Viewing archive of Monday, 14 October 2002
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 2002 Oct 14 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.comJoint USAF/NOAA Report of Solar and Geophysical Activity
SDF Number 287 Issued at 2200Z on 14 Oct 2002
IA. Analysis of Solar Active Regions and Activity from 13-2100Z to 14-2100Z
Solar activity increased to moderate. A long-duration
M2/Sf event occurred early in the period peaking at 14/0010 UTC,
from bright plage just east of the large spot in Region 159
(S11E57). This event was accompanied by a large CME evident in
SOHO/LASCO imagery, with an estimated plane-of-sky velocity of about
850 km/s. Region 159 also produced a C4/Sf event at 14/0945 UTC. A
Type-II radio sweep of estimated velocity 743 km/s was observed at
14/1429 UTC, in association with a small impulsive C1 flare, and
followed shortly thereafter by a very long-lived enhancement in
x-ray flux that began at about 14/1520 UTC, and remained in progress
at the end of the period. Available H-alpha imagery revealed no
apparent source for this activity, and SOHO EIT and LASCO data were
mostly unavailable for the period. The lack of subsequent particle
enhancement from this potential CME event seems to suggest an
east-limb source for this activity. New Region 160 (S20E54) was
numbered today.
IB. Solar Activity Forecast
Solar activity is expected to be low
to moderate for the next three days.
IIA. Geophysical Activity Summary 13-2100Z to 14-2100Z
The geomagnetic field ranged from quiet to major storm levels. An
extended interval of active conditions, with an isolated period of
major storming at high latitudes, appeared to occur primarily due to
a sustained strong southward orientation of Bz, and a slow increase
in solar wind speed. Other solar wind data suggest an overall
pattern of a CIR evolving toward to a weak high speed stream pattern
near the end of the period.
IIB. Geophysical Activity Forecast
The geomagnetic field is
expected to be quiet to active for the early part of the forecast
period, with mostly quiet to unsettled conditions by the end of day
one and into day two. By day three, some CME passage effects may
occur in response to the solar activity described above, and may
cause isolated active or minor storm conditions by the end of the
period.
III. Event Probabilities 15 Oct to 17 Oct
Class M | 30% | 30% | 30% |
Class X | 05% | 05% | 05% |
Proton | 05% | 01% | 01% |
PCAF | green
|
IV. Penticton 10.7 cm Flux
Observed 14 Oct 181
Predicted 15 Oct-17 Oct 175/175/165
90 Day Mean 14 Oct 182
V. Geomagnetic A Indices
Observed Afr/Ap 13 Oct 006/010
Estimated Afr/Ap 14 Oct 017/026
Predicted Afr/Ap 15 Oct-17 Oct 015/018-012/012-015/025
VI. Geomagnetic Activity Probabilities 15 Oct to 17 Oct
A. Middle Latitudes |
Active | 25% | 20% | 30% |
Minor storm | 05% | 05% | 10% |
Major-severe storm | 01% | 01% | 01% |
B. High Latitudes |
Active | 30% | 25% | 35% |
Minor storm | 10% | 05% | 15% |
Major-severe storm | 01% | 01% | 05% |
All times in UTC
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