Date: Sun, 28 Nov 93 01:10:50 PST
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Subject: Info-Hams Digest V93 #1395
To: Info-Hams


Info-Hams Digest            Sun, 28 Nov 93       Volume 93 : Issue 1395

Today's Topics:
                           Calculating SWR
     Daily Summary of Solar Geophysical Activity for 20 November
     Daily Summary of Solar Geophysical Activity for 26 November
                    Email callbook server (2 msgs)
             How useful are DSP units in noisy locations?
                        Mag Mount Paint Damage
                 Modem Software to Alert Many Pagers?

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We trust that readers are intelligent enough to realize that all text
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policies or positions of any party.  Your mileage may vary.  So there.
----------------------------------------------------------------------

Date: Sat, 27 Nov 1993 18:48:05 GMT
From: yuma!galen@purdue.edu
Subject: Calculating SWR
To: info-hams@ucsd.edu

In article <1993Nov26.200816.19512@combdyn.com> lawrence@combdyn.com (Lawrence *The Dreamer* Chen) writes:
>How do you calculate SWR?  I have a power meter...and I can measure the forward
>and reflected power.  How to I take the two values to determine the SWR?

         1+SQRT(Wr/Wf)
VSWR=   _______________
  1-SQRT(Wr/Wf)

Where SQRT denotes the square root of (this), Wr is reflected power and
      Wf is forward power.

>Right now I have forward power of 5 Watts and reflected power of 0.1 Watts,
>what SWR would that correspond to?

I get 1.329:1  .

Galen, KF0YJ

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

Date: Sat, 20 Nov 1993 21:55:55 MST
From: dog.ee.lbl.gov!agate!usenet.ins.cwru.edu!magnus.acs.ohio-state.edu!math.ohio-state.edu!cyber2.cyberstore.ca!nntp.cs.ubc.ca!alberta!adec23!ve6mgs!usenet@network.ucsd.edu
Subject: Daily Summary of Solar Geophysical Activity for 20 November
To: info-hams@ucsd.edu

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

                 DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY

                                20 NOVEMBER, 1993

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

                  (Based In-Part On SESC Observational Data)


SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 20 NOVEMBER, 1993
------------------------------------------------------------

!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 324, 11/20/93
10.7 FLUX=100.5  90-AVG=094        SSN=058      BKI=3312 1221  BAI=007
BGND-XRAY=B1.5     FLU1=3.7E+05  FLU10=1.2E+04  PKI=3411 2222  PAI=009
  BOU-DEV=021,026,006,012,009,010,010,007   DEV-AVG=012 NT     SWF=00:000
 XRAY-MAX= C5.2   @ 0032UT    XRAY-MIN= B1.2   @ 1919UT   XRAY-AVG= B4.0
NEUTN-MAX= +002%  @ 0945UT   NEUTN-MIN= -002%  @ 1145UT  NEUTN-AVG= -0.3%
  PCA-MAX= +0.1DB @ 1215UT     PCA-MIN= -0.1DB @ 1900UT    PCA-AVG= +0.0DB
BOUTF-MAX=55364NT @ 0231UT   BOUTF-MIN=55346NT @ 1952UT  BOUTF-AVG=55355NT
GOES7-MAX=P:+000NT@ 0000UT   GOES7-MIN=N:+000NT@ 0000UT  G7-AVG=+066,+000,+000
GOES6-MAX=P:+128NT@ 1836UT   GOES6-MIN=N:-070NT@ 0951UT  G6-AVG=+087,+019,-038
 FLUXFCST=STD:105,110,110;SESC:105,110,110 BAI/PAI-FCST=010,010,020/012,015,035
    KFCST=1115 4000 1112 2111  27DAY-AP=009,029   27DAY-KP=4222 1221 2235 6533
 WARNINGS=*SWF
   ALERTS=**245STRM:0613-0817UTC
!!END-DATA!!

NOTE: The Effective Sunspot Number for 19 NOV 93 was  25.0.
      The Full Kp Indices for 19 NOV 93 are: 3+ 6- 2- 2o   3- 4- 3- 3o



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

             Solar activity was low.  Region 7618 (N07W31) remains the
       most impressive area on the disk.  In white light, the region
       has decreased in area and spot number, but still retains its
       beta-delta configuration.  New Region 7621 (S09E48) was
       numbered overnight.  An area of interest to watch is on the
       east limb at N12 where an impressive bright surge was reported
       by Learmonth last night.  All other areas/regions were stable.

