Date: Mon, 21 Mar 94 14:09:02 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 #314
To: Info-Hams
Info-Hams Digest Mon, 21 Mar 94 Volume 94 : Issue 314
Today's Topics:
1994 Contest calendar enclosed
Daily Summary of Solar Geophysical Activity for 19 March
Daily Summary of Solar Geophysical Activity for 20 March
Macintosh Amateur Radio Software - January 1994
Packet, Internet & the FCC
QSL Route
US License Examination Opportunities Scheduled 3/18/94 to 6/20/94
WARNING: Potential Satellite Anomaly Warning Update - 20 March
What is (and how do I make) a diplexer?
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: 21 Mar 94 18:23:38 GMT
From: dog.ee.lbl.gov!agate!news.Brown.EDU!noc.near.net!xap!usenet@ucbvax.berkeley.edu
Subject: 1994 Contest calendar enclosed
To: info-hams@ucsd.edu
dbushong@wang.com (Dave Bushong)
>
>Here is the 1994 contest calendar from CQ.
[lots deleted]
>ARRL June VHF Contest 2/Jun 33
Looks like either CQ misprinted this or someone somewhere made an
assumption that the ARRL June VHF QSO Party is on its traditional
second weekend of June date. As it stands now, the ARRL June VHF
QSO Party is on the FIRST weekend of June in 1994.
I've already written letters to several ARRL people to complain
about the date change. Dave Sumner at ARRL HQ replied to tell me
he is passing it off to the ARRL Membership Services Department.
I don't think there's much chance of the date being moved back to
its traditional second weekend of June.
73,
Scott WO1G
sasminkey@eng.xyplex.com
------------------------------
Date: Sun, 20 Mar 1994 12:52:55 MST
From: ihnp4.ucsd.edu!usc!math.ohio-state.edu!cyber2.cyberstore.ca!nntp.cs.ubc.ca!alberta!ve6mgs!usenet@network.ucsd.edu
Subject: Daily Summary of Solar Geophysical Activity for 19 March
To: info-hams@ucsd.edu
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY
19 MARCH, 1994
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
(Based In-Part On SESC Observational Data)
SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 19 MARCH, 1994
---------------------------------------------------------
NOTE: Minor stratospheric warming exists over eastern Siberia, Alaska,
Canada, the Canadian Arctic, Greenland, and southern Europe. The
temperature gradient is reversed between 60N and the pole at 10 HPA
and above.
!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 078, 03/19/94
10.7 FLUX=089.1 90-AVG=106 SSN=011 BKI=3434 1113 BAI=013
BGND-XRAY=A6.1 FLU1=1.2E+06 FLU10=1.7E+04 PKI=4434 3223 PAI=015
BOU-DEV=034,042,023,042,006,008,006,021 DEV-AVG=022 NT SWF=00:000
XRAY-MAX= B1.3 @ 0730UT XRAY-MIN= A4.9 @ 0108UT XRAY-AVG= A8.9
NEUTN-MAX= +003% @ 1130UT NEUTN-MIN= -002% @ 0835UT NEUTN-AVG= +0.3%
PCA-MAX= +0.2DB @ 0025UT PCA-MIN= -0.2DB @ 2335UT PCA-AVG= +0.0DB
BOUTF-MAX=55344NT @ 0339UT BOUTF-MIN=55312NT @ 1813UT BOUTF-AVG=55331NT
GOES7-MAX=P:+000NT@ 0000UT GOES7-MIN=N:+000NT@ 0000UT G7-AVG=+066,+000,+000
GOES6-MAX=P:+120NT@ 1941UT GOES6-MIN=N:-122NT@ 0704UT G6-AVG=+086,+025,-050
FLUXFCST=STD:090,090,095;SESC:090,090,095 BAI/PAI-FCST=010,015,020/015,025,030
KFCST=2334 3222 2334 4334 27DAY-AP=013,060 27DAY-KP=4333 3222 2237 7756
WARNINGS=
ALERTS=
!!END-DATA!!
NOTE: The Effective Sunspot Number for 18 MAR 94 was 28.0.
The Full Kp Indices for 18 MAR 94 are: 4o 4+ 4+ 2+ 3o 2+ 2o 3+
The 3-Hr Ap Indices for 18 MAR 94 are: 30 32 31 9 15 9 7 20
Greater than 2 MeV Electron Fluence for 19 MAR is: 4.0E+08
SYNOPSIS OF ACTIVITY
--------------------
Solar activity was very low. Just one simple spot group,
7692 (N19E19), remains. The northernmost 8 degrees of the large
diagonally-oriented filament in the western hemisphere
disappeared during the first part of the day. A prominence
located near N21E90 was seen to erupt at 0633Z.
