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CX2SA  > SWPC     30.04.12 00:23l 65 Lines 2815 Bytes #999 (0) @ WW
BID : 59720-CX2SA
Read: GUEST
Subj: Report of Solar-Geophysical Activity
Path: IZ3LSV<IK2XDE<DB0RES<DK0WUE<7M3TJZ<CX2SA
Sent: 120429/2219Z @:CX2SA.SAL.URY.SA #:59720 [Salto] FBB7.00e $:59720-CX2SA
From: CX2SA@CX2SA.SAL.URY.SA
To  : SWPC@WW

:Product: Report of Solar-Geophysical Activity
:Issued: 2012 Apr 29 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 120 Issued at 2200Z on 29 Apr 2012
IA.  Analysis of Solar Active Regions and Activity from  28/2100Z
to 29/2100Z:  Solar activity was at low levels due to low-level
C-class events from Regions 1465 (S18W80), 1466 (N13W65), 1467
(N12E04), 1469 (S19W01) and 1471 (S23E57). New Region 1472 (S29E40)
emerged on the disk as a simple bi-polar group. GONG H-alpha and
SDO/AIA 304 imagery observed a filament eruption along a six degree
long channel centered near N06E36, just to the SE of Region 1467.
This eruption occurred during the period 28/1800 - 2000Z. Associated
multiple CME activity was visible off the east limb as observed in
LASCO/C2 imagery at 28/1936Z and 28/2024Z. At the time of this
report, analysis was ongoing as to the geoeffective nature of these
CMEs.
IB.  Solar Activity Forecast:  Solar activity is expected to be low
for the next three days (30 April - 02 May).
IIA.  Geophysical Activity Summary 28/2100Z to 29/2100Z:
The geomagnetic field was at quiet to unsettled levels. Through the
period, ACE solar wind velocities ranged between 380 to 440 km/s
while the Bz component of the interplanetary magnetic field did not
vary much beyond +/- 4 nT. The greater than 2 MeV electron flux at
geosynchronous orbit reached high levels during the period.
IIB.  Geophysical Activity Forecast:  The geomagnetic field is
expected to be at predominately quiet levels for day one (30 April).
By days two and three (01 - 02 May), quiet to unsettled levels with
a slight chance for isolated active periods are expected as a
coronal hole high speed stream moves into a geoeffective position.
III.  Event Probabilities 30 Apr-02 May
Class M    10/10/10
Class X    01/01/01
Proton     01/01/01
PCAF       green
IV.  Penticton 10.7 cm Flux
Observed           29 Apr 116
Predicted   30 Apr-02 May  115/115/110
90 Day Mean        29 Apr 112
V.  Geomagnetic A Indices
Observed Afr/Ap 28 Apr  005/005
Estimated Afr/Ap 29 Apr  005/006
Predicted Afr/Ap 30 Apr-02 May  004/005-007/008-007/008
VI.  Geomagnetic Activity Probabilities 30 Apr-02 May
A.  Middle Latitudes
Active                10/15/15
Minor storm           01/01/05
Major-severe storm    01/01/01
B.  High Latitudes
Active                10/20/20
Minor storm           01/05/05
Major-severe storm    01/01/01

___________________________________________________________

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



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