            Solar activity forecast:  solar activity is expected to be
       low to moderate with Region 7618 the most likely candidate to
       produce C and M-class activity.  A new, active region may rotate
       into view over the next few days and could also contribute to
       activity.

       STD: X-ray imagery from the Yohkoh satellite showed a fairly
       strong and bright loop system at about 02:50 UTC from the
       region just beyond the east limb. A Yohkoh full-disk x-ray
       image showing the enhanced northeast limb emissions has been
       appended to this report.

            The geomagnetic field has been at mostly unsettled levels.
       Since 09Z, the middle latitude field has been at quiet levels.

            Geophysical activity forecast:  the geomagnetic field is
       expected to be at mostly unsettled levels for the first two
       days of the period with active to minor storm conditions
       expected early on day three due to a favorably located coronal
       hole.  The disturbance is expected to last only one day with
       levels forecasted to decrease to mostly unsettled thereafter.

            Event probabilities 21 nov-23 nov

                             Class M    50/50/50
                             Class X    05/05/05
                             Proton     05/05/05
                             PCAF       Green

            Geomagnetic activity probabilities 21 nov-23 nov

                        A.  Middle Latitudes
                        Active                20/25/35
                        Minor Storm           10/10/20
                        Major-Severe Storm    01/05/10

                        B.  High Latitudes
                        Active                25/30/40
                        Minor Storm           10/15/30
                        Major-Severe Storm    01/10/15

            HF propagation conditions were near-normal over the low
       and middle latitude paths.  High and polar latitude paths
       experienced additional periods of below-normal propagation due
       primarily to periods of enhanced geomagnetic and auroral
       activity within the auroral zone.  Conditions improved notably
       by the end of the day.  Propagation conditions are expected to
       continue near-normal over the next 48 hours (through about
       22 November inclusive).  Activity could become gradually
       enhanced during the latter half of 22 November.  On
       23 November, a recurrent coronal hole is expected to increase
       levels of geophysical activity to near-storm levels which
       is expected to cause below-normal (poor to occasionally very
       poor) propagation for transpolar and transauroral paths.
       Middle-latitude night-sector paths may also be affected on
       22 November.


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

REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 20/2400Z NOVEMBER
-----------------------------------------------------------
NMBR LOCATION  LO  AREA  Z   LL   NN MAG TYPE
7618  N08W31  338  0580 DKI  08  026 BETA-DELTA
7620  N04E43  264  0000 AXX  01  001 ALPHA
7621  S10E49  258  0000 AXX  00  001 ALPHA
REGIONS DUE TO RETURN 21 NOVEMBER TO 23 NOVEMBER
NMBR LAT    LO
NONE


LISTING OF SOLAR ENERGETIC EVENTS FOR 20 NOVEMBER, 1993
-------------------------------------------------------
BEGIN  MAX  END  RGN   LOC   XRAY  OP 245MHZ 10CM   SWEEP SWF
     NO EVENTS OBSERVED


POSSIBLE CORONAL MASS EJECTION EVENTS FOR 20 NOVEMBER, 1993
-----------------------------------------------------------
 BEGIN        MAX      END     LOCATION   TYPE   SIZE  DUR  II IV
20/ 0338     0403     0444       N08W20   LDE    C1.3   66


INFERRED CORONAL HOLES. LOCATIONS VALID AT 20/2400Z
---------------------------------------------------
               ISOLATED HOLES AND POLAR EXTENSIONS
      EAST   SOUTH  WEST   NORTH  CAR  TYPE  POL  AREA   OBSN
48   S42W53 S44W61 S09W90 S09W90  023  ISO   NEG   010 10830A
49   N30E05 N18W04 N25W13 N38W05  316  ISO   POS   005 10830A


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

 Date   Begin  Max   End  Xray  Op Region  Locn    2695 MHz  8800 MHz  15.4 GHz
------  ----  ----  ----  ----  -- ------ ------  --------- --------- ---------
19 Nov: 0337  0342  0344  B3.1  SF  7618  N09W07                       
        0359  0404  0408  B3.2                                         
        0710  0759  0828  B8.9                                         
        1845  2004  2051  B9.8                                         
       B2007 U2009 A2015        SF  7618  N12W12                       


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

                C   M   X     S   1   2   3   4   Total   (%)
               --  --  --    --  --  --  --  --    ---  ------
  Region 7618:  0   0   0     2   0   0   0   0    002  (40.0)
Uncorrellated: 0   0   0     0   0   0   0   0    003  (60.0)

 Total Events: 005 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.


