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.comJoint 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 M | 01% | 01% | 01% |
Class X | 01% | 01% | 01% |
Proton | 01% | 01% | 01% |
PCAF | green
|
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 |
Active | 35% | 35% | 20% |
Minor storm | 20% | 20% | 10% |
Major-severe storm | 10% | 05% | 01% |
B. High Latitudes |
Active | 40% | 40% | 25% |
Minor storm | 25% | 30% | 15% |
Major-severe storm | 15% | 10% | 01% |
All times in UTC
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