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OK0NAG > SOLAR    27.05.11 23:04l 302 Lines 10087 Bytes #999 (0) @ EU
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Subj: Report of Solar Geophysical Activity (RSGA)
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Subject: Report of Solar Geophysical Activity (RSGA)
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:Product: Report of Solar-Geophysical Activity

:Issued: 2011 May 27 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 147 Issued at 2200Z on 27 May 2011

IA.  Analysis of Solar Active Regions and Activity from  26/2100Z

to 27/2100Z:  Solar activity was low.  New Region 1226 (S18E74)

produced a B-class event and four C-class events since being

numbered today.  The largest was a C5 observed at 27/1643Z.  This

region began with a B1 event at 26/1654Z as it approached the

southeast limb yesterday.  It is currently an H-type group, however,

the region is still rotating onto the disk and more white light area

are evident in the SDO/HMI imagery just visible on the limb.  Region

1223 (S16W00) produced the only other event during the period, a B4

at 27/0953Z.  This region is a Dso group with a beta magnetic

classification and grew slightly in sunspot count.  Two more regions

were numbered today as Regions 1224 (N21W15) and 1225 (N18E55). 

Region 1224 is a Dso group with a beta magnetic classification and

1225 is another H-type group.

IB.  Solar Activity Forecast:  Solar activity is expected to be low

with a chance for C-class events, and a slight chance for an M-class

event, as regions on the disk continue to evolve.

IIA.  Geophysical Activity Summary 26/2100Z to 27/2100Z:

The geomagnetic field was quiet to unsettled.  Observations from the

ACE spacecraft suggest the earth is under the continued influence of

the co-rotating interaction region in advance of the recurrent

coronal hole high speed stream.  Solar winds have slowly increased

from around 390 to 500 km/s.  The IMF Bt averaged around 8 nT with

the Bz mostly southward (-8 nT) through the period.

IIB.  Geophysical Activity Forecast:  The geomagnetic field is

expected to be predominately unsettled with occasional active

periods, including isolated minor storm conditions at high-latitudes

for day one (28 May).  This is expected due to effects from the

recurrent coronal hole high speed stream (CH HSS).  In addition

there are possible effects from the disappearing filament observed

on 25 May.  Quiet to unsettled conditions, with isolated active

levels, are expected for days two and three (29-30 May) with

continued CH HSS effects.

III.  Event Probabilities 28 May-30 May

Class M    10/10/10

Class X    01/01/01

Proton     01/01/01

PCAF       green

IV.  Penticton 10.7 cm Flux

Observed           27 May 090

Predicted   28 May-30 May  090/095/095

90 Day Mean        27 May 108

V.  Geomagnetic A Indices

Observed Afr/Ap 26 May  004/007

Estimated Afr/Ap 27 May  ???/???

Predicted Afr/Ap 28 May-30 May  015/018-010/012-008/008

VI.  Geomagnetic Activity Probabilities 28 May-30 May

A.  Middle Latitudes

Active                25/20/15

Minor storm           10/05/05

Major-severe storm    05/01/01

B.  High Latitudes

Active                35/30/20

Minor storm           15/10/10

Major-severe storm    05/05/05



Thank you for using the Product Subscription Service. If you would like 
to remove a product subscription or update the personal information in 
your account, go to: https://pss.swpc.noaa.gov. Please do not use the from 
address for correspondence, as it is not monitored. For comments or help, 
please contact us: pss.help@noaa.gov.
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