SPECIAL INSERT: CURRENT X-RAY EMISSIONS FROM THE JAPANESE YOHKOH SPACECRAFT
===========================================================================

                     20 November 1993, 02:50 UTC

                                    North
    ..   .     . .                  .....         ................
 ..................              .,,,,,,,,......,,:::::::::,:,,,......         
.....,...,,,,,,::,,,,,..,..      .,,,,,,,,,,,,,,:::::::::;;::::,,,,.....       
.,,,,::,,,,,:::::;;;:,,,... ..........,.,,,,,,,,,,,,,,,:,::;;;;::,,,.....      
,,::::;::::::::;;;;:::,.. ... ..........,,,,,,,,,,,,,.,,,,,,,:::::::,,,....    
::::;;;;;;;;;;;;;::::::,......   ...,,,,:,,,,,,,,,:,,,,,,,,,,,::;;;:::,,,,.....
:;;;----------;::::,,::,,,.....  .,.,,::::::::::::::::,,,,,,,,:::;;;;;:::,,,,..
;;--+++++|++-;:::,,,::,,,,..  . . ....,:::;;;;---;;;;::,:,,,:,:::::;--;;;::,,,.
;--++||||||-;;:::;:,,,,,,... ...., . ..,::;;-+++++---;;:::::::::;:;:;-+-;;;::,,
-+++|!111!+-;;;;::::,,,,,,............,,,,:;-+|!!!|++---;;;;;;;;;;;;;;-+--;:::,
|!124*##4|+--;;;:::::,,,,.,:,,,,,,,,.,,,:+!!+;-!221!!|----;;;;;;;---;;;---;;;::
13*@@@@@4|+----;;;:::,,,,,,,,,,,,,,,,,::::;+-;;-1432!!|++---;;;;;;;;;;;;+++-;;:
4*#@@@@@1|++----;-;:::,,,,,,,,,,,,,:::::::;;;;--!24**32++++--;;;;--;;;;;+!|+-;;
123*#@@3!!!|||--;;;;:,,,,,.,,,,,,,,--:::::::;;-+!4@@@*!|++----;;-++--;;;-||+--;
||!1233|||2!3+-;;;;;:,,,,,,,,,,,,,,,,,,,::::;-++|1#@#2|+-------;--------+||++--
--+++||---++-;::::;;:,,,,,,:,,,,,,,,,,,,,,::;-+|!112!|+------;;;;;;;;--+-|++---
;;;----;;;;;;::::,:::,,,,,,,,,,,,,,,,,,,,,::;;-+||||||+;;;;--;;;-----+---+++--;
:;;;---;;;+-:::::::::,,,,,,,,,,,,,,,,,,,.,:::::;;-;;;;;;;-;;;;----++||+--++--;;
:::;;;--:;+|::::;;:,,::,::,,.,,,,:,,.,,,.,,,,,,:::::;;-+-;;;;----;-+||-;+|+-;;;
,:::;;;-;:::,:,,,,,,,,,,,,,,..,,,,:::,,......,,,,,,:::;;;::::;-;;-+|+;:-||+-;;;
,,::;;;;-;::,,,,,,,,,,,,,,,,.,,,,,,,,,,,.....,..,,,,:;;:::::;;----;:,:;||+--;;:
,,:::;;;;-;::,,,,,,,,,,,,,,,,,,,,,,............,,,,,,,,:;;;;;;;;::,,:;||++-;;;:
.,,,::;;;;-;:;::::,,,,,,,,,,,,,,,..............,,,,,,,:,:::;;;;:,,,:-++++--;;::
..,,,::::;;;--:::::,,,....,,.,...,...............,,,,,,,,::::::,,:;+++---;;;::,
...,,,:::::;;;;;::,,,,,,,,,,,,,,,...........  . ..,,,,,..,,,....,;-----;;:::,,,
 ....,,,,:::;;;--;::,,,,,,.,,,,,.........         .... .. ..,.,;;;;;;;:::,,,,..
   .....,,,:::;;;;;::....   ..,,.....               .......:;-;;;:::::,,,,.....
    ........,,,,:::::::,,       .              .    . .,:;----;::::::,,,.....  
      . .......,,,,,,,,,,,,,...                  ..,:;;----;;;;::::,,,,...     
            ..............,,,................,,,::::;;;;;:::::::,,,,....       
                      .. ..           .. ...  .  ...,,,,,,,,,,,,....           
                                                    ...........                

