Viewing archive of Thursday, 14 February 2008

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 2008 Feb 14 2203 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 045 Issued at 2200Z on 14 Feb 2008

IA. Analysis of Solar Active Regions and Activity from 13-2100Z to 14-2100Z

Solar activity was at very low levels. The visible disk remains spotless.
IB. Solar Activity Forecast
Solar activity is expected to be very low.
IIA. Geophysical Activity Summary 13-2100Z to 14-2100Z
The geomagnetic field was predominately quiet to unsettled due to a geoeffective coronal hole high speed stream. Solar wind speed remains in excess of 600 km/s. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels today.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be quiet to unsettled, with possible isolated active conditions, 15 - 16 February due to the continued influence of the coronal hole high speed stream. On 17 February conditions are expected to abate to quiet.
III. Event Probabilities 15 Feb to 17 Feb
Class M01%01%01%
Class X01%01%01%
Proton01%01%01%
PCAFGreen
IV. Penticton 10.7 cm Flux
  Observed       14 Feb 071
  Predicted   15 Feb-17 Feb  072/072/072
  90 Day Mean        14 Feb 075
V. Geomagnetic A Indices
  Observed Afr/Ap 13 Feb  010/012
  Estimated     Afr/Ap 14 Feb  008/012
  Predicted    Afr/Ap 15 Feb-17 Feb  008/010-008/010-005/005
VI. Geomagnetic Activity Probabilities 15 Feb to 17 Feb
A. Middle Latitudes
Active35%35%30%
Minor storm10%10%05%
Major-severe storm01%01%01%
B. High Latitudes
Active40%40%35%
Minor storm15%15%10%
Major-severe storm05%05%05%

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