Viewing archive of Sunday, 9 March 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 Mar 09 2203 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 069 Issued at 2200Z on 09 Mar 2008

IA. Analysis of Solar Active Regions and Activity from 08-2100Z to 09-2100Z

Solar activity was very low. The visible disk is spotless.
IB. Solar Activity Forecast
Solar activity is expected to continue at very low levels.
IIA. Geophysical Activity Summary 08-2100Z to 09-2100Z
The geomagnetic field was at quiet to minor storm levels due to the influence of a recurrent coronal hole high speed stream. Solar wind at the ACE spacecraft increased from 438 km/s to a maximum of 691 km/s at 09/2023Z.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to range from quiet to active levels with isolated minor storm periods possible for the next three days (10 - 12 March), due to the coronal hole high speed stream. Isolated major storm conditions are possible at high latitudes during this period.
III. Event Probabilities 10 Mar to 12 Mar
Class M01%01%01%
Class X01%01%01%
Proton01%01%01%
PCAFGreen
IV. Penticton 10.7 cm Flux
  Observed       09 Mar 070
  Predicted   10 Mar-12 Mar  070/070/070
  90 Day Mean        09 Mar 074
V. Geomagnetic A Indices
  Observed Afr/Ap 08 Mar  006/011
  Estimated     Afr/Ap 09 Mar  020/025
  Predicted    Afr/Ap 10 Mar-12 Mar  010/015-010/010-010/015
VI. Geomagnetic Activity Probabilities 10 Mar to 12 Mar
A. Middle Latitudes
Active30%30%30%
Minor storm15%15%15%
Major-severe storm05%05%05%
B. High Latitudes
Active40%40%40%
Minor storm20%20%20%
Major-severe storm10%10%10%

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