                                    South

KEY: East and west limbs are to the left and right respectively. Emission
     strength, from minimum to maximum are coded in the following way:

     [space] . , : ; - + | ! 1 2 3 4 * # @

     Units used are arbitrary, for illustrative purposes.  Get "showasc.zip"
     from "pub/solar/Software" at the anonymous FTP site: xi.uleth.ca
     (IP # 142.66.3.29) to view these images on VGA screens.


**  End of Daily Report  **

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

Date: Fri, 26 Nov 1993 20:54:14 MST
From: swrinde!cs.utexas.edu!uwm.edu!spool.mu.edu!agate!library.ucla.edu!news.mic.ucla.edu!unixg.ubc.ca!kakwa.ucs.ualberta.ca!alberta!ugc!nebulus!ve6mgs!usenet@network.ucsd.edu
Subject: Daily Summary of Solar Geophysical Activity for 26 November
To: info-hams@ucsd.edu

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

                 DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY

                                26 NOVEMBER, 1993

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

                  (Based In-Part On SESC Observational Data)


SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 26 NOVEMBER, 1993
------------------------------------------------------------

!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 330, 11/26/93
10.7 FLUX=093.2  90-AVG=094        SSN=052      BKI=2222 2242  BAI=009
BGND-XRAY=B1.5     FLU1=9.2E+05  FLU10=1.3E+04  PKI=2212 2342  PAI=009
  BOU-DEV=018,012,013,010,015,018,043,017   DEV-AVG=018 NT     SWF=00:000
 XRAY-MAX= C2.1   @ 1606UT    XRAY-MIN= B1.3   @ 2328UT   XRAY-AVG= B2.3
NEUTN-MAX= +002%  @ 2155UT   NEUTN-MIN= -002%  @ 1810UT  NEUTN-AVG= -0.1%
  PCA-MAX= +0.2DB @ 1545UT     PCA-MIN= -0.3DB @ 2135UT    PCA-AVG= +0.1DB
BOUTF-MAX=55364NT @ 1344UT   BOUTF-MIN=55333NT @ 1826UT  BOUTF-AVG=55357NT
GOES7-MAX=P:+000NT@ 0000UT   GOES7-MIN=N:+000NT@ 0000UT  G7-AVG=+064,+000,+000
GOES6-MAX=P:+130NT@ 1742UT   GOES6-MIN=N:-055NT@ 0825UT  G6-AVG=+085,+016,-028
 FLUXFCST=STD:095,090,090;SESC:095,090,090 BAI/PAI-FCST=005,005,005/010,010,010
    KFCST=3122 2112 3212 2122  27DAY-AP=005,007   27DAY-KP=2121 2122 1132 2223
 WARNINGS=*SWF
   ALERTS=
!!END-DATA!!

NOTE: The Effective Sunspot Number for 25 NOV 93 was  42.0.
      The Full Kp Indices for 25 NOV 93 are: 2- 1+ 1o 0+   2- 2o 2- 3-


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

             Solar activity was low with several C-class flares
       observed.  New Region 7623 (S11E67) rotated onto the disk and
       produced a C2/SF flare at 26/1605Z.  Region 7620 (N04W40)
       produced a C1 flare at 26/1712Z.  All regions appear to be
       stable.

            Solar activity forecast:  solar activity is expected to be
       at low levels during the period.

       STD: The latest Yohkoh image has been appended to this report.

