home
***
CD-ROM
|
disk
|
FTP
|
other
***
search
/
QRZ! Ham Radio 4
/
QRZ Ham Radio Callsign Database - Volume 4.iso
/
digests
/
infoham
/
940656.txt
< prev
next >
Wrap
Internet Message Format
|
1994-11-13
|
27KB
Date: Sun, 12 Jun 94 22:01:06 PDT
From: Info-Hams Mailing List and Newsgroup <info-hams@ucsd.edu>
Errors-To: Info-Hams-Errors@UCSD.Edu
Reply-To: Info-Hams@UCSD.Edu
Precedence: Bulk
Subject: Info-Hams Digest V94 #656
To: Info-Hams
Info-Hams Digest Sun, 12 Jun 94 Volume 94 : Issue 656
Today's Topics:
440 in So. Cal.
<<Best dual band verticals?>>
ANS-162 BULLETINS
Any Ham in CASARA ?
Beware of RADIOKIT kits (IMHO) (2 msgs)
Daily Summary of Solar Geophysical Activity for 11 June
HTX 202 (2 msgs)
IPS Daily Report - 12 June 94
Send Replies or notes for publication to: <Info-Hams@UCSD.Edu>
Send subscription requests to: <Info-Hams-REQUEST@UCSD.Edu>
Problems you can't solve otherwise to brian@ucsd.edu.
Archives of past issues of the Info-Hams Digest are available
(by FTP only) from UCSD.Edu in directory "mailarchives/info-hams".
We trust that readers are intelligent enough to realize that all text
herein consists of personal comments and does not represent the official
policies or positions of any party. Your mileage may vary. So there.
----------------------------------------------------------------------
Date: 12 Jun 1994 21:27:20 -0700
From: news.claremont.edu!kaiwan.com!not-for-mail@uunet.uu.net
Subject: 440 in So. Cal.
To: info-hams@ucsd.edu
Brian Suggs (suggs@tcville.es.hac.com) wrote:
> I've been following this thread with some interest from the point of view
> of someone who will be a newcomer on the airwaves. (I'm taking the license
> exams this weekend.) From what I understand, as far as the FCC is concerned,
> a coordinated repeater has preference over an uncoordinated one should they
> be interfering with each other, and that is all. My question is this: Who
> are the coordinating bodies and how are they appointed. Is there any official
> (FCC recognized) status of these bodies, or could anyone form a group and
> claim to be a new repeater coordinating body? Also, what criteria are used by
> coordinating bodies to resolve disputes, and are these criteria consistent
> amoung different coordinating bodies? If someone gets a repeater to be
> coordinated do they get to keep their frequencies indefinitely, or can the
> coordinating body be persuaded to give it to someone else. (and again, what
> criteria would they use to decide.)
Hi Brian. By now you've taken that test. How did you do?
These coordinating bodies form. Their power basically is in acceptance
by the amateur community. The FCC's only sanction of them are some warm
words in Part 97. How disputes are resolved, and the rules about how
stations are coordinated, are up to these bodies.
In practice, it's a tough thankless job.
--
_[ Robb Topolski ][ San Clemente CA ][ topolski@kaiwan.com ][ 192.215.30.2 ]_
Mattel has come out with a new Barbie doll for Christmas: Divorcee' Barbie.
It comes with all the usual accessories, plus all of Ken's stuff.
------------------------------
Date: Sun, 12 Jun 1994 21:31:19 GMT
From: ihnp4.ucsd.edu!swrinde!howland.reston.ans.net!usenet.ins.cwru.edu!ncoast!fmsystm.telemax.com!fmsys!macy@network.ucsd.edu
Subject: <<Best dual band verticals?>>
To: info-hams@ucsd.edu
In article <2tdee3$lgo@brahms.udel.edu> penneys@brahms.udel.edu (Robert Penneys) writes:
>
>We are having some debate in the club about the best base station verticals
>for 2m/440.
We've used several types for the couple local clubs I'm involved with.
What always seems to work best is the Diamond X-500 or X-500RH.
Yes, they wave around a bit in the wind, but they work very well.
(We've tried others, but keep coming back to the Diamond X-500)
Diamonds will not withstand direct lightning strikes. Some commercial
antennas seem to do better with lightning, but offer lesser performance.
