Date: Tue, 15 Feb 94 00:40:32 PST
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 #153
To: Info-Hams
Info-Hams Digest Tue, 15 Feb 94 Volume 94 : Issue 153
Today's Topics:
(none)
440 MHz in Orlando - Open Repeaters??
Butternut HF6V upgrade kit ???
callsign server info
CELLULAR SURVEILLANCE
Copying High-Speed CW: Print or Script?
Daily Summary of Solar Geophysical Activity for 09 February
FCC.GOV on-line
FCC Daily Digests for the
Nude amateur radio clubs
QSL route for RW0LZ, please?
RTTY DX NOTES 11 FEB
which is better qrp band--30 or 40?
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: 15 Feb 94 06:29:27 GMT
From: news-mail-gateway@ucsd.edu
Subject: (none)
To: info-hams@ucsd.edu
subscribe
------------------------------
Date: 13 Feb 1994 07:40:42 GMT
From: agate!howland.reston.ans.net!wupost!udel!pacs.sunbelt.net!lynx.unm.edu!netsun!edberg@ames.arpa
Subject: 440 MHz in Orlando - Open Repeaters??
To: info-hams@ucsd.edu
Hello,
I happen to be in Orlando, Florida on business (ignore signature) and I
didn't bring my repeater directory. Are there any open repeaters here,
and if so, what freqs? Either reply here or call my hotel 407-351-1000.
Thanks and 73s.
don N6CLP
--
*****************************************************************
* e-mail: edberg@netsun.mdc.com * Don Edberg *
* CI$:72417.2067@compuserve.com * Advanced Programs & Technology*
* phone: 1-714-896-5210 * McDonnell-Douglas Aerospace *
* FAX: 1-714-896-6930 * 5301 Bolsa Ave, MS 13-3 *
* Call: N6CLP * Huntington Bch, CA 92647-2099 *
*****************************************************************
------------------------------
Date: 11 Feb 1994 18:20:03 GMT
From: mvb.saic.com!unogate!news.service.uci.edu!usc!sdd.hp.com!sgiblab!cs.uoregon.edu!news.uoregon.edu!fp2-st-affairs-11.uoregon.edu!user@network.ucsd.edu
Subject: Butternut HF6V upgrade kit ???
To: info-hams@ucsd.edu
Now that I finally have a radio that covers the WARC bands, I'm thinking of
getting the add on kit for 12 & 17 meters for my Butternut vertical.
Does anyone have any experience with this upgrade?
I'm specifically interested in whether the bandwidth is narrowed on the
other bands once this kit is installed.
For example, Butternut has said that the 160 meter add on kit will narrow
the bandwidth on 80 meters. Will this one affect the others to any great
extent?
BTW, the Butternut is the best performing vertical I've owned. I'd love to
see what I could get out of it if I got it up in the air. Right now it's
ground mounted with 17 radials, most of which are cut for the higher bands.
Since Dec. 1989, have worked 275 countries overall with it (about 268 of
them running barefoot). Also have worked 150+ countries on 40 meters with
it, at least 110 of those running barefoot.
Performance barefoot is dropping off considerably with the solar cycle the
way it is these days, but for a vertical, I'm still very happy with it.
Steve
------------------------------
Date: 15 Feb 1994 00:13:14 GMT
From: agate!howland.reston.ans.net!wupost!udel!news.sprintlink.net!news.clark.net!andy@network.ucsd.edu
Subject: callsign server info
To: info-hams@ucsd.edu
Jerry Sy (ah301@yfn.ysu.edu) wrote:
: which port do I telnet to get to callsign server on
: cs.buffalo.edu ?
It is port 2000. Therefore, your command is: open cs.buffalo.edu 2000
-k4adl
------------------------------
Date: 15 Feb 94 03:02:50 GMT
From: news-mail-gateway@ucsd.edu
Subject: CELLULAR SURVEILLANCE
To: info-hams@ucsd.edu
94-02-14
Finally, as the result of the efforts of a number of Internet gurus,
we're able to tell you how to download a demo copy of the software
that controls our Cellular Surveillance Interface, via e-mail. The
program is entitled CELLDEMO.ZIP
Send an e-mail message to: ftpmail@decwrl.dec.com
Leave the subject line blank or use the word: file
In the body of the e-mail message, type the following six lines starting
at line 1. Put YOUR e-mail address where is says your-email-address:
reply your-email-address
connect ftp.funet.fi
binary
uuencode
get pub/dx/software/msdos/rx-control/celldemo.zip
quit
Except for your e-mail address, type it EXACTLY the way it reads above.