            The geomagnetic field has been at quiet levels for
       the past 24 hours.  High latitudes reported isolated
       undettled levels during the period.

            Geophysical activity forecast:  the geomagnetic field is
       expected to be at quiet to unsettled levels.

            Event probabilities 27 nov-29 nov

                             Class M    10/10/10
                             Class X    01/01/01
                             Proton     01/01/01
                             PCAF       Green

            Geomagnetic activity probabilities 27 nov-29 nov

                        A.  Middle Latitudes
                        Active                05/05/05
                        Minor Storm           05/05/05
                        Major-Severe Storm    01/01/01

                        B.  High Latitudes
                        Active                05/05/10
                        Minor Storm           01/05/05
                        Major-Severe Storm    01/01/01

            HF propagation conditions were normal over all regions.
       No changes are expected over the next three days, through 29
       November inclusive.  Normal propagation should persist over all
       regions.


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

REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 26/2400Z NOVEMBER
-----------------------------------------------------------
NMBR LOCATION  LO  AREA  Z   LL   NN MAG TYPE
7620  N04W40  268  0280 ESI  12  017 BETA
7622  N13E06  222  0040 CSO  03  004 BETA
7623  S11E67  161  0030 HAX  01  001 ALPHA
7621  S09W30  258                    PLAGE
REGIONS DUE TO RETURN 27 NOVEMBER TO 29 NOVEMBER
NMBR LAT    LO
NONE


LISTING OF SOLAR ENERGETIC EVENTS FOR 26 NOVEMBER, 1993
-------------------------------------------------------
BEGIN  MAX  END  RGN   LOC   XRAY  OP 245MHZ 10CM   SWEEP
NONE


POSSIBLE CORONAL MASS EJECTION EVENTS FOR 26 NOVEMBER, 1993
-----------------------------------------------------------
 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
51   S01E47 S13E32 N15E15 N35E42  202  ISO   POS   023 10830A


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

 Date   Begin  Max   End  Xray  Op Region  Locn    2695 MHz  8800 MHz  15.4 GHz
------  ----  ----  ----  ----  -- ------ ------  --------- --------- ---------
25 Nov: 0009  0020  0037  C1.0  SF  7620  N04W14                       
        0105  0105  0112        SF  7620  N05W14                       
        0116  0117  0124        SF  7620  N03W15                       
        0138  0145  0204  B9.7  SF  7620  N05W14                       
        0343  0357  0406  C2.6                                         
        0458  0518  0527        SF  7620  N03W15                       
        0534  0540  0555  C1.2  1N  7620  N03W17                       
        0614  0621  0625  C5.7                                         
        0805  0809  0815  C2.1  SF  7620  N03W17                       
        0902  0912  0918  C1.9  SF  7620  N04W19                       
        1214  1223  1231  B7.5                                         
        1744  1754  1803  B3.9                                         
        2020  2027  2037  C1.8  SF  7620  N04W24                       
        2251  2254  2256  B2.7                                         


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

                C   M   X     S   1   2   3   4   Total   (%)
               --  --  --    --  --  --  --  --    ---  ------
  Region 7620:  5   0   0     8   1   0   0   0    009  (64.3)
Uncorrellated: 2   0   0     0   0   0   0   0    005  (35.7)

 Total Events: 014 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
------  ----  ----  ----  ----  -- ------ ------   ---------------------------
25 Nov: 0614  0621  0625  C5.7                     III

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.


SPECIAL INSERT: CURRENT X-RAY EMISSIONS FROM THE JAPANESE YOHKOH SPACECRAFT
===========================================================================

