Viewing archive of Friday, 4 December 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 Dec 04 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 338 Issued at 2200Z on 04 DEC 1998

IA. Analysis of Solar Active Regions and Activity from 03-2100Z to 04-2100Z

SOLAR ACTIVITY WAS LOW. FOUR MINOR C-CLASS X-RAY EVENTS OCCURRED, TWO UNCORRELATED, AND ONE EACH FROM REGIONS 8402 (N17E30) AND 8399 (N20W40). OF THE SEVEN ACTIVE REGIONS ON THE VISIBLE DISK, 8402 AND 8395 REMAIN THE MOST COMPLEX. REGION 8402 HAS GROWN SLIGHTLY SINCE YESTERDAY, AND IS CURRENTLY A 22-SPOT 'FSO' GROUP, WITH A BETA-GAMMA-DELTA MAGNETIC CLASSIFICATION AS REPORTED BY THE MT. WILSON OBSERVATORY. REGION 8395 (N20W40) HAS BEEN RELATIVELY STABLE DURING THE PAST 24 HOURS, AND IS NOW AN 11-SPOT 'FSO' GROUP, WITH A BETA-GAMMA MAGNETIC CLASSIFICATION BY MT. WILSON. NEW REGION 8403 (N20E37), A SMALL 'HSX' ALPHA GROUP WAS NUMBERED LATE YESTERDAY.
IB. Solar Activity Forecast
SOLAR ACTIVITY IS EXPECTED TO BE LOW TO MODERATE, WITH THE CONTINUED LIKLIHOOD OF C-CLASS, AND POSSIBILITY OF M-CLASS, EVENTS FROM REGIONS 8395 AND 8402.
IIA. Geophysical Activity Summary 03-2100Z to 04-2100Z
THE GEOMAGNETIC FIELD HAS BEEN QUIET TO UNSETTLED FOR THE PAST 24 HOURS.
IIB. Geophysical Activity Forecast
THE GEOMAGNETIC FIELD IS EXPECTED TO BE QUIET TO UNSETTLED FOR THE NEXT THREE DAYS.
III. Event Probabilities 05 DEC to 07 DEC
Class M25%25%25%
Class X05%05%05%
Proton05%05%05%
PCAFGREEN
IV. Penticton 10.7 cm Flux
  Observed       04 DEC 148
  Predicted   05 DEC-07 DEC  147/146/145
  90 Day Mean        04 DEC 131
V. Geomagnetic A Indices
OBSERVED AFR/AP 03 DEC  007/007
ESTIMATED AFR/AP 04 DEC  010/010
PREDICTED AFR/AP 05 DEC-07 DEC  010/010-010/010-005/010
VI. Geomagnetic Activity Probabilities 05 DEC to 07 DEC
A. Middle Latitudes
Active15%15%15%
Minor storm05%05%05%
Major-severe storm01%01%01%
B. High Latitudes
Active15%15%15%
Minor storm05%05%05%
Major-severe storm01%01%01%

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

Gillam, MB, Yellowknife, NT
A transequatorial coronal hole was detected in an earth-facing position on Monday, 24 March 2025

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Monday, 24 March 2025
Coronal hole faces Earth

The anticipated strong G3 geomagnetic storm watch never materialized as the coronal mass ejection that was supposed to arrive early yesterday didn't arrive until today just past midnight UTC. The impact was very lackluster with the Bt (total strength of the IMF) increasing to a moderate 15nT at best and the solar wind speed reaching just 420km/s. A far cry from the anticipated 700 to 800km/s. That once again goes to show how hard it is to forecast space weather events and any resulting geomagnetic conditions. We remain under the influence of the CME and high latitude sky watchers should remain alert for some nice aurora displays but middle latitude sky watchers will probably have to wait for the next opportunity. 

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Active geomagnetic conditions (Kp4) Threshold Reached: 02:33 UTC

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