Viewing archive of Sunday, 29 May 2005
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.
:Product: 20050529SGAS.txt
:Issued: 2005 May 29 0250 UT
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.comJoint USAF/NOAA Solar and Geophysical Activity Summary
SGAS Number 149 Issued at 0245Z on 29 May 2005 This report is compiled from data received at SWO on 28 MayA. Energetic Events
Begin Max End Rgn Loc Xray Op 245MHz 10cm Sweep None
B. Proton Events
None
C. Geomagnetic Activity Summary
The geomagnetic field was quiet to
active. Active periods are due to the effects of a recurrent coronal
hole high speed stream. At approximately 28/0330 UTC a Co-rotating
Interaction Region (CIR) was observed at ACE preceding the coronal
hole high speed stream. Solar wind speed at ACE increased from
approximately 275 km/s to 550 km/s and decreased slightly to around
420 km/s.
D. Stratwarm
Not available
E. Daily Indices: (real-time preliminary/estimated values)
10 cm 092 SSN 071 Afr/Ap 012/013 X-ray Background B1.5 Daily Proton Fluence (flux accumulation over 24 hrs) GT 1 MeV 6.6e+05 GT 10 MeV 1.6e+04 p/(cm2-ster-day) (GOES-11 satellite synchronous orbit W114 degrees) Daily Electron Fluence GT 2 MeV 3.60e+07 e/(cm2-ster-day) (GOES-12 satellite synchronous orbit W75 degrees) 3 Hour K-indices Boulder 1 3 3 2 2 4 4 4 Planetary 1 3 2 2 2 4 4 4
F. Comments
None
All times in UTC
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