50) REMAINS THE LARGEST SUNSPOT GROUP ON THE VISIBLE DISK. THIS REGION HAS CONTINUED TO GROW IN WHITE LIGHT AREA BUT REMAINS RELATIVELY SIMPLE IN MAGNETIC COMPLEXITY. THE REGION PRODUCED SEVERAL C-CLASS SUBFLARES SINCE YESTERDAY.
IB. Solar Activity Forecast
SOLAR ACTIVITY IS EXPECTED TO BE LOW. ADDITIONAL C-CLASS FLARES ARE LIKELY IN REGION 8171. A SMALL M-CLASS FLARE IS POSSIBLE BUT NOT IMMINENT.
IIA. Geophysical Activity Summary 02-2100Z to 03-2100Z
THE GEOMAGNETIC FIELD WAS QUIET TO UNSETTLED. THE GREATER THAN 2 MEV ELECTRON FLUX AT GEOSYNCHRONOUS ALTITUDE WAS MODERATE.
IIB. Geophysical Activity Forecast
THE GEOMAGNETIC FIELD IS EXPECTED TO BE QUIET TO UNSETTLED.
III. Event Probabilities 04 MAR to 06 MAR
Class M05%05%05%
Class X01%01%01%
Proton01%01%01%
PCAFGREEN
IV. Penticton 10.7 cm Flux
  Observed       03 MAR 097
  Predicted   04 MAR-06 MAR  098/098/096
  90 Day Mean        03 MAR 095
V. Geomagnetic A Indices
OBSERVED AFR/AP 02 MAR  011/014
ESTIMATED AFR/AP 03 MAR  004/005
PREDICTED AFR/AP 04 MAR-06 MAR  010/008-010/012-005/008
VI. Geomagnetic Activity Probabilities 04 MAR to 06 MAR
A. Middle Latitudes
Active15%15%15%
Minor storm10%10%10%
Major-severe storm05%05%01%
B. High Latitudes
Active15%15%15%
Minor storm10%10%10%
Major-severe storm05%05%01%

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