If you make any spelling or spacing mastakes, it won't work. Send it or
mail it when you're sure it's correct.
Some time later you'll get a few pieces of e-mail. Two of these will
each contain a portion of the demo program. The others are information
only. Now you need to do some additional work. Edit the first of the
two files you received to remove everything before the line that reads:
begin 444 ftpmail
This should now be line 1 of the file. Save the file.
The 444 refers to the number of lines in the two files, and ftpmail is
the file name that you'll end up with when you combine them.
Edit the second file to remove everything before the line that begins
with uppercase garbled text (similar to the text starting on line 2 of
the first file). Save this file also.
Now you need a program called UUDECODE. If you don't have it, download
and run the program UUE.EXE (or something similar) from a BBS in your
area.
Now type: UUDECODE name-of-the-FIRST-file you received-and-edited
You'll now have a new file named FTPMAIL that is the sum of the two
separate files your received and edited.
Rename this new file: celldemo.zip
Remember, celldemo.zip was the file you originally asked FTP to send
you.
Now you need a program called PKUNZIP. If you don't have it, download
and run the program PKZ204G.EXE from a BBS in your area.
Now type: PKUNZIP celldemo.zip
You'll now have four new files. Read the READ.ME file and then run the
CSIDEMO program.
We realize that this was a lot of work. However, it didn't cost you
anything except some time, and you now have a demo of the CSI unit. In
addition, if this worked for you, you now know how to FTP any program,
from anywhere, via e-mail. All you need to know is the FTP site, and
the directory and name of the program you want. You may wish to save
this FTP tutorial for future use.
Regards,
Bill Fischer Internet: bill.fischer@T8000.cuc.ab.ca
---
SLMR 2.0
------------------------------
Date: Mon, 14 Feb 1994 12:58:38 -0500
From: agate!howland.reston.ans.net!usenet.ins.cwru.edu!neoucom.edu!news.ysu.edu!psuvm!cunyvm!rohvm1!rohvm1.mah48d@network.ucsd.edu
Subject: Copying High-Speed CW: Print or Script?
To: info-hams@ucsd.edu
In article <13690@tekig7.PEN.TEK.COM>, gaulandm@tekig7.PEN.TEK.COM (Mike
Gauland) wrote:
> A mailing I read is involved in a comparision of the speeds of
> printing and cursive writing. I decided to consult some experts.
> So, all you high-speed CW ops, which do _you_ use?
>
I have used, for years, upper/lower-case printing for anything that takes
putting text onto paper by hand. Never could write cursive! But what
comes out tends to have characteristics of cursive writing without the
connecting lines.
As a result, I can write lower-case print-style characters without thinking
about them, so that's what I use copying code. I think the real key _is_
using something you don't have to think about, because stopping to think
about any aspect of your copy slows you down. (Again why I can't copy on a
typewriter/computer.)
Even when, at slower speeds, I'm writing block capitals for legibility (few
can read what I've written in the lower-case printing), I use the
lower-case "e" because the block "e" just takes too long.
Would have replied sooner, but got snowed out of the computer!!
__
73 de John Taylor W3ZID
rohvm1.mah48d@rohmhaas.com
------------------------------
Date: Thu, 10 Feb 1994 18:34:50 MST
From: mvb.saic.com!unogate!news.service.uci.edu!usc!elroy.jpl.nasa.gov!swrinde!cs.utexas.edu!math.ohio-state.edu!sol.ctr.columbia.edu!destroyer!nntp.cs.ubc.ca!alberta!ve6mgs!usenet@network.UCSD
Subject: Daily Summary of Solar Geophysical Activity for 09 February
To: info-hams@ucsd.edu
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
DAILY SUMMARY OF SOLAR GEOPHYSICAL ACT
09 FEBRUARY, 1994
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
(Based In-Part On SESC Observational Data)
SOLAR AND GEOPHYSICAL ACT
------------------------------------------------------------
!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 040, 02/09/94
10.7 FLUX=101 90-AVG=106 SSN=064 BKI=4544 4554 BAI=034
BGND-XRAY=B2.1 FLU1=0.0E+00 FLU10=0.0E+00 PKI=4445 4455 PAI=034
BOU-DEV=060,095,068,074,031,044,033,048 DEV-AVG=056 NT SWF=00:000
XRAY-MAX= C3.0 @ 1822UT XRAY-MIN= B1.6 @ 0312UT XRAY-AVG= B3.7
NEUTN-MAX= +002% @ 2155UT NEUTN-MIN= -003% @ 0955UT NEUTN-AVG= +0.1%
PCA-MAX= +0.1DB @ 2115UT PCA-MIN= -0.3DB @ 0405UT PCA-AVG= +0.0DB
BOUTF-MAX=55360NT @ 0300UT BOUTF-MIN=55305NT @ 1806UT BOUTF-AVG=55336NT
GOES7-MAX=P:+000NT@ 0000UT GOES7-MIN=N:+000NT@ 0000UT G7-AVG=+065,+000,+000
GOES6-MAX=P:+124NT@ 2004UT GOES6-MIN=N:-068NT@ 0423UT G6-AVG=+086,+035,-031
FLUXFCST=STD:103,104,109;SESC:103,104,109 BAI/PAI-FCST=025,020,015/025,025,020
KFCST=3355 4333 3355 4333 27DAY-AP=021,019 27DAY-KP=4433 5334 3344 4333
WARNINGS=*GSTRM;*AURMIDWCH
ALERTS=**MAJSTRM
!!END-DATA!!