Since we can buy a X-500RH (heavy duty version) for around $220, we've
decided to bear with replacing them when they are destroyed by lightning.
Around here, thats about every two years for an tower mounted unit.
Note: for some reason we have not tried the similiar Comet. I hear
other clubs have, and like it. Also, its a good idea to seal up these
fiberglass antennas with silcone seal when you assemble them. Every
once in a while, a leak around a joint will develop, probably from
the flexing in the wind.
Regards,
--
Macy M. Hallock, Jr. N8OBG +1.216.723.3030 macy@telemax.com macy@fms.com
Telemax, Inc. - F M Systems, Inc. 152 Highland Drive Medina, OH 44256 USA
------------------------------
Date: 13 Jun 94 01:20:28 GMT
From: news-mail-gateway@ucsd.edu
Subject: ANS-162 BULLETINS
To: info-hams@ucsd.edu
SB SAT @ AMSAT $ANS-162.01
DOVE VOICE TESTING STATUS
HR AMSAT NEWS SERVICE BULLETIN 162.01 FROM AMSAT HQ
SILVER SPRING, MD JUNE 11, 1994
TO ALL RADIO AMATEURS BT
BID: $ANS-162.01
DOVE-OSCAR-17 (DOVE) Voice Synthesizer Testing Continues
At about 11-JUNE-94 05:30 UTC the DOVE Ground Command Team completed a
reload of the DOVE software and activated another voice test. The pro-
nunciation of the word "Hi" is a bit different and the overall amplitude of
the voice is higher. The text message is a greeting to those attending the
ARRL Convention and Education Forum.
The DOVE Ground Command Team expects to continue the hardware testing pro-
cess while simultaneously proceeding with software development. It is
expected that this effort will probably last several days to a few weeks
before all the testing and software developement is completed. There may
be times when the voice message will not be heard due to uploading of new
software.
It would be appreciate if reports on how well the voice can be heard with
simple receiving equipment (a H/T with a rubber duck antenna) could be sent
to any of the following individuals who have mail address on INTERNET:
WJ9F@amsat.org
PY2BJO@amsat.org
WD0E@amsat.org
VK7ZBX@amsat.org
N5AHD@amsat.org
Telemetry is not needed at this time.
[The AMSAT News Service would like to thank Jim White (WD0E) for this
bulletin item. ]
/EX
SB SAT @ AMSAT $ANS-162.02
IO-26 STATUS REPORT
HR AMSAT NEWS SERVICE BULLETIN 162.02 FROM AMSAT HQ
SILVER SPRING, MD JUNE 11, 1994
TO ALL RADIO AMATEURS BT
BID: $ANS-162.02
ITAMSAT-OSCAR-26 (IO-26) Status Report
After a couple of weeks of being in the stand-by mode, IO-26, under ground
command, was switched back ON. A new MBL code was successfully loaded to
test the modified s/c configuration (secondary TX on). Telemetry shows all
the vital parameters in nominal status. Further tests will be carried out
in the next days. Also due to the very limited time budget of the command
stations please expect a few weeks before normal operations.
[The AMSAT News Service (ANS) would like to thank Alberto Zagni (I2KBD)
for this bulletin item.]
/EX
SB SAT @ AMSAT $ANS-162.03
WEEKLY OSCAR STATUS REPORTS
HR AMSAT NEWS SERVICE BULLETIN 162.03 FROM AMSAT HQ
SILVER SPRING, MD JUNE 11, 1994
TO ALL RADIO AMATEURS BT
BID: $ANS-162.03
Weekly OSCAR Status Reports: 11-JUN-94
AO-13: Current Transponder Operating Schedule:
L QST *** AO-13 TRANSPONDER SCHEDULE *** 1994 May 07-Jul 11
Mode-B : MA 0 to MA 170 |
Mode-BS : MA 170 to MA 218 |
Mode-S : MA 218 to MA 220 |<- S beacon only
Mode-S : MA 220 to MA 230 |<- S transponder; B trsp. is OFF
Mode-BS : MA 230 to MA 250 | Alon/Alat 230/-5
Mode-B : MA 250 to MA 256 |
Omnis : MA 250 to MA 120 | Move to attitude 180/0, Jul 11
[G3RUH/DB2OS/VK5AGR]
LO-19: LO-19 is on the air but only telemetry is being sent and there are
are no BBS functions operational. [WH6I]
KO-23: This bird and KO-25 are very busy at the present time with message
and file traffic. There have been a lot of new earth imaging
files available for down loading on both birds. The file
KAIW008D gives a good image of the Italian penninsula in the Med.
