Viewing archive of Sunday, 15 April 2001

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 2001 Apr 15 0245 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Solar and Geophysical Activity Summary

SGAS Number 105 Issued at 0245Z on 15 Apr 2001 This report is compiled from data received at SWO on 14 Apr
A. Energetic Events
Begin  Max  End  Rgn   Loc   Xray  Op 245MHz 10cm   Sweep
1715 1811 1828  9415 S16W71 M1.0  Sf 210    31
1734 1737 1742                       250    150
1752 1752 1755                       52     55     II
2320 2323 2326  9415 S20W71 B7.9  Sf 110
B. Proton Events
There were no proton events detected at geosynchronous orbit. However, the greater than 10 MeV proton flux continued at enhanced levels (due to recent major flare activity) as it gradually declined toward background levels.
C. Geomagnetic Activity Summary
Activity was at unsettled to active levels until 14/0900 UTC, then decreased to quiet to unsettled levels.
D. Stratwarm
None
E. Daily Indices: (real-time preliminary/estimated values)
10 cm 139  SSN 149  Afr/Ap 017/015   X-ray Background B5.1
Daily Proton Fluence (flux accumulation over 24 hrs)
GT 1 MeV 4.1e+06   GT 10 MeV 1.7e+05 p/(cm2-ster-day)
(GOES-8 satellite synchronous orbit W75 degrees)
Daily Electron Fluence
GT 2 MeV 6.50e+07 e/(cm2-ster-day)
(GOES-8 satellite synchronous orbit W75 degrees)
3 Hour K-indices
Boulder 3 4 4 3 3 3 3 2 Planetary 3 3 4 3 3 3 3 2
F. Comments
  None

All times in UTC

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G2 - Moderate geomagnetic storm

Observed Kp: 6
Threshold reached: 19:52 UTC

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

Oulu, Rovaniemi, Sodankylä
Luleå

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

Tórshavn
Kuopio
Bergen, Trondheim
Arkhangelsk
Sundsvall, Umeå

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

Tampere
Petrozavodsk
The solar wind speed is currently moderately high (551.1 km/sec.)
The density of the solar wind is high (48.27 p/cm3)

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