                     26 November 1993, 02:00 UTC

                                    North
                                 .          .................  .
                          ....,...,.......... .....,:,:,,,,,,,,,......         
                      .....,.,,,,,,,,,,,,,,,.,........,,:::::::,,,,.....       
         ....  .........,,.,,,,,,,,,,,,,,,,,,,,,,,..,...,,,::::::,,,,,.......  
     .......,,,,,,.  ....,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,...,,:;::::,,,,,,,....
    .....,,,::::,..  ...,,,:,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,..,:;;:::::::,,,,.
 ...,,,,,:-+-:;:,......,::::::::::,,,::,,,,,,,,,,,,,,,,,,,,,,,,,,,:;;--;;;;:::,
..,,,,:::-|!|;:,,... ..,::;;:;;::::::::::::,,,,,,,,,,,,,,:,,:::::,,:-++++++--;:
,,:::::;;-|21-:,... ...,,:;;-------;::::::::,:,,,:,,,,,,,,,,,::::::::+!!||+-;;:
.,::;;;;;;;-;:.. .....,,,:;---+||+++-;;::::::::,:,::,:,:::::::::::::::+!!!|-;;:
,,:::;;;:,,...    ....,,,::;+++|!!|+++-;;;;;::::::;;;;;:;;::::::::::::;!21+-;;;
,,::;;;;,.. ..  ....,,,,,:;-4331!!||++---;;;;;;;;;;;;---+++-;:::::::;:;-221!||+
,::;;;-;,. .  ...,,,,::::;;|21!|||++++-----;--++-----+|!!|+|-;;::::::;;-3*31|||
::;;---;,. .. ..,,,,:,,::;;--------;;::;;;;;--++++--+|24*3!++-;;:::::;;+1#3!+--
;;--+++-:.......,,,,,,,::;;;;;;;;;;;;:;;::::;-++++--+3@@@3!++-;::::::;;-|431!+;
;--+|!!-:.......,,,,,,,,::::::::::::::::::,::;;;;;;-+!122!!-;;;:::,::::;-|!|+-;
-+|!122|:,,,...,,,,,:,,,,,,,,,,,,::,,,,,,,,,,::::;;;-||||!|;::::::,:::;;-+--;;:
-++!123!-;;:;:,,,:::::,,,,,,,,,,,,,,,,,,,,,,,,::;;;:;;;---;;::,,,,,::::;--;;:,,
;-++!122|+--++:,:::::,,,,,,,,,,,,,,,,,,,,....,:::-+:,:::::::,,,,,,,,,::;-;::,,,
;;;+|!11!+++||-;;;::,,,,,,,,..,.,.,,.,........,,,:,,,,,,,,,,,,,,,,,,:::-;:,,,,,
::;++|!!|++!1!-;;;::,,,....................,...,........,,,,,,,,,,,,::;;:,,,...
.,;;----++---;;-;;::,,,................................,,,,,,,,,,,,,:;;::,,....
.,::;;;------;;;;::::,,,.,,.,,................,...,,,,,,,,,,,,,,,,,:;;::,,.....
.,,:::;;;-----;:::,,,,,,,........................,,,,,,,....,.,,,:::::,,,..... 
.,,,::::;;;;;;;;::,,,,,,......................,..........,,,,,,,::,,,,....     
..,,,,:::::::;;;;;::,,,.......,,,..,,...,...,,,,,,,,,,,,,,,,,,,,,....          
 ...,,,,,,::::;;;;;;;:,,,...  .  .........,...............,,,...               
 .....,,,,,::::;;;-----;;:,.              .            ...                     
 .......,,,,,::;;;;;;;;;;::,..                ...                              
   .......,,,,,,,:::::,,,...             .........                             
    ...................                                                        
     ..                                                                        

                                    South

KEY: East and west limbs are to the left and right respectively. Emission
     strength, from minimum to maximum are coded in the following way:

     [space] . , : ; - + | ! 1 2 3 4 * # @

     Units used are arbitrary, for illustrative purposes.  Get "showasc.zip"
     from "pub/solar/Software" at the anonymous FTP site: xi.uleth.ca
     (IP # 142.66.3.29) to view these images on VGA screens.


**  End of Daily Report  **

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

Date: 28 Nov 93 06:24:50 GMT
From: ogicse!uwm.edu!cs.utexas.edu!howland.reston.ans.net!noc.near.net!news.delphi.com!usenet@network.ucsd.edu
Subject: Email callbook server
To: info-hams@ucsd.edu

In the last message I said that he (ko4rk, aka 44.62.0.122) might not
pick up an Internet message from an .ampr. source. That should have read
a NON-.ampr. source, that is, not from a packet BBS.
 
Also, there are other REQQTH servers all over the place. This  is the only
one I am sure of.
 
Again, hope  this helps.
Jason!