There is also a steady stream of WISP files as ZL2TPO keeps the
his programing modifications coming. Also, the program WISP can
also be found on the BBS. [WH6I]
AO-16: AO-16 is running strong, the only 1200 baud bird in operation at the
present time. [WH6I]
IO-26: IO-26 is sending telemtry, but the BBS is not yet on. [WH6I]
The AMSAT NEWS Service (ANS) is looking for volunteers to contribute weekly
OSCAR status reports. If you have a favorite OSCAR which you work on a
regular basis and would like to contribute to this bulletin, please send
your observations to WD0HHU at his CompuServe address of 70524,2272, on
INTERNET at wd0hhu@amsat.org, or to his local packet BBS in the Denver, CO
area, WD0HHU @ W0LJF.#NECO.CO.USA.NOAM. Also, if you find that the current
set of orbital elements are not generating the correct AOS/LOS times at
your QTH, PLEASE INCLUDE THAT INFORMATION AS WELL. The information you
provide will be of value to all OSCAR enthusiasts.
/EX
------------------------------
Date: 13 Jun 94 04:19:33 GMT
From: news-mail-gateway@ucsd.edu
Subject: Any Ham in CASARA ?
To: info-hams@ucsd.edu
Greetings,
I would like to know if their are any ham operators who work for
CASARA (Civil Air Search And Rescue Association).
Guy VE3 XGQ
Co-Sysop of the Sudbury Amateur Radio BBS 1:224/50
guy@penage.cs.laurentian.ca
------------------------------
Date: 13 Jun 1994 00:15:05 GMT
From: ihnp4.ucsd.edu!swrinde!gatech!news-feed-1.peachnet.edu!hobbes.cc.uga.edu!aisun1.ai.uga.edu!mcovingt@network.ucsd.edu
Subject: Beware of RADIOKIT kits (IMHO)
To: info-hams@ucsd.edu
That is unfortunate. Radiokit has been around for quite a few years;
surely they wouldn't have lasted that long if that kind of performance
were the norm.
--
< Michael A. Covington, Assc Rsch Scientist, Artificial Intelligence Center >
< The University of Georgia, Athens, GA 30602-7415 USA mcovingt@ai.uga.edu >
< Unless specifically indicated, I am not speaking for the University. > <><
For information about any U.Ga. graduate program, email gradadm@uga.cc.uga.edu.
------------------------------
Date: 12 Jun 1994 19:16:06 -0700
From: nntp.crl.com!crl2.crl.com!not-for-mail@decwrl.dec.com
Subject: Beware of RADIOKIT kits (IMHO)
To: info-hams@ucsd.edu
In article <2tg8e9$1k5@hobbes.cc.uga.edu> mcovingt@aisun1.ai.uga.edu (Michael Covington) writes:
>That is unfortunate. Radiokit has been around for quite a few years;
>surely they wouldn't have lasted that long if that kind of performance
>were the norm.
Oh, I don't know, maybe they hired a MBA to run their quality control?
Jeff
--
Jeff Jones AB6MB | Remember nothing is impossible to
jeffj@crl.com | a sick mind!
------------------------------
Date: Sat, 11 Jun 1994 21:51:43 MDT
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 11 June
To: info-hams@ucsd.edu
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY
11 JUNE, 1994
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
(Based In-Part On SESC Observational Data)
SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 11 JUNE, 1994
--------------------------------------------------------
NOTE: Electron fluence at greater than 2 MeV is at moderate levels.