NOTE: The Effective Sunspot Number for 08 FEB 94 was 25.0.
The Full Kp Indices for 08 FEB 94 are: 6- 5o 6- 6o 6o 4+ 5- 5-
The 3-Hr Ap Indices for 08 FEB 94 are: 63 48 67 87 87 35 36 41
SYNOPSIS OF ACT
--------------------
Solar activity was low. Region 7668 (N08E35) was
the most active this period producing several optical flares
with B-class enhancements while showing good white light growth.
Rgn 7664 (S12W75) produced the only C-class flare this period
which maxed at 1822. This rgn is also showing growth as it
approaches the west limb. All other regions are stable.
Solar activity forecast: solar activity is expected to be
low with Regions 7664 and 7668 showing the most promise for
C-class activity. Old Region 7654 (N09, carrington 207) is due
to return late on the 11Th. During its last rotation, it
produced 4 M-class and 27 C-class flares.
At middle latitudes, the geomagnetic field has been at
active to minor storm levels while at high latitudes, the field
has been at mostly active to major storm levels with isolated
severe storm conditions reported. A favorably positioned
coronal hole is believed to be responsible for the storm
conditions.
Geophysical activity forecast: the geomagnetic field
should remain at mostly active levels for the duration of
the forecast period. Occasional periods of minor to major
storms are still likely. Disturbed geomagnetic conditions
should be expected for the next six days.
STD: High energy electrons at greater than 2 MeV continue to
be observed. Satellite charging anomalies are possible and
will remain possible for as long as this enhancement continues.
Event probabilities 10 feb-12 feb
Class M 10/15/20
Class X 01/01/01
Proton 01/01/01
PCAF Green
Geomagnetic activity probabilities 10 feb-12 feb
A. Middle Latitudes
Active 50/45/20
Minor Storm 15/15/10
Major-Severe Storm 15/10/05
B. High Latitudes
Active 50/50/55
Minor Storm 15/15/10
Major-Severe Storm 10/10/10
HF propagation conditions are disturbed over all regions.
Although transpolar and transauroral circuits have been hit the
hardest, degradations have been noticed through to the
equatorial regions. MUFs are well below normal, depressed by
between 20 and 50 percent. LUFs are also elevated, narrowing
the available bandwidth. Periods of total radio blackouts are
continuing to be observed for transauroral and transpolar
circuits. Although conditions are expected to very gradually
improve over the next week, nothing substantial is expected.
COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS
========================================================
REGIONS WIT
-----------------------------------------------------------
NMBR LOCATION LO AREA Z LL NN MAG TYPE
7664 S12W75 035 0180 EAO 11 009 BET
7665 N03W69 029 0000 AXX 01 001 ALPHA
7666 N18W28 348 0110 CAO 04 004 BET
7668 N08E35 285 0240 DAO 09 010 BET
7667 S07W15 335 PLAGE
REGIONS DUE TO RET
NMBR LAT
7652 N04 221
7654 N09 207
LISTING OF SOLAR ENERGETIC EVENTS FOR 09 FEBRUARY, 1994
-------------------------------------------------------
BEGIN MAX END RGN LOC XRAY OP 245MHZ 10CM SWEEP
NONE
POSSIBLE CORONAL MASS EJECTION EVENTS FOR 09 FEBRUARY, 1994
-----------------------------------------------------------
BEGIN MAX END LOCATION TYPE SIZE DUR II IV
NO EVENTS OBSERVED
INFERRED CORONAL HOLES. LOCATIONS VALID AT 09/2400Z
---------------------------------------------------
ISOLATED HOLES AND POLAR EXT
EAST SOUTH WEST NORTH CAR TYPE POL AREA OBSN
NO DAT
SUMMARY OF FLARE EVENTS FOR THE PREVIOUS UTC DAY
------------------------------------------------
Date Begin Max End Xray Op Region Locn 2695 MHz 8800 MHz 15.4 GHz
------ ---- ---- ---- ---- -- ------ ------ --------- --------- ---------
08 Feb: 0746 0817 0837 1F 7668 N07E60
0957 0959 1007 SF 7668 N07E59
1305 1312 1328 SF 7668 N08E55
1605 1613 1619 B7.3 SF 7668 N08E54
1750 1753 1833 SF 7668 N08E53
1917 1921 1932 SF 7668 N08E52
2323 2327 2331 B4.7
REGION FLARE STATISTICS FOR THE PREVIOUS UTC DAY
------------------------------------------------
C M X S 1 2 3 4 Total (%)
-- -- -- -- -- -- -- -- --- ------
Region 7668: 0 0 0 5 1 0 0 0 006 (85.7)
Uncorrellated: 0 0 0 0 0 0 0 0 001 (14.3)
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 **
------------------------------
Date: Sun, 13 Feb 1994 08:13:04 GMT
From: agate!howland.reston.ans.net!vixen.cso.uiuc.edu!sdd.hp.com!portal!unix.portal.com!twise@ames.arpa
Subject: FCC.GOV on-line
To: info-hams@ucsd.edu
What will FCC.GOV give us access to?
Travis A. Wise Del Mar High School email: twise@shell.portal.com
1421 Grace Avenue Home: 408/267-9562 AX.25: KB8FOU@N6LDL.CA.USA.NA
San Jose, CA 95125 Fax: 408/267-6981 FTP: portal.com /pub/twise
------------------------------
Date: 14 Feb 94 13:01:51 GMT
From: psinntp!psinntp!wlnntp.psi.com!usenet@rutgers.rutgers.edu
Subject: FCC Daily Digests for the
To: info-hams@ucsd.edu
>DATE: 13 Feb 94 14:21:00 GMT
>FROM: Steve Allen <steve.allen@brent.uucp>
>
>bruce@pixar.com (Bruce Perens) writes, and writes, and writes:
>[ cable-tv, broadcast FM, commercial microwave, satellite pager
>drivel omitted...
>]
>
>Bruce: besides being 99.9% irrelevant to amateur radio, this is an
>incredible waste of bandwidth. If you feel a need to post this
>stuff, form your own newsgroup.
>-Steve N2WSA
>---
While I agree it is "99.9% irrelevant to amateur radio" it is "THE"
most interesting thread on this group.
- Tom -
=========================================================================
Thomas J. Alessi - WB1L | INTERNET: TJA@Panix.Com
P.O. Box 16781, Stamford CT. 06905 | AmprNet: 44.88.6.35
203-969-1880(H) 203-977-5200(W) | ax.25: WB1L@KC2FD.#nli.ny.us
=========================================================================
------------------------------
Date: Mon, 14 Feb 1994 23:49:52 GMT
From: agate!howland.reston.ans.net!darwin.sura.net!news.duc.auburn.edu!eng.auburn.edu!weltyrc@network.ucsd.edu
Subject: Nude amateur radio clubs
To: info-hams@ucsd.edu
I trust they don't work much SSTV !?
kd4vzx
------------------------------
Date: 13 Feb 1994 13:07:00 -0800
From: ucsnews!sol.ctr.columbia.edu!howland.reston.ans.net!agate!apple.com!apple.com!not-for-mail@network.ucsd.edu
Subject: QSL route for RW0LZ, please?
To: info-hams@ucsd.edu
Can anyone help me with the QSL route for RW0LZ? (R-W-zero-L-Z)
(Not in 1994 Callbook.)
Thanks and 73,
Kok Chen, AA6TY kchen@apple.com
Apple Computer, Inc.
