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Info-Hams Digest            Mon,  7 Mar 94       Volume 94 : Issue  257

Today's Topics:
       Daily Summary of Solar Geophysical Activity for 06 March

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Date: Mon, 7 Mar 1994 00:01:57 MST
From: ihnp4.ucsd.edu!swrinde!gatech!newsxfer.itd.umich.edu!nntp.cs.ubc.ca!alberta!ve6mgs!usenet@network.ucsd.edu
Subject: Daily Summary of Solar Geophysical Activity for 06 March
To: info-hams@ucsd.edu

                /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\

                 DAILY SUMMARY OF SOLAR GEOPHYSICAL ACT

                                 06 MARCH, 1994

                /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\

                  (Based In-Part On SESC Observational Data)


SOLAR AND GEOPHYSICAL ACT
---------------------------------------------------------

!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 065, 03/06/94
10.7 FLUX=095.5  90-AVG=106        SSN=101      BKI=2222 1223  BAI=007
BGND-XRAY=B1.2     FLU1=4.3E+06  FLU10=1.9E+04  PKI=2233 1223  PAI=009
  BOU-DEV=015,017,016,013,006,012,015,033   DEV-AVG=015 NT     SWF=00:000
 XRAY-MAX= C2.3   @ 1237UT    XRAY-MIN= A8.9   @ 0710UT   XRAY-AVG= B1.7
NEUTN-MAX= +002%  @ 1845UT   NEUTN-MIN= -002%  @ 2355UT  NEUTN-AVG= -0.2%
  PCA-MAX= +0.1DB @ 2320UT     PCA-MIN= -0.4DB @ 0850UT    PCA-AVG= -0.0DB
BOUTF-MAX=55342NT @ 2352UT   BOUTF-MIN=55315NT @ 1858UT  BOUTF-AVG=55324NT
GOES7-MAX=P:+000NT@ 0000UT   GOES7-MIN=N:+000NT@ 0000UT  G7-AVG=+072,+000,+000
GOES6-MAX=P:+141NT@ 1820UT   GOES6-MIN=N:-083NT@ 0357UT  G6-AVG=+092,+033,-032
 FLUXFCST=STD:098,100,101;SESC:098,100,101 BAI/PAI-FCST=020,025,025/025,030,030
    KFCST=3454 4433 4454 4444  27DAY-AP=054,056   27DAY-KP=4647 65*3 6566 6455
 WARNINGS=*GSTRM;*AURMIDWCH
   ALERTS=
!!END-DATA!!

NOTE: The Effective Sunspot Number for 05 MAR 94 is not available.
      The Full Kp Indices for 05 MAR 94 are: 1+ 1- 1+ 2-   1o 1- 2- 3- 
      The 3-Hr Ap Indices for 05 MAR 94 are:   5   3   5   6   4   3   6  11 
      Greater than 2 MeV Electron Fluence for 06 MAR is: 7.5E+06


SYNOPSIS OF ACT
--------------------

       SUMMARY COVERS THE PERIOD FROM 05/2100Z TO 06/2100Z:

             Solar activity was low.  An optically uncorrelated C2
       x-ray event was recorded at 06/1237Z.  Region 7682 (S19W81) has
       declined in area and spot number and produced no activity this
       period.  Regions 7680 (S11W29) and 7685 (S08E09) were the most
       active producing numerous B-class/SF flares.  Two new regions
       were numbered this period:  Region 7686 (N08W46) and Region
       7687 (N18E16).  Since appearing on the disk, both new regions
       have shown white light growth.  All other regions are quiet and
       stable.

            Solar activity forecast:  solar activity is expected to be
       very low to low.  Regions 7685,7686, and 7687 all have the
       potential for producing C-class activity.

            The geomagnetic field has been at mostly quiet to unsettled
       levels the past 24 hours.

            Geophysical activity forecast:  the geomagnetic field is
       expected to be mostly unsettled to active for the next three
       days with minor storm conditions expected at high latitudes on
       days two and three.

       STD: Levels of geomagnetic activity have increased to active
       levels just prior to the release of this report (early on 07
       March).  It would appear that the coronal-hole related
       disturbance has arrived.  Minor storming has been observed over
       many high latitude sites over the last 3 hours (07/00Z to 03Z).
       Levels of auroral activity have likewise increased with only a
       slight equatorward migration of the northern oval apparent at
       the present time.  Local night-sector substorming should
       produce moderate levels of auroral activity over the next
       several days.