!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 162, 06/11/94
10.7 FLUX=086.4 90-AVG=081 SSN=080 BKI=3334 3323 BAI=015
BGND-XRAY=A7.3 FLU1=2.9E+05 FLU10=1.2E+04 PKI=3345 3223 PAI=020
BOU-DEV=026,031,023,040,029,021,015,022 DEV-AVG=025 NT SWF=00:000
XRAY-MAX= B1.8 @ 1735UT XRAY-MIN= A6.7 @ 0822UT XRAY-AVG= A8.7
NEUTN-MAX= +002% @ 2205UT NEUTN-MIN= -002% @ 1825UT NEUTN-AVG= +0.5%
PCA-MAX= +0.2DB @ 1920UT PCA-MIN= -0.3DB @ 2100UT PCA-AVG= +0.0DB
BOUTF-MAX=55327NT @ 0208UT BOUTF-MIN=55298NT @ 0929UT BOUTF-AVG=55310NT
GOES7-MAX=P:+000NT@ 0000UT GOES7-MIN=N:+000NT@ 0000UT G7-AVG=+080,+000,+000
GOES6-MAX=P:+149NT@ 1939UT GOES6-MIN=N:-089NT@ 0913UT G6-AVG=+108,+030,-029
FLUXFCST=STD:086,086,086;SESC:086,086,086 BAI/PAI-FCST=018,015,010/018,015,010
KFCST=3344 3333 3234 3332 27DAY-AP=030,030 27DAY-KP=3356 4334 4454 6433
WARNINGS=
ALERTS=**245STRM:1136-1526UTC(MOD-INTENSITY)
!!END-DATA!!
NOTE: The Effective Sunspot Number for 10 JUN 94 was 39.0.
The Full Kp Indices for 10 JUN 94 are: 2o 3- 3- 5o 3- 4- 3- 3o
The 3-Hr Ap Indices for 10 JUN 94 are: 8 14 11 46 14 21 13 15
Greater than 2 MeV Electron Fluence for 10 JUN is: 2.5E+08
SYNOPSIS OF ACTIVITY
--------------------
Solar activity continued at a very low level. Slow decay
was observed in most regions and the east limb is quiet as seen
in Yohkoh soft x-ray imagery. A small region emerged near
N13E04 and was numbered as new Region 7734.
Solar activity forecast: solar activity should continue
at a very low level. An isolated C-class flare is a slight
possibility.
The geomagnetic field was mostly unsettled. The period
between approximately 0900-1200Z was at active to minor
storm levels with some high latitude sites reporting major
storming during that interval. Energetic electron fluxes
at geosynchronous altitude were at mostly moderate levels.
Geophysical activity forecast: the geomagnetic field
should be unsettled to slightly active. The most disturbed
periods should occur near local nighttime. Isolated storm
conditions are expected at high latitudes.
Event probabilities 12 jun-14 jun
Class M 01/01/01
Class X 01/01/01
Proton 01/01/01
PCAF Green
Geomagnetic activity probabilities 12 jun-14 jun
A. Middle Latitudes
Active 35/30/25
Minor Storm 20/15/10
Major-Severe Storm 10/05/01
B. High Latitudes
Active 40/35/30
Minor Storm 20/20/15
Major-Severe Storm 15/15/05
HF propagation conditions were near-normal over all
regions. No significant degradation was reported. The
strength of the anticipated coronal-hole disturbance has thus
far been weaker than expected. Conditions should remain
near-normal over all regions throughout the next 72 hours.
Sporadic minor signal degradation can be expected on
transauroral night-crossing circuits.
COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS
========================================================
REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 11/2400Z JUNE
-------------------------------------------------------
NMBR LOCATION LO AREA Z LL NN MAG TYPE
7730 S10E22 128 0080 DAO 05 009 BETA
7731 N08E27 123 0090 DAO 03 003 BETA
7732 S09W67 217 0030 BXO 06 005 BETA
7733 N05W21 171 0030 BXO 06 008 BETA
7734 N13E03 147 0020 CRO 04 005 BETA
REGIONS DUE TO RETURN 12 JUNE TO 14 JUNE
NMBR LAT LO
NONE
LISTING OF SOLAR ENERGETIC EVENTS FOR 11 JUNE, 1994
---------------------------------------------------
BEGIN MAX END RGN LOC XRAY OP 245MHZ 10CM SWEEP SWF
NO EVENTS OBSERVED
POSSIBLE CORONAL MASS EJECTION EVENTS FOR 11 JUNE, 1994
-------------------------------------------------------
NO EVENTS OBSERVED
INFERRED CORONAL HOLES: LOCATIONS VALID AT 11/2400Z
---------------------------------------------------
ISOLATED HOLES AND POLAR EXTENSIONS
EAST SOUTH WEST NORTH CAR TYPE POL AREA OBSN
85 S17W05 S25W54 S20W64 N28W32 189 ISO POS 024 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
------ ---- ---- ---- ---- -- ------ ------ --------- --------- ---------
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 **
------------------------------
Date: Sun, 12 Jun 1994 21:22:37 GMT
From: ihnp4.ucsd.edu!swrinde!howland.reston.ans.net!usenet.ins.cwru.edu!ncoast!fmsystm.telemax.com!fmsys!macy@network.ucsd.edu
Subject: HTX 202
To: info-hams@ucsd.edu
In article <441@bjohns.win.net> bret@bjohns.win.net (Bret A. Johnson) writes:
>I am looking for opions on the Radio Shack HTX 202 HT.
