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WA7EES > RSGA     10.06.12 04:20l 151 Lines 6664 Bytes #999 (0) @ WW
BID : WA7EESF18
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Subj: Report of Solar Geophysical Activity (RSGA)
Path: IZ3LSV<IW0QNL<VE2PKT<VK2DOT<N9LYA<N0XR<W6IDS
Sent: 120609/2253Z 7782@W6IDS.IN.USA.NOAM BPQK1.4.50

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:Product: Report of Solar-Geophysical Activity
:Issued: 2012 Jun 09 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 161 Issued at 2200Z on 09 Jun 2012
IA.  Analysis of Solar Active Regions and Activity from  08/2100Z
to 09/2100Z:  Solar activity was moderate. New Region 1505 (S09E63)
produced an impulsive M1 flare at 09/1132Z. This region was
classified as a Axx type group with alpha magnetic characteristics.
New Region 1504 (S18E67) followed with an impulsive M1/Sf at
09/1645Z and was classified as a Cao type group with beta magnetic
characteristics. Region 1499 (N16W31) produced C1 events at
09/0308Z, 1032Z,  and 1527Z. The first event was also associated
with an Sf optical flare. Region 1499 was classified as a Cao type
group with beta-gamma magnetic characteristics. There were no
earth-directed CMEs observed during the period.
IB.  Solar Activity Forecast:  Solar activity is expected to remain
low with an increasing chance for occasional M-class activity for
the next three days (10-12 June).
IIA.  Geophysical Activity Summary 08/2100Z to 09/2100Z:
The geomagnetic field activity was mostly quiet. A weak disturbance
was observed on both ground and GOES magnetometers at 09/1841Z
leading to the single unsettled period of the day. Solar wind speed
at the ACE spacecraft continued to decline and ended the period near
440 km/s. The Bz component of the interplanetary magentic field
remained mostly neutral or positive. 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 quiet to unsettled for the next three days (10-12
June) with the anticiapted glancing blows from CMEs on 06 June and
08 June and the arrival on 11 June of a coronal hole high speed
stream.
III.  Event Probabilities 10 Jun-12 Jun
Class M    45/50/55
Class X    01/01/01
Proton     01/01/01
PCAF       Green
IV.  Penticton 10.7 cm Flux
Observed           09 Jun 128
Predicted   10 Jun-12 Jun  130/130/130
90 Day Mean        09 Jun 117
V.  Geomagnetic A Indices
Observed Afr/Ap 08 Jun  009/009
Estimated Afr/Ap 09 Jun  006/007
Predicted Afr/Ap 10 Jun-12 Jun  007/010-007/010-007/010
VI.  Geomagnetic Activity Probabilities 10 Jun-12 Jun
A.  Middle Latitudes
Active                20/20/20
Minor storm           10/10/10
Major-severe storm    01/01/01
B.  High Latitudes
Active                15/15/15
Minor storm           25/25/25
Major-severe storm    30/30/30


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    <pre>:Product: Report of Solar-Geophysical Activity
:Issued: 2012 Jun 09 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 161 Issued at 2200Z on 09 Jun 2012
IA.  Analysis of Solar Active Regions and Activity from  08/2100Z
to 09/2100Z:  Solar activity was moderate. New Region 1505 (S09E63)
produced an impulsive M1 flare at 09/1132Z. This region was
classified as a Axx type group with alpha magnetic characteristics. 
New Region 1504 (S18E67) followed with an impulsive M1/Sf at
09/1645Z and was classified as a Cao type group with beta magnetic
characteristics. Region 1499 (N16W31) produced C1 events at
09/0308Z, 1032Z,  and 1527Z. The first event was also associated
with an Sf optical flare. Region 1499 was classified as a Cao type
group with beta-gamma magnetic characteristics. There were no
earth-directed CMEs observed during the period.
IB.  Solar Activity Forecast:  Solar activity is expected to remain
low with an increasing chance for occasional M-class activity for
the next three days (10-12 June).
IIA.  Geophysical Activity Summary 08/2100Z to 09/2100Z:
The geomagnetic field activity was mostly quiet. A weak disturbance
was observed on both ground and GOES magnetometers at 09/1841Z
leading to the single unsettled period of the day. Solar wind speed
at the ACE spacecraft continued to decline and ended the period near
440 km/s. The Bz component of the interplanetary magentic field
remained mostly neutral or positive. 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 quiet to unsettled for the next three days (10-12
June) with the anticiapted glancing blows from CMEs on 06 June and
08 June and the arrival on 11 June of a coronal hole high speed
stream.
III.  Event Probabilities 10 Jun-12 Jun
Class M    45/50/55
Class X    01/01/01
Proton     01/01/01
PCAF       Green
IV.  Penticton 10.7 cm Flux
Observed           09 Jun 128
Predicted   10 Jun-12 Jun  130/130/130
90 Day Mean        09 Jun 117
V.  Geomagnetic A Indices
Observed Afr/Ap 08 Jun  009/009
Estimated Afr/Ap 09 Jun  006/007
Predicted Afr/Ap 10 Jun-12 Jun  007/010-007/010-007/010
VI.  Geomagnetic Activity Probabilities 10 Jun-12 Jun
A.  Middle Latitudes
Active                20/20/20
Minor storm           10/10/10
Major-severe storm    01/01/01
B.  High Latitudes
Active                15/15/15
Minor storm           25/25/25
Major-severe storm    30/30/30
</pre>
    <br>
    <hr>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 the <a
      href="https://pss.swpc.noaa.gov">Product Subscription Site.</a>
    Please do not use the from address for correspondence, as it is not
    monitored. For comments or help, please contact <a
      href="mailto:pss.help@noaa.gov">SWPC Help.</a>
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