------------------------------
Date: 10 Feb 94 15:41:13 CST
From: tulane!agwbbs!Angelo_Glorioso_Iii@ames.arpa
Subject: RTTY DX NOTES 11 FEB
To: info-hams@ucsd.edu
RTTY DX NOTES 11 FEB 93
RTTY DX NOTES W/E 11 FEB 94
VK2SG RTTY DX NOTES FOR WEEK ENDING 11 FEB 93 (BID RTDX0211)
OUR INFORMATION THIS WEEK CAME FROM 9X5LJ, I5AAX AND THE IK5PWJ
PACKET CLUSTER, I5FLN, WB2CJL, AA5AU, W5KSI, ZS5S, AND THE NJ0M NODE
OF THE TWIN CITIES DX PACKETCLUSTER NETWORK. THANKS TO ALL FOR
YOUR HELP.
BANDPASS:
FRIDAY 4
0735-14084 FK8GS REV.
0939-14082 YL1ZE
1142-21083 UN8PFE
1302-14085 4S7RM
1320-14089 SO6AD/9
1340-14091 HK0DPA
1348-14088 9H1ET
1500-21085 TZ6FIC
1510-21089 XE1SRF
2350-14089 JA3DLE/1
SATURDAY 5
0245-14086 VQ9TV
0835-14082 6W6JX
1257-14087 YV5KAJ
1304-21085 TZ6FIC
1316-21082 TU4EV
1400-21088 ZD7DP
1435-21085 CU3EM
1525-14086 J88BS
1543-14081 4U1ITU
1707-14083 XU7VK
1817-14082 J28JJ
1918-14086 EA8AK
1922-14088 ZA1MH
2008-14092 FG5FI
2149-14085 FM5GN
2156-14087 LU4DXU
SUNDAY 6
0006-14085 S92ZM
0042-21076 3Y0PI FEC QSL KA6V SEE NOTE
0103-21076 3Y0PI ARQ
0620-14079 UA0ST
0624-14086 TR8MD QSL F6FNU
0648-14082 S53X
0756-14079 4U1ITU
0756 14079 4X/OK1FGV
0800-14080 T91ENS PACTOR
0826-14090 ER1PE
0830-14071 OD5ZZ PACTOR
0921-21086 EA6VS
0926-14083 UX0KC
0930-14085 6W6JX
0950-14090 UY7LT
0951-14090 RW8LZ
1035-14086 RV9CX
1050-14086 XU7VK QSL HA0HW
1053-14085 UN5PR
1053-14085 UH8WAD
1340-21085 ZS5J
1343-21083 SV9CAG
1400-14085 BV7WB
1400-21086 ZD7DP
1403-14087 4U1ITU
1405-14085 XU7VK
1415-14088 CU3EM
1431-14089 HP1XVI
1440-14091 YB3AQF
1441-28083 V50CM
1454-14086 TA5C
1506-21076 TU2BB PACTOR
1509-14091 UT2UZ
1533-14087 5B4VX
1538-21083 V50CM
1532-14080 VU2YK PACTOR
1705-14083 XU7VK
2226-14087 FM5GN
2322-14087 HP1XVI
MONDAY 7
1107-14085 XU7VK
1711-14089 CO2AW
1829-14083 C91AI QSL CT1DGZ
1900-14084 3Y0PI INVERTED
2007-14083 CX3ABE
2021-21085 ZD7SM
2148-14084 CO2AW
2206-14084 YN4JAR
2224-14084 HK0DPA
2239-14084 S92ZM
2340-14084 ZP6EM
2354-14086 KP4SQ
TUESDAY 8
0002-14088 PJ2MI
0026-14083 VP8CIL
0030-14083 FY5FG
0032-14085 ZP6EM
0039-14080 3Y0PI QSX UP
0119-14076 3Y0PI
0302-14081 3Y0PI
0048-14082 CE3NDN PACTOR
1721-14090 HK0DPA
1822-14086 CO2AW
1857-14083 CX3ABE
1904-14085 5Z4FO
1930-14083 YN5JAR
2153-14070 V31AR FEC/ARQ
2218-14084 9Y4VU
2230-14082 CO2AW
2235-14080 3Y0PI PACTOR QRM
2300-14082 3Y0PI QSY'D TO ESCAPE PACTOR QRM
WEDNESDAY 9
0102-14082 3Y0PI STILL GOING STRONG
THURSDAY 10
0100-14081 V31JU
NOTES OF INTEREST:
TNX TO TONY WA4JQS, AT 3Y0PI, FOR HIS VALIANT EFFORTS IN
SUCCESSFULLY REPAIRING THE RTTY GEAR UNDER THE MOST ADVERSE
CONDITIONS.
