Viewing archive of Tuesday, 24 April 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 Apr 24 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 115 Issued at 2200Z on 24 Apr 2012

IA. Analysis of Solar Active Regions and Activity from 23-2100Z to 24-2100Z

Solar activity has been at low levels for the past 24 hours with multiple C-class x-ray events. A C3 flare was observed at 24/0745Z off the east limb from new Region 1467 (N14E72). Associated with this event, were both a type II radio sweep (estimated shock velocity of 1029 km/s) and a non-Earth directed CME. Two other new regions were numbered today, Region 1468 (N09E12) which rapidly emerged on the disk and Region 1469 (S21E68), which rotated onto the disk. The remaining active regions were stable and quiet today, except for Region 1465 (S19W12). Region 1465 showed a consolidation of both leader and follower spot groups into one cluster and is now classified as a beta-gamma-delta.
IB. Solar Activity Forecast
Solar activity is expected to be at low levels with a slight chance for M-class activity for the next three days (25 - 27 April).
IIA. Geophysical Activity Summary 23-2100Z to 24-2100Z
The geomagnetic field ranged from quiet to major storm levels during the past 24 hours due to continued CME effects and the arrival of a coronal hole high speed stream (CH HSS). Early in the period, measurements from the ACE spacecraft showed extensive southward (negative) periods of the Bz component of the IMF. Even though solar wind speeds remained well below nominal levels, these periods drove the majority of the geomagnetic activity. Around 24/0200Z, CH HSS characteristics were observed by the ACE spacecraft with solar wind density dropping off as the solar wind speed increased. At the time of this report, solar wind speeds had increased from around 350 km/s to around 630 km/s.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at quiet to active levels on day one (25 April) as the effects of a CH HSS continue. An increase to active with a chance for isolated minor storm periods is expected on day two (26 April) as the CME from 23 April is expected to become geoeffective. Quiet to unsettled levels are expected on day three (27 April) as effects of the CME wane.
III. Event Probabilities 25 Apr to 27 Apr
Class M20%20%20%
Class X01%01%01%
Proton01%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observed       24 Apr 134
  Predicted   25 Apr-27 Apr  130/130/125
  90 Day Mean        24 Apr 112
V. Geomagnetic A Indices
  Observed Afr/Ap 23 Apr  021/030
  Estimated     Afr/Ap 24 Apr  021/031
  Predicted    Afr/Ap 25 Apr-27 Apr  012/018-017/022-011/015
VI. Geomagnetic Activity Probabilities 25 Apr to 27 Apr
A. Middle Latitudes
Active25%40%25%
Minor storm10%20%10%
Major-severe storm01%05%01%
B. High Latitudes
Active45%50%40%
Minor storm25%30%25%
Major-severe storm15%15%10%

All times in UTC

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