Solar activity forecast: solar activity is expected to
persist at very low levels.
The geomagnetic field has been at quiet to active levels
for the past 24 hours. Nighttime substorms have weakened. The
greater than 2 MeV electron event is declining, with peak
values of near 1.0E+04 observed during the day.
Geophysical activity forecast: the geomagnetic field is
expected to be predominantly unsettled the first half of the
forecast period. A favorably positioned coronal hole should
send high speed solar wind this way the latter part of the
interval. Active to minor storm conditions are anticipated
then.
Event probabilities 20 mar-22 mar
Class M 01/01/01
Class X 01/01/01
Proton 01/01/01
PCAF Green
Geomagnetic activity probabilities 20 mar-22 mar
A. Middle Latitudes
Active 25/25/45
Minor Storm 15/15/25
Major-Severe Storm 05/05/10
B. High Latitudes
Active 25/25/40
Minor Storm 15/15/30
Major-Severe Storm 05/05/15
HF propagation conditions were near-normal over all
regions. Similar conditions are expected over the next 24 to
48 hours. However, another well-placed coronal hole could
give degraded propagation again on 22 March.
COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS
========================================================
REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 19/2400Z MARCH
--------------------------------------------------------
NMBR LOCATION LO AREA Z LL NN MAG TYPE
7692 N18E19 161 0060 HSX 02 001 ALPHA
7688 N19W49 229 PLAGE
7691 N07W57 237 PLAGE
REGIONS DUE TO RETURN 20 MARCH TO 22 MARCH
NMBR LAT LO
7679 N02 084
7682 S19 069
LISTING OF SOLAR ENERGETIC EVENTS FOR 19 MARCH, 1994
----------------------------------------------------
BEGIN MAX END RGN LOC XRAY OP 245MHZ 10CM SWEEP
NONE
POSSIBLE CORONAL MASS EJECTION EVENTS FOR 19 MARCH, 1994
--------------------------------------------------------
BEGIN MAX END LOCATION TYPE SIZE DUR II IV
19/B0633 0813 N21E90 EPL
INFERRED CORONAL HOLES. LOCATIONS VALID AT 19/2400Z
---------------------------------------------------
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
------ ---- ---- ---- ---- -- ------ ------ --------- --------- ---------
18 Mar: 0235 0320 0539 C2.7
REGION FLARE STATISTICS FOR THE PREVIOUS UTC DAY
------------------------------------------------
C M X S 1 2 3 4 Total (%)
-- -- -- -- -- -- -- -- --- ------
Uncorrellated: 1 0 0 0 0 0 0 0 001 (100.0)
Total Events: 001 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: 21 Mar 94 14:36:11 GMT
From: agate!howland.reston.ans.net!math.ohio-state.edu!cyber2.cyberstore.ca!nntp.cs.ubc.ca!alberta!ve6mgs!usenet@ucbvax.berkeley.edu
Subject: Daily Summary of Solar Geophysical Activity for 20 March
To: info-hams@ucsd.edu
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY
20 MARCH, 1994
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
(Based In-Part On SESC Observational Data)
SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 20 MARCH, 1994
---------------------------------------------------------
NOTE: Minor stratospheric warming exists over southeastern Europe and western
Siberia, and over eastern Siberia, Alaska, and Canada with the adjacent
Arctic. The temperature gradient is reversed between 60N and the pole
above 10 HPA.
!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 079, 03/20/94
10.7 FLUX=088.6 90-AVG=106 SSN=011 BKI=3331 0222 BAI=008
BGND-XRAY=A4.9 FLU1=1.8E+06 FLU10=1.7E+04 PKI=3333 2233 PAI=011
BOU-DEV=021,021,023,008,003,012,012,019 DEV-AVG=014 NT SWF=00:000
XRAY-MAX= B1.3 @ 1139UT XRAY-MIN= A3.4 @ 1945UT XRAY-AVG= A6.6
NEUTN-MAX= +003% @ 2235UT NEUTN-MIN= -002% @ 1005UT NEUTN-AVG= +0.7%
PCA-MAX= +0.2DB @ 0015UT PCA-MIN= -0.4DB @ 0825UT PCA-AVG= +0.0DB
BOUTF-MAX=55340NT @ 1457UT BOUTF-MIN=55305NT @ 1939UT BOUTF-AVG=55329NT
GOES7-MAX=P:+000NT@ 0000UT GOES7-MIN=N:+000NT@ 0000UT G7-AVG=+082,+000,+000
GOES6-MAX=P:+144NT@ 1921UT GOES6-MIN=N:-086NT@ 0403UT G6-AVG=+099,+021,-040
FLUXFCST=STD:090,090,095;SESC:090,090,095 BAI/PAI-FCST=015,020,015/020,030,025
KFCST=2334 4334 3445 5333 27DAY-AP=060,046 27DAY-KP=2237 7756 7645 4333
WARNINGS=
ALERTS=
!!END-DATA!!
