Viewing archive of Sunday, 27 May 2012

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 2012 May 27 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 148 Issued at 2200Z on 27 May 2012

IA. Analysis of Solar Active Regions and Activity from 26-2100Z to 27-2100Z

Solar activity was low. Region 1492 produced a long duration C-class flare at 27/0552Z. This event was associated with a CME observed off the southeast limb of the solar disk in LASCO C2/C3 and does not appear to be earth directed. Another more impressive CME was observed at the end of the period yesterday. No flare was observed in conjunction due to a source from around the west limb. However, type II and IV radio sweeps were observed from the event, in addition to a later observed 10 MeV proton event (NOAA Scale S1). The CME shock and driver cloud are observable in LASCO C2/C3 as a backside asymmetric halo and are not expected to be geoeffective.
IB. Solar Activity Forecast
Solar activity is expected to be very low to low for the next 3 days (28-30 May).
IIA. Geophysical Activity Summary 26-2100Z to 27-2100Z
The geomagnetic field was quiet. The greater than 10 MeV proton event at geosynchronous orbit that began at 27/0535Z, reached a maximum of 14 pfu at 27/1045Z and ended at 27/1235Z. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels during the period.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be mostly quiet for the next 3 days (28-30 May).
III. Event Probabilities 28 May to 30 May
Class M05%05%05%
Class X01%01%01%
Proton01%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       27 May 111
  Predicted   28 May-30 May  110/110/110
  90 Day Mean        27 May 117
V. Geomagnetic A Indices
  Observed Afr/Ap 26 May  005/004
  Estimated     Afr/Ap 27 May  004/004
  Predicted    Afr/Ap 28 May-30 May  006/005-006/005-006/005
VI. Geomagnetic Activity Probabilities 28 May to 30 May
A. Middle Latitudes
Active05%05%05%
Minor storm01%01%01%
Major-severe storm01%01%01%
B. High Latitudes
Active15%15%15%
Minor storm15%15%15%
Major-severe storm10%10%10%

All times in UTC

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

Norilsk, Vorkuta
The maximum X-ray flux of the past two hours is:
M1.61

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