Pros:
Fairly easy to use.
Good intermod performance, well suited to urban/suburban areas.
Good sensitivity.
Uses easy to obtain accessories (same as a popular older ICOM model)
Inexpensive, RS was selling them for $188, I've seen them for $150
at hamfests recently. May be the best buy in a handheld today.
Durable. Not a fragile unit.
Radio Shack will sell extended warranty, if you wish.
(I prefer to use my Gold Mastercard's extended warranty program, BTW)
Well liked for packet operation in non-fringe areas.
Cons:
RS name is disliked by some (but unit _is_ well constructed)
Does not have advanced features some prefer.
Cannot operate out of band as other units can.
Larger and heavier than many current models by others.
Not a large number of memories.
In summary, a nice basic or entry level hand held 2m unit.
If you want small, highly featured or prestige, look elsewhere.
For basic, durable and straightforward, these are hard to beat.
I'm looking for one of these used for my son to use at Ohio State
this fall, for all the reasons above. I hesitated and missed one
for $150 w/spkrmike at the hamfest today. (Seems as though these
always sell quickly at hamfests, when priced below $188)
Regards,
--
Macy M. Hallock, Jr. N8OBG +1.216.723.3030 macy@telemax.com macy@fms.com
Telemax, Inc. - F M Systems, Inc. 152 Highland Drive Medina, OH 44256 USA
------------------------------
Date: Sun, 12 Jun 94 23:18:40 -0500
From: news.delphi.com!usenet@uunet.uu.net
Subject: HTX 202
To: info-hams@ucsd.edu
Macy Hallock <macy@telemax.com> writes:
>Cannot operate out of band as other units can.
Is there an extended recieve code anywhere out there for this radio?
also, I'm sort of new to both HAM and internet, in the first message, there
was a series of codes, what in the world was that?
I'd appreciate any assistance, advice, or suggestions relating to this radio.
Thanks,
Larry Good, N2WNO
------------------------------
Date: Sun, 12 Jun 1994 23:25:12 GMT
From: ihnp4.ucsd.edu!swrinde!pipex!sunic!trane.uninett.no!nac.no!nntp.uio.no!ifi.uio.no!wabbit.cc.uow.edu.au!metro!ipso!rwc@network.ucsd.edu
Subject: IPS Daily Report - 12 June 94
To: info-hams@ucsd.edu
SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 12/2330Z JUNE 1994 BY IPS RADIO AND SPACE SERVICES
FROM THE REGIONAL WARNING CENTRE (RWC), SYDNEY.
SUMMARY FOR 12 JUNE AND FORECAST UP TO 15 JUNE
IPS Warning 16 was issued on 08 June and is current
for interval June 11-13.
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity: very low
Flares: none.
Observed 10.7 cm flux/Equivalent Sunspot Number : 086/029
1B. SOLAR FORECAST
13 June 14 June 15 June
Activity Low Very low Very low
Fadeouts None expected None expected None expected
Forecast 10.7 cm flux/Equivalent Sunspot Number : 086/029
1C. SOLAR COMMENT
A solar filament near the centre of the solar disk has dissappeared.
-----------------------------------------------------------
2A. MAGNETIC SUMMARY
Geomagnetic field at Learmonth: unsettled to active
Estimated Indices : A K Observed A Index 11 June
Learmonth 21 3344 4433
Fredericksburg 21 15
Planetary 22 16
Observed Kp for 11 June: 3345 3223
2B. MAGNETIC FORECAST
DATE Ap CONDITIONS
13 Jun 20 Active.
14 Jun 16 Unsettled.
15 Jun 16 Unsettled to active.
2C. MAGNETIC COMMENT
Active levels expected June 13 due to coronal hole. Active periods
may be observed during June 16-17 due to dissappearing solar
filament.