            Event probabilities 07 mar-09 mar

                             Class M    05/05/05
                             Class X    01/01/01
                             Proton     01/01/01
                             PCAF       Green

            Geomagnetic activity probabilities 07 mar-09 mar

                        A.  Middle Latitudes
                        Active                20/25/25
                        Minor Storm           15/25/30
                        Major-Severe Storm    10/15/15

                        B.  High Latitudes
                        Active                25/30/35
                        Minor Storm           20/30/35
                        Major-Severe Storm    10/20/20

            HF propagation conditions were normal over all regions.
       Some regions experienced notable enhancements in both signal
       quality and MUF.  Conditions are presently (early on 07 March)
       beginning to wane, with poor propagation being observed over
       some high latitude sites.  Poor to very poor propagation is
       expected over the next 48 to 72 hours on transpolar and
       transauroral circuits.  Middle latitudes should see good to
       fair propagation with occasional night-sector poor propagation.
       No improvements are expected for at least the next 48 to 72
       hours.


COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS
========================================================

REGIONS WIT
--------------------------------------------------------
NMBR LOCATION  LO  AREA  Z   LL   NN MAG TYPE
7680  S11W29  020  0000 BXO  02  002 BET
7682  S19W81  073  0100 CAO  11  007 BET
7684  S08W16  007  0010 BXO  03  003 BET
7685  S08E09  342  0100 DAO  07  014 BET
7686  N08W46  037  0030 CRO  04  005 BET
7687  N18E16  335  0040 BXO  04  010 BET
7678  S11W52  043                    PLAGE
REGIONS DUE TO RET
NMBR LAT
NONE


LISTING OF SOLAR ENERGETIC EVENTS FOR 06 MARCH, 1994
----------------------------------------------------
BEGIN  MAX  END  RGN   LOC   XRAY  OP 245MHZ 10CM   SWEEP
NONE


POSSIBLE CORONAL MASS EJECTION EVENTS FOR 06 MARCH, 1994
--------------------------------------------------------
 BEGIN        MAX      END     LOCATION   TYPE   SIZE  DUR  II IV
06/ 1752             B1818       N17E23   DSF    B2.9   24


INFERRED CORONAL HOLES. LOCATIONS VALID AT 06/2400Z
---------------------------------------------------
               ISOLATED HOLES AND POLAR EXT
      EAST   SOUTH  WEST   NORTH  CAR  TYPE  POL  AREA   OBSN
          NONE VISIBLE


SUMMARY OF FLARE EVENTS FOR THE PREVIOUS UTC DAY
------------------------------------------------

 Date   Begin  Max   End  Xray  Op Region  Locn    2695 MHz  8800 MHz  15.4 GHz
------  ----  ----  ----  ----  -- ------ ------  --------- --------- ---------
05 Mar: 0000  0003  0006  B4.3                                         
        0348  0352  0354  B2.5                                         
        1211  1223  1241  B3.7  SF  7682  S17W66                       
        1350  1351  1354  B1.6  SF  7680  S13W08                       
        1848  1851  1853  B2.7                                         
        2229  2230  2235        SF  7680  S11W14                       
        2301  2304  2306  B2.4                                         


REGION FLARE STATISTICS FOR THE PREVIOUS UTC DAY
------------------------------------------------

                C   M   X     S   1   2   3   4   Total   (%)
               --  --  --    --  --  --  --  --    ---  ------
  Region 7680:  0   0   0     2   0   0   0   0    002  (28.6)
  Region 7682:  0   0   0     1   0   0   0   0    001  (14.3)
Uncorrellated: 0   0   0     0   0   0   0   0    004  (57.1)

 Total Events: 007 optical and x-ray.


EVENTS WIT
----------------------------------------------------------------

 Date   Begin  Max   End  Xray  Op Region  Locn    Sweeps/Optical Observations
------  ----  ----  ----  ----  -- ------ ------   ---------------------------
                            NO EVENTS OBSERVED.

NOTES:
     All times are in Universal Time (UT).  Characters preceding begin, max,
     and end times are defined as:  B = Before,  U = Uncertain,  A = After.
     All times associated with x-ray flares (ex. flares which produce
     associated x-ray bursts) refer to the begin, max, and end times of the
     x-rays.  Flares which are not associated with x-ray signatures use the
     optical observations to determine the begin, max, and end times.

     Acronyms used to identify sweeps and optical phenomena include:

          II        = Type II Sweep Frequency Event
          III       = Type III Sweep
          IV        = Type IV Sweep
          V         = Type V Sweep
          Continuum = Continuum Radio Event
          Loop      = Loop Prominence System,
          Spray     = Limb Spray,
          Surge     = Bright Limb Surge,
          EPL       = Eruptive Prominence on the Limb.


**  End of Daily Report  **

------------------------------

End of Info-Hams Digest V94 #257
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