A35JJ, TONGA - LOOK FOR A35JJ BETWEEN 12 AND 20 FEBRUARY
ON ALL BANDS. QSL TO JR2KDN.
FOR NEXT WEEK'S BULLETIN, SEND YOUR BANDPASS AND
NOTES OF INTEREST TO LUCIANO, I5FLN AT ZS5S.ZAF.AF OR
AT 9X5LJ.#KGL.RWA.AF.
73 ES GOOD HUNTING DE JULES W2JGR AT W2TKU.#SRQFL.FL.USA.NA
/EX
-- Via DLG Pro v1.0
Internet:angelo_glorioso_III@agwbbs.new-orleans.LA.US
Usenet:rex!agwbbs!angelo_glorioso_III
Packet:N5UXT @ N5UXT.#NOLA.LA.USA.NA
Tcp/ip:N5UXT.AMPR.ORG [44.108.2.13]
------------------------------
Date: 11 Feb 1994 17:21:49 GMT
From: mustang.mst6.lanl.gov!nntp-server.caltech.edu!news.claremont.edu!paris.ics.uci.edu!csulb.edu!library.ucla.edu!europa.eng.gtefsd.com!howland.reston.ans.net!vixen.cso.uiuc.edu@nntp.ucsb.edu
Subject: which is better qrp band--30 or 40?
To: info-hams@ucsd.edu
In article <slayCKx9CH.CFp@netcom.com> slay@netcom.com (Sandy Lynch) writes:
>mtrail@violet.berkeley.edu wrote:
>: The title says it all. Which band do you qrp'ers
>: prefer?
>
>For questions on QRP - I suggest a good source of info is the QRP reflector.
>To subscribe to the mailing list, simply send an e-mail msg to:
>
>qrp-request@think.com
>
>I can't recall if you should only enter SUBSCRIBE or also include info
>on yourself (e.g. name, call, qrp rig, etc).
>Cheers de Sandy WA6BXH/7J1ABV
>
The QRP mailing list has changed in the way that it is administered.
Please read the following that was posted to QRP this week:
Subject: QRP List now under Majordomo
All administrative requests should now be sent to "Majordomo@Think.COM";
mail sent to the QRP-Request address will cause an automatic reply from
Majordomo telling you what you should do.
If you want to unsubscribe from this list, send a message to the majordomo
address above containing only the line:
unsubscribe qrp
If you want to get the QRP-Digest list (still considered highly
experimental!) instead of the QRP list, send a message containing these two
commands:
unsubscribe qrp
subscribe qrp-digest
More info on things you can do with/to majordomo can be had by sending the
command:
help
Eventually, I will move the files which are in the QRP anonymous FTP area
into an area where they can be automaticaly retrieved by majordomo; as yet,
you'll find nothing with "index qrp".
If you still have questions or comments that require a human, send to
QRP-Admin@Think.COM, and someone will (eventually) get back to you.
73,
--Bruce Walker
bruce@think.com WT1M
------------------------------
Date: Tue, 15 Feb 1994 00:09:12 GMT
From: scubed!ihnp4.ucsd.edu!sdd.hp.com!vixen.cso.uiuc.edu!howland.reston.ans.net!cs.utexas.edu!oakhill!yosemite.sps.mot.com!ben@network.ucsd.edu
To: info-hams@ucsd.edu
References <gdavis.760825204@griffin>, <1994Feb10.171218.7423@dtint.dtint.com>, <1994Feb12.022037.1025@megatek.com>edu
Subject : Re: Nude amateur radio clubs
In article <1994Feb12.022037.1025@megatek.com>,
Jim Campbell <jimc@megatek.com> wrote:
>In article <1994Feb10.171218.7423@dtint.dtint.com> Allen Wallace <allen@dtint.dtint.com> writes:
>>
>>There might be, but I bet that they are all OMs and no YLs or XYLs!
>
> Close. There is a YL that checks in from Alaska on a fairly regular
>basis. The weeks when she shows up are the weeks we have more check-ins on the
>net. hmmmmmmm......
There have been one or two YL's besides her that have checked in as well.
IMHO, the number of YL's checking in is likely to be proportional to the
number of YL's that are hams rather than of those that are nudists.
--ben
--
Ben Thornton Amateur call: WD5HLS
Internet: ben@yosemite.sps.mot.com Motorola Inc., Austin, TX
Caution: Wearing clothes has been shown to cause permanent psychological
dependence on textiles. WEAR THEM AT YOUR OWN RISK.
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End of Info-Hams Digest V94 #153
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