Viewing archive of Monday, 26 August 2002

Geophysical 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.
Solar and Geophysical Activity Summary 2002 Aug 26 0245 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Solar and Geophysical Activity Summary

SGAS Number 238 Issued at 0245Z on 26 Aug 2002 This report is compiled from data received at SWO on 25 Aug
A. Energetic Events
Begin  Max  End  Rgn   Loc   Xray  Op 245MHz 10cm   Sweep
0236 0236 0236                       370
0252 0253 0254                       210
0315 0321 0330              C3.1                   II
0447 0447 0447                       130
0558 0602 0606                       170
0640 0640 0641                       180
1845 1853 1858  0083 S17W40 M1.1  Sf 85     46
2251 2255 2255                       970
2338 2346 2353  0083 S18W42 M1.9  Sf 340
B. Proton Events
The greater than 10 MeV proton event continues in progress--start 24/0140 UTC, 317 pfu peak 24/0835 UTC, and current flux about 20 pfu.
C. Geomagnetic Activity Summary
The geomagnetic field was quiet to unsettled.
D. Stratwarm
None
E. Daily Indices: (real-time preliminary/estimated values)
10 cm 179  SSN 136  Afr/Ap 006/009   X-ray Background C1.1
Daily Proton Fluence (flux accumulation over 24 hrs)
GT 1 MeV 7.0e+07   GT 10 MeV 6.8e+06 p/(cm2-ster-day)
(GOES-8 satellite synchronous orbit W75 degrees)
Daily Electron Fluence
GT 2 MeV 4.20e+07 e/(cm2-ster-day)
(GOES-8 satellite synchronous orbit W75 degrees)
3 Hour K-indices
Boulder 2 2 2 1 3 2 1 3 Planetary 2 2 2 2 2 3 3 3
F. Comments
  The Afr index reported in Part E is estimated from
Boulder observations.

All times in UTC

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G1 - Minor geomagnetic storm

Observed Kp: 5
Threshold reached: 19:50 UTC

Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future

Tórshavn
Oulu, Rovaniemi, Kuopio, Sodankylä, Utsjoki
Reykjavik
Kirkenes, Tromsø, Trondheim
Arkhangelsk, Murmansk, Norilsk, Vorkuta
Kiruna, Luleå, Sundsvall, Umeå
The solar wind speed is currently moderately high (545.4 km/sec.)
The maximum X-ray flux of the past two hours is:
C7.95

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