Viewing archive of Saturday, 28 April 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 Apr 28 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 118 Issued at 2200Z on 28 Apr 2001

IA. Analysis of Solar Active Regions and Activity from 27-2100Z to 28-2100Z

Solar activity dropped to low levels. Region 9433 (N17W50) produced isolated C-class flares, the largest of which was a C7/1f at 28/0934 UTC. Gradual decay continued in the leading and intermediate portions of this region. However, no decay was evident within its trailing spots, where a strong magnetic delta configuration remained. Region 9441 (N07E23) continued a gradual growth phase that began on 27 April, but the region remained a moderate-sized, simply-structured bipole. New Regions 9444 (S11E67) and 9445 (N23E76) were assigned.
IB. Solar Activity Forecast
Solar activity is expected to be at moderate to high levels. Region 9433 is expected to produce isolated M-class flares. This region could also produce an isolated major flare during the period.
IIA. Geophysical Activity Summary 27-2100Z to 28-2100Z
Geomagnetic field activity ranged from quiet to minor storm levels. An interplanetary shock at the leading edge of a CME passed the ACE spacecraft at 28/0432 UTC, followed by a sudden impulse (SI) at 28/0520 UTC (76 nT, as measured by the Boulder USGS magnetometer). The source for the CME was an M7/2b flare on 26 April. Field activity increased to unsettled to minor storm levels following the SI. The greater than 10 MeV proton flux at geosynchronous orbit briefly crossed event threshold in response to the shock passage. The greater than 10 MeV event began at 28/0430 UTC, reached a maximum of 57 PFU at 28/0500 UTC, then ended at 28/0520 UTC. Proton fluxes had decreased to near background levels by the close of the period.
IIB. Geophysical Activity Forecast
Geomagnetic field activity is expected to be at unsettled to active levels through midday, 29 April as the disturbance gradually subsides. Quiet to unsettled levels are expected for the remainder of the period. Region 9433 could produce another proton flare before it crosses the west limb on 02 May. The greater than 2 MeV electron flux at geosynchronous orbit may reach high levels during the first half of the period.
III. Event Probabilities 29 Apr to 01 May
Class M75%75%75%
Class X20%20%20%
Proton20%20%20%
PCAFyellow
IV. Penticton 10.7 cm Flux
  Observed       28 Apr 188
  Predicted   29 Apr-01 May  185/180/175
  90 Day Mean        28 Apr 167
V. Geomagnetic A Indices
  Observed Afr/Ap 27 Apr  003/006
  Estimated     Afr/Ap 28 Apr  026/028
  Predicted    Afr/Ap 29 Apr-01 May  015/015-012/010-010/010
VI. Geomagnetic Activity Probabilities 29 Apr to 01 May
A. Middle Latitudes
Active30%25%20%
Minor storm15%10%10%
Major-severe storm10%05%01%
B. High Latitudes
Active35%30%25%
Minor storm20%15%10%
Major-severe storm15%10%05%

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