NOTE: The Effective Sunspot Number for 19 MAR 94 was 28.2.
The Full Kp Indices for 19 MAR 94 are: 4- 4- 3+ 4- 3o 2o 2+ 3-
The 3-Hr Ap Indices for 19 MAR 94 are: 24 24 17 21 16 7 9 13
Greater than 2 MeV Electron Fluence for 20 MAR is: 8.6E+08
SYNOPSIS OF ACTIVITY
--------------------
Solar activity was very low. Region 7692 (N18E06)
is the only region visible. No activity of any type was
reported.
Solar activity forecast: solar activity is expected to be
very low.
The geomagnetic field was quiet to unsettled. The greater than
2 MeV electron fluxes continue to hover near 1.0E+04.
Geophysical activity forecast: the geomagnetic field is
expected to be unsettled to mildly active over the next 24
hours. High speed solar wind from a well-located coronal
hole is due early on 22 March. This disturbance should slowly
weaken by the end of the interval.
Event probabilities 21 mar-23 mar
Class M 01/01/01
Class X 01/01/01
Proton 01/01/01
PCAF Green
Geomagnetic activity probabilities 21 mar-23 mar
A. Middle Latitudes
Active 25/45/40
Minor Storm 15/25/20
Major-Severe Storm 05/10/10
B. High Latitudes
Active 25/40/35
Minor Storm 15/30/25
Major-Severe Storm 05/15/15
HF propagation conditions were normal over all regions.
Similar conditions are expected over the next 72 hours. Minor
signal degradation is expected at times for high and polar
latitude night-sector paths.
COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS
========================================================
REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 20/2400Z MARCH
--------------------------------------------------------
NMBR LOCATION LO AREA Z LL NN MAG TYPE
7692 N18E06 160 0040 HSX 02 001 ALPHA
7688 N19W62 228 PLAGE
7691 N07W70 236 PLAGE
REGIONS DUE TO RETURN 21 MARCH TO 23 MARCH
NMBR LAT LO
7682 S19 071
7686 N08 037
LISTING OF SOLAR ENERGETIC EVENTS FOR 20 MARCH, 1994
----------------------------------------------------
BEGIN MAX END RGN LOC XRAY OP 245MHZ 10CM SWEEP
NONE
POSSIBLE CORONAL MASS EJECTION EVENTS FOR 20 MARCH, 1994
--------------------------------------------------------
BEGIN MAX END LOCATION TYPE SIZE DUR II IV
20/ 1039 1138 1315 LDE B1.3 156
INFERRED CORONAL HOLES. LOCATIONS VALID AT 20/2400Z
---------------------------------------------------
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 **
------------------------------
Date: 21 Mar 1994 14:27:02 -0500
From: hp81.prod.aol.net!search01.news.aol.com!not-for-mail@uunet.uu.net
Subject: Macintosh Amateur Radio Software - January 1994
To: info-hams@ucsd.edu
In article <2m4g40INNhgv@sweetpea.genrad.com>, dls@genrad.com (Diana L.
Carlson) writes:
And I have noted this in the latest version to be relased in amonth or so.
Thanks Diana... sorry you lost your Mac! I know that many people enjoyed using
your Hyoercard stacks to prep for their tests!
Has anyone else picked up the role of keeping the stacks up-to-date? Is there a
volunteer out there on the net?
73 for now.... c u on the shortwaves
Terry Stader - KA8SCP
America Online Ham Radio Club Host
Ham Radio Software for the Macintosh List Maintainer
------------------------------
Date: 21 Mar 94 12:57:37 GMT
From: ihnp4.ucsd.edu!dog.ee.lbl.gov!agate!howland.reston.ans.net!news.intercon.com!psinntp!psinntp!psinntp!barilvm!vms.huji.ac.il!gorski@network.ucsd.edu
Subject: Packet, Internet & the FCC
To: info-hams@ucsd.edu
In article <netnewsCMvvLn.964@netcom.com>, jrimmer@netcom.com writes:
>
> I've been seeing snippets of messages here and there about the Amateur
> rules and Packet, but've been unable to gleen a straight answer. What are the
> current rules for message forwarding? i.e. I want to set my computer up to
> recieve Internet mail, and then forward it over packet, is this kosher?
