Viewing archive of Monday, 5 April 2010

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 2010 Apr 05 2201 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 095 Issued at 2200Z on 05 Apr 2010

IA. Analysis of Solar Active Regions and Activity from 04-2100Z to 05-2100Z

Solar activity was very low. Todays activity consisted of a few low-level B-class events, primarily from newly emerging Region 1061 (N14W11). Region 1061 is a small D-type sunspot group. Region 1060 (N25E45) was quiet and stable and is a small C-type sunspot group.
IB. Solar Activity Forecast
Solar activity is expected to be very low for the next three days (06-08 April). There is, however a chance for an isolated C-class event from Region 1061.
IIA. Geophysical Activity Summary 04-2100Z to 05-2100Z
The geomagnetic field ranged from quiet to severe storm levels during the past 24 hours. Conditions were initially quiet to unsettled, but increased to active levels after 0300Z, and increased further to major to severe storm levels between 0900-1200Z. The increase in activity followed a strong shock observed at the ACE spacecraft at 0756Z which led to a sudden impulse at Earth at 0826Z (observed to be 38 nT at the Boulder magnetometer). Numerous high-latitude stations reported severe storm levels during the interval as did several mid-latitude stations in the nighttime sectors. Activity declined to active to major storm levels from 1200-1800Z and declined further to mostly unsettled levels from 1800-2100Z. Solar wind observations showed elevated solar wind velocity behind the shock with speeds between 720-800 km/s with fairly strong Bz (peak negative values around -15 nT). Solar wind speed and magnetic field observations showed a decreasing trend during the last 4-5 hours of the interval. The most probable source for the disturbance is the halo CME that was observed on 03 April at 0954Z. The greater than 2 MeV electron flux reached high levels during the past 24 hours.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be unsettled to active during the early part of the first day (06 April) due to persistent effects from the current disturbance. In addition, another increase to unsettled levels with a chance for active periods is expected late in the day and continuing through the second day (07 April) due to the onset of a high speed stream from a favorably positioned coronal hole. Activity levels are expected to decline to mostly unsettled levels on the third day (08 April).
III. Event Probabilities 06 Apr to 08 Apr
Class M01%01%01%
Class X01%01%01%
Proton01%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       05 Apr 079
  Predicted   06 Apr-08 Apr  082/085/085
  90 Day Mean        05 Apr 083
V. Geomagnetic A Indices
  Observed Afr/Ap 04 Apr  011/013
  Estimated     Afr/Ap 05 Apr  025/025
  Predicted    Afr/Ap 06 Apr-08 Apr  015/017-012/012-008/008
VI. Geomagnetic Activity Probabilities 06 Apr to 08 Apr
A. Middle Latitudes
Active35%35%20%
Minor storm20%20%10%
Major-severe storm10%05%01%
B. High Latitudes
Active40%40%25%
Minor storm25%30%15%
Major-severe storm15%10%01%

All times in UTC

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