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CX2SA  > SWPC     22.04.12 00:23l 71 Lines 3134 Bytes #999 (0) @ WW
BID : 59397-CX2SA
Read: GUEST
Subj: Report of Solar-Geophysical Activity
Path: IZ3LSV<IW0QNL<IK6ZDE<VE3UIL<CX2SA
Sent: 120421/2219Z @:CX2SA.SAL.URY.SA #:59397 [Salto] FBB7.00e $:59397-CX2SA
From: CX2SA@CX2SA.SAL.URY.SA
To  : SWPC@WW

:Product: Report of Solar-Geophysical Activity
:Issued: 2012 Apr 21 2200 UTC
# Prepared jointly by the U.S. Dept. of Commerce, NOAA,
# Space Weather Prediction Center and the U.S. Air Force.
#
Joint USAF/NOAA Report of Solar and Geophysical Activity
SDF Number 112 Issued at 2200Z on 21 Apr 2012
IA.  Analysis of Solar Active Regions and Activity from  20/2100Z
to 21/2100Z:  Solar activity was low. Regions 1460 (N16W27 -
Dkc/beta) and 1465 (S17E27 - Dso/beta) each produced a low-level
C-class flare. Region 1460 showed minor interior spot growth and
some mixed polarities in its trailer portion. Minor interior spot
growth also occurred in Region 1465 as well as penumbral growth in
its trailer. Region 1459 (S14W13 - Eac/beta) showed penumbral growth
in its interior portion and maintained a simple beta magnetic
configuration. No Earth-directed CMEs were observed during the
period. No new regions were numbered.
IB.  Solar Activity Forecast:  Solar activity is expected to be low
during the period (22 - 24 April) with a chance for an isolated
M-class flare.
IIA.  Geophysical Activity Summary 20/2100Z to 21/2100Z:
Geomagnetic field activity was at quiet levels until around 21/1900Z,
then increased to quiet to unsettled levels. The increase was
associated with a weak interplanetary shock (IPS) passage, detected
at ACE at around 21/1611Z, and followed by a weak geomagnetic field
response at around 21/1712Z (no Sudden Geomagnetic Impulse
observed). ACE solar wind data showed a change to mostly southward
IMF Bz following the IPS passage (maximum deflections to -8 nT) as
well as a gradual increase in IMF Bt (peaks to 9 nT). A minor
increase in wind speeds also followed the IPS passage. It is likely
the CME passage was associated with the partial-halo CME observed on
18 April.
IIB.  Geophysical Activity Forecast:  Geomagnetic field activity is
expected to be at quiet to unsettled levels during the period (22 -
24 April) with a chance for active levels. Weak CME-passage effects
are expected during 22 - 23 April (another CME is expected to arrive
late on 22 April). A recurrent coronal hole high-speed stream is
expected to become geoeffective on 24 April.
III.  Event Probabilities 22 Apr-24 Apr
Class M    30/30/30
Class X    01/01/01
Proton     01/01/01
PCAF       green
IV.  Penticton 10.7 cm Flux
Observed           21 Apr 149
Predicted   22 Apr-24 Apr  150/150/145
90 Day Mean        21 Apr 112
V.  Geomagnetic A Indices
Observed Afr/Ap 20 Apr  007/008
Estimated Afr/Ap 21 Apr  006/007
Predicted Afr/Ap 22 Apr-24 Apr  011/012-010/010-010/010
VI.  Geomagnetic Activity Probabilities 22 Apr-24 Apr
A.  Middle Latitudes
Active                20/20/25
Minor storm           10/10/15
Major-severe storm    01/01/01
B.  High Latitudes
Active                25/25/35
Minor storm           15/15/25
Major-severe storm    05/05/10

___________________________________________________________

Automatic packet bulletin created with information received
by cx2sa.net from the SWPC Space Weather Prediction Center.
___________________________________________________________



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