Viewing archive of Tuesday, 15 July 2003
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 2003 Jul 15 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.comJoint USAF/NOAA Report of Solar and Geophysical Activity
SDF Number 196 Issued at 2200Z on 15 Jul 2003
IA. Analysis of Solar Active Regions and Activity from 14-2100Z to 15-2100Z
Solar activity was low. Today's activity consisted of a
few low-level C-class flares from Region 409 (N15E41). Region 409
showed growth with the development of new spots in the trailing
portion of the region. The penumbra in the region has developed to
form a compact distribution of spots, suggesting that a delta
configuration may form if the current trend continues. A seven
degree filament near (N41E11) disappeared between 1046 UTC and 1211
UTC. New Region 411 (N16E62) was assigned today.
IB. Solar Activity Forecast
Solar activity is expected to be low
to moderate over the next three days, with Region 409 as the most
likely source of M-class flares. There is a slight chance for major
flare activity from Region 409 if the current trend continues.
IIA. Geophysical Activity Summary 14-2100Z to 15-2100Z
The geomagnetic field ranged from unsettled to minor storm levels. An
initially active geomagnetic field reached minor storm levels from
0000-0600 UTC. Active to minor storm levels were also observed
between 0900-1200 UTC. Conditions have been unsettled since 1200
UTC. The activity increase was seen in response to a jump in solar
wind velocity and density accompanied by a southward turning of Bz
between 14/2100 UTC and 15/0100 UTC. Solar wind conditions remained
elevated for the remainder of the day, ranging mostly between 550 to
600 km/s. The solar wind data appear to be consistent with a brief
interval of a co-rotating interaction region followed by a
high-speed, coronal-hole-driven solar wind stream. 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 active, with a chance for isolated minor storm
periods, during the next 24 hours as a solar coronal hole rotates
through a geoeffective position. A decline to unsettled to active
levels is expected on the second day and a return to mostly
unsettled levels is expected by the third day.
III. Event Probabilities 16 Jul to 18 Jul
Class M | 40% | 40% | 40% |
Class X | 10% | 10% | 10% |
Proton | 05% | 05% | 05% |
PCAF | green
|
IV. Penticton 10.7 cm Flux
Observed 15 Jul 126
Predicted 16 Jul-18 Jul 125/123/121
90 Day Mean 15 Jul 126
V. Geomagnetic A Indices
Observed Afr/Ap 14 Jul 013/015
Estimated Afr/Ap 15 Jul 020/025
Predicted Afr/Ap 16 Jul-18 Jul 020/025-015/020-010/015
VI. Geomagnetic Activity Probabilities 16 Jul to 18 Jul
A. Middle Latitudes |
Active | 50% | 40% | 30% |
Minor storm | 25% | 20% | 15% |
Major-severe storm | 05% | 05% | 05% |
B. High Latitudes |
Active | 30% | 30% | 30% |
Minor storm | 35% | 25% | 20% |
Major-severe storm | 20% | 15% | 10% |
All times in UTC
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