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Subject: Daily Summary of Solar Geophysical Activity for 26 May
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Date: Fri, 27 May 1994 12:17:15 MDT
From: oler@rho.uleth.ca (Cary Oler)
Newsgroups: rec.radio.amateur.misc,rec.radio.shortwave,rec.radio.info
Message-ID: <9405271817.AA00916@rho.uleth.ca>

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                 DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY

                                  26 MAY, 1994

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

                  (Based In-Part On SESC Observational Data)


SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 26 MAY, 1994
-------------------------------------------------------

!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 146, 05/26/94
10.7 FLUX=071.5  90-AVG=084        SSN=011      BKI=1343 2222  BAI=011
BGND-XRAY=A1.1     FLU1=1.6E+06  FLU10=1.3E+04  PKI=2344 2322  PAI=014
  BOU-DEV=006,021,047,033,018,015,010,013   DEV-AVG=020 NT     SWF=00:000
 XRAY-MAX= A7.9   @ 1430UT    XRAY-MIN= A1.0   @ 2354UT   XRAY-AVG= A2.1
NEUTN-MAX= +002%  @ 2235UT   NEUTN-MIN= -002%  @ 0705UT  NEUTN-AVG= -0.2%
  PCA-MAX= +0.1DB @ 2225UT     PCA-MIN= -0.2DB @ 2215UT    PCA-AVG= -0.0DB
BOUTF-MAX=55331NT @ 0005UT   BOUTF-MIN=55295NT @ 1714UT  BOUTF-AVG=55314NT
GOES7-MAX=P:+000NT@ 0000UT   GOES7-MIN=N:+000NT@ 0000UT  G7-AVG=+074,+000,+000
GOES6-MAX=P:+126NT@ 1803UT   GOES6-MIN=N:-078NT@ 0551UT  G6-AVG=+101,+030,-036
 FLUXFCST=STD:070,070,070;SESC:070,070,070 BAI/PAI-FCST=010,010,025/015,020,035
    KFCST=3324 4223 3324 4223  27DAY-AP=006,002   27DAY-KP=1231 1013 0110 1011
 WARNINGS=*GSTRM;*AURMIDWRN
   ALERTS=
!!END-DATA!!

NOTE: The Effective Sunspot Number for 25 MAY 94 was  25.4.
      The Full Kp Indices for 25 MAY 94 are: 3o 5+ 4- 4o   2- 3- 2o 4- 
      The 3-Hr Ap Indices for 25 MAY 94 are:  15  57  25  30   7  12   8  22 
      Greater than 2 MeV Electron Fluence for 26 MAY is: 4.3E+07


SYNOPSIS OF ACTIVITY
--------------------

            Solar activity was very low.  All regions were quiet.

            Solar activity forecast:  solar activity is expected to be
       very low.

            The geomagnetic field was quiet to active. Storm conditions
       occurred at some high latitude stations from 26/0600-1200Z.
       The greater than 2 MeV electron flux was moderate except for a
       5 hour period, from 26/0500-1000Z, when it was normal. (STD:
       Overall > 2 MeV electron fluence levels are near-normal.)

            Geophysical activity forecast:  the geomagnetic field is
       expected to be quiet to unsettled for the next two days. A
       recurrent disturbance is expected to start by the end of the
       third day.

            Event probabilities 27 may-29 may

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

            Geomagnetic activity probabilities 27 may-29 may

                        A.  Middle Latitudes
                        Active                15/30/30
                        Minor Storm           05/25/25
                        Major-Severe Storm    05/15/15

                        B.  High Latitudes
                        Active                15/30/30
                        Minor Storm           05/25/25
                        Major-Severe Storm    05/15/15

            HF propagation conditions were near-normal over most
       regions.  Minor signal degradation was observed over the high
       and polar latitude paths between 06:00 UTC and 12:00 UTC due to
       minor storming in those regions.  However, conditions returned
       to normal levels by 18:00 UTC.  Sporadic-E was also prevalent
       over some middle latitude stations.  No changes in propagation
       are expected over the next 24 to 48 hours.  The recurrent
       coronal hole disturbance noted above will begin degrading high
       and polar latitude signals on 29 May.  Thereafter, effects of
       this activity will spill over into the middle latitude regions.


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

REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 26/2400Z MAY
------------------------------------------------------
NMBR LOCATION  LO  AREA  Z   LL   NN MAG TYPE
7728  S07E38  323  0000 AXX  00  001 ALPHA
7727  N08W52  053                    PLAGE
REGIONS DUE TO RETURN 27 MAY TO 29 MAY
NMBR LAT    LO
NONE


LISTING OF SOLAR ENERGETIC EVENTS FOR 26 MAY, 1994
--------------------------------------------------
BEGIN  MAX  END  RGN   LOC   XRAY  OP 245MHZ 10CM   SWEEP
NONE


POSSIBLE CORONAL MASS EJECTION EVENTS FOR 26 MAY, 1994
------------------------------------------------------
 BEGIN        MAX      END     LOCATION   TYPE   SIZE  DUR  II IV
     NO EVENTS OBSERVED


INFERRED CORONAL HOLES. LOCATIONS VALID AT 26/2400Z
---------------------------------------------------
               ISOLATED HOLES AND POLAR EXTENSIONS
      EAST   SOUTH  WEST   NORTH  CAR  TYPE  POL  AREA   OBSN
                 NO DATA AVAILABLE FOR ANALYSIS


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

 Date   Begin  Max   End  Xray  Op Region  Locn    2695 MHz  8800 MHz  15.4 GHz
------  ----  ----  ----  ----  -- ------ ------  --------- --------- ---------
NO EVENTS OBSERVED.


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

                C   M   X     S   1   2   3   4   Total   (%)
               --  --  --    --  --  --  --  --    ---  ------
Uncorrellated: 0   0   0     0   0   0   0   0    000  ( 0.0)

 Total Events: 000 optical and x-ray.


EVENTS WITH SWEEPS AND/OR OPTICAL PHENOMENA FOR THE LAST UTC DAY
----------------------------------------------------------------

 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  **