> According to a year old FAQ, it is as long as you "hand" forward the
> messages. I really don't want to do that... Furthermore, the FAQ specifies
> that the FCC sees Internet mail as third-party traffic, therefore must be
> screened by the control-op.
> Do these rules still apply? Or has Internet Mail forwarding been given
> a blessing by the FCC? What's up?
>
> Jason Rimmer
> Eclectic Technologies
> jrimmer@netcom.com
> Where technology and your desk meet (most of the time)
Now let us not forget third-party treaties and business traffic rules.
When In doubt I find that a good course is to follow the more restrictive of
the rulings that apply.
The may not really be an "on point answer" but it is my 2 cents/2 agarot worth.
Shalom and 73's from Jerusalem,
Azriel 4X1PI/W7SI
------------------------------
Date: 21 Mar 94 21:20:35 GMT
From: news-mail-gateway@ucsd.edu
Subject: QSL Route
To: info-hams@ucsd.edu
Hi Gang,
Does anybody out there in Cyberspace, know the QSL route for VP2MKY or
the where abouts of KY5R?
Thanks in advance
Lynn Geitgey KB0LRB
------------------------------
Date: 20 Mar 94 14:06:41 GMT
From: agate!howland.reston.ans.net!math.ohio-state.edu!cyber2.cyberstore.ca!nntp.cs.ubc.ca!alberta!ve6mgs!usenet@ucbvax.berkeley.edu
Subject: US License Examination Opportunities Scheduled 3/18/94 to 6/20/94
To: info-hams@ucsd.edu
AMATEUR RADIO EXAMINATION OPPORTUNITIES
*****************************************************************
Special Note: Amateur Radio licenses usually arrive between 8 and
10 weeks after the test session. The FCC considers their
processing time to be 90 days--from the date they receive the
application. The FCC usually receives the application one
to two weeks after the test session (once the VE Team and the
coordinating VEC have completed their processing).
Note: Codeless Technician to Technician w/HF upgraders (who pass a
Morse code test) will not receive a new license from the FCC.
The existing Technician license plus the CSCE conveying the Morse
code test credit is the only documentation issued for use of
the additional HF privileges.
*****************************************************************
The following test session information is provided by the
ARRL/VEC for the upcoming six to eight week period. For
further information, please contact the test session CONTACT
PERSON at the telephone number provided. If necessary, you
may contact the ARRL/VEC at 203-666-1541 x282 for additional
information. Electronic mail may be forwarded to the ARRL/VEC
via USENET at "bjahnke@arrl.org" or via MCI Mail to
MCI ID: 653-2312 or 215-5052.
Although the test session information presented here does
not indicate whether walk-ins are accepted or not, most test
sessions do allow walk-ins. We encourage you, however, to
always contact the CONTACT PERSON at the telephone number
provided so that the VE Team is aware that you be attending
the test session.
STILL NEED TO PREPARE FOR YOUR EXAM?
If you would like information on how to become licensed; or
how to locate Amateur Radio clubs, instructors, licensing
classes and/or Novice examiners in your area; please contact
the ARRL Educational Activities Department (EAD) at 203-666-
1541 x219. The EAD can also provide information on
recommended study materials. Electronic mail may be forwarded
to the ARRL EAD via USENET at "rwhite@arrl.org" or via MCI Mail to
MCI ID: 215-5052.
EXAM LISTINGS - DEFINITION OF FIELDS
STATE
Test Date,VEC,City,,Contact Phone,Contact Person
The SECOND field in the following listing specifies the VEC
which is coordinating this examination. This single-character
designator denotes the VEC as defined below. An "A" (for example)
indicates that this examination is coordinated by the ARRL/VEC.
For further information on any examinations listed, or if you do not
find any examinations listed for your area, you may contact
any of the coordinating VECs below.
A = ARRL/VEC, 225 Main St, Newington, CT 06111; (d) 203-666-1541
The 1994 test fee is $5.75.
X = Anchorage ARC, 2628 Turnagain Parkway, Anchorage, AK 99517;
(d) 907-786-8121, (n) 907-243-2221 (or) 907-276-5121
(or) 907-274-5546
C = Central Alabama VEC, 1215 Dale Dr SE, Huntsville, AL 35801;
205-536-3904
N = Charlotte VEC, 227 Bennett Ln, Charlotte, NC 28213;
704-596-2168
D = Great Lakes ARC VEC Inc., PO Box 273, Glenview, IL 60025;
708-486-8019
E = Golden Empire ARS, PO Box 508, Chico, CA 95927; No phone.
G = Greater Los Angeles ARG, 9737 Noble Ave, Sepulveda, CA 91343;
818-892-2068, 805-822-1473.
J = Jefferson ARC, PO Box 24368, New Orleans, LA 70184-4368;
504-737