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

Date: 28 Nov 93 06:19:52 GMT
From: ogicse!uwm.edu!cs.utexas.edu!howland.reston.ans.net!noc.near.net!news.delphi.com!usenet@network.ucsd.edu
Subject: Email callbook server
To: info-hams@ucsd.edu

The only  E-mail servers I know of are available on packet BBSs. You may
want to try the following (It might work):
send a message to REQQTH@44.62.0.122  and in the SUBJECT of the message,
put the callsign(s) of the station(s) you are looking for, separated
only by spaces. Put nothing in the actual text section.
 
I'm not  sure if he will pick up an Internet message from a .ampr. source,
but it might be worth a shot. You might also try a telnet to
plan9.njit.edu 2000 or mudgate.imsa.edu 2000.
 
I hope I've answered your question with at least one of the options.
 
-=*>Jason!<*=-
JTRIOLO@delphi.com
kd4acg@k9iu.ampr.org (k9iu.#sin.in.usa.na)
kd4acg@wa4ong.ampr.org (wa4ong.va.usa.na)

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

Date: 25 Nov 1993 16:22:58 GMT
From: munnari.oz.au!sgiblab!swrinde!gatech!usenet.ufl.edu!mailer.acns.fsu.edu!freenet2.scri.fsu.edu!friederw@network.ucsd.edu
Subject: How useful are DSP units in noisy locations?
To: info-hams@ucsd.edu

NIR-10 does a really good job for me here in Tallahassee.  The recent
firmware upgrade did wonders for it--QRN almost disappears!     73
-- 
**********************************************************************************************
William A. "Bill" Frieder  friederw@freenet.tlh.fl.us
N4QNF  Packet Mail =  N4QNF @ W1FJI 
(904) 488-2381 days     (904) 893-3738 till 9:30 P.M. EDT

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

Date: Fri, 26 Nov 1993 21:49:00 GMT
From: pacbell.com!UB.com!wetware!rhohan!express@ames.arpa
Subject: Mag Mount Paint Damage
To: info-hams@ucsd.edu

SMK>From: sknapp@iastate.edu (Steven M. Knapp) SMK>Organization: Iowa State University, Ames, IA SMK>In article <CGx7KB.FHq@srgenprp.sr.hp.com> alanb@sr.hp.com (Alan SMK>Bloom) writes: SMK>>David Van Nuys (vannuysd@sonoma.edu) wrote: SMK>>: I notice that my two-meter mag mount is leaving rings on the paint SMK>of my SMK>>: trunk.  Has anyone got any tips for preserving the paint and still SMK>using SMK>>: a mag mount?  Try putting the base of the antenna into a plastic sandwich bag and
e car. Steve Fleckenstein  - Red Onion Express BBS - 914-342-4585  * OLX 2.1 TD * Paper clips are the larval stage of coat hangers. --- RBBSMail v18.2  * Origin: Red Onion, Express  Wawayanda,New York  914 342 4585 (100:911/7.0)

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

Date: 22 Nov 1993 03:05:00 GMT
From: dog.ee.lbl.gov!agate!howland.reston.ans.net!cs.utexas.edu!geraldo.cc.utexas.edu!slip-3-1.ots.utexas.edu!user@network.ucsd.edu
Subject: Modem Software to Alert Many Pagers?
To: info-hams@ucsd.edu

Our local Amateur Radio Emergency Service (ARES) group needs some software
that could notify all our pager-carrying members when an emergency happens.

Many of our members carry pagers for their jobs, and most of these are
digital pagers. We need an application that would go down a list of pager
phone numbers, dialing each, waiting until the phone is answered, then
sending the TouchTones (r) for "14694". This number would be recognized by
our members as meaning 146.94 MHz, the local ARES repeater frequency.

Has anyone seen an app (for PC or Mac) that can do this? Thank you.

= = = = = = = = = = = = = = = = = = = =
  _     Miles Abernathy, N5KOB        =
 | |__  miles@mbs.telesys.utexas.edu  =
_|    | POB 7580, Austin TX 78713     =
\  * /  University of Texas @ Austin  =
  \/    tel. (512) 471-6521  U.S.A.   =
= = = = = = = = = = = = = = = = = = = =

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

End of Info-Hams Digest V93 #1395
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