3A. GLOBAL HF PROPAGATION SUMMARY
LATITUDE BAND
DATE LOW MIDDLE HIGH
12 Jun normal fair fair
PCA Event : None.
3B. GLOBAL HF PROPAGATION FORECAST
LATITUDE BAND
DATE LOW MIDDLE HIGH
13 Jun normal fair poor
14 Jun normal fair poor
15 Jun normal fair poor
3C. GLOBAL HF PROPAGATION COMMENT
Degraded HF comms conditions expected today for mid and high lats.
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
MUFs at Sydney were about 15% above predicted monthly values
Observed T index for 12 June: 53
Predicted Monthly T Index for June is 30.
4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
DATE T-index MUFs
13 Jun 40 About 10% above predicted monthly values.
14 Jun 40 About 10% above predicted monthly values.
15 Jun 40 About 10% above predicted monthly values.
4C. AUSTRALIAN REGION COMMENT
Degraded HF comms possible today.
--
IPS Regional Warning Centre, Sydney |IPS Radio and Space Services
email: rwc@ips.oz.au fax: +61 2 4148331 |PO Box 5606
RWC Duty Forecaster tel: +61 2 4148329 |West Chatswood NSW 2057
Recorded Message tel: +61 2 4148330 |AUSTRALIA
------------------------------
Date: 12 Jun 1994 21:47:52 -0700
From: ihnp4.ucsd.edu!library.ucla.edu!csulb.edu!paris.ics.uci.edu!news.claremont.edu!kaiwan.com!not-for-mail@network.ucsd.edu
To: info-hams@ucsd.edu
References <199406071807.LAA19308@ucsd.edu>, <rogjdCr2voM.4IA@netcom.com>, <CSLE87-090694095911@145.39.1.10>
Subject : Re: 440 in So. Cal.
Karl Beckman (CSLE87@email.mot.com) wrote:
> Roger, from your callsign I can see that you hold a high enough class of
> license to know that you can either personally fill some of that
> underutilized spectrum with your own repeater, or join one of the smaller
> special interest groups that utilize 440 for their amateur radio
> activities. Open repeaters weren't the issue, access to spectrum was and
> continues to be the problem.
Karl,
The Subject: line of this message is still 440 in Southern California.
This is not Texas or Ohio.
If Roger wanted to put up a 440 repeater in Southern California, all
indications are this widely popular service would be co-channeled with
other open repeaters on about a half-dozen frequencies. I don't have my
repeater guide with me, but I think six is pretty close to the actual
number of pairs -- out of all the 440 band -- where open repeaters are
coordinated.
Every other pair has a single or multiple closed-channel repeaters on
them -- if the repeaters exist at all (and many don't).
Now the "Scrubba" dudes can't be all bad -- this took some thought to
accomplish. I don't think when this bandplan was formulated that they
figured that in the 1990's, 440 was going to be a popular band.
Times changed. The method has become their madness. We need to triple
the available "open" pairs and create a few for extremely high-level
wide-area signalling, a few for regional use, and a few for community use
on a shared CTCSS-controlled inputs. And that would leave plenty of room
for the private repeaters.
Coordination has to be more assertive. First come, first served may work
great at the bakery. But in a city with borders, planning and
negotiating go hand-in-hand. So XYZARC can't put their private repeater
on Mount Horizon at 500 watts Omni, they'll have to decide between Lookout
Hill at 50 watts or Polaroid Point at 100 watts with a Southern
directional. Sorry fellas. What's that? You want Lookout Hill at 150
watts Omni? Well lets make it 100 watts and you can increase to 150
watts during your weekly net and during emergencies. Fair enough? Deal!
See? Easy!
73
--
_[ Robb Topolski ][ San Clemente CA ][ topolski@kaiwan.com ][ 192.215.30.2 ]_
Mattel has come out with a new Barbie doll for Christmas: Divorcee' Barbie.
It comes with all the usual accessories, plus all of Ken's stuff.
------------------------------
End of Info-Hams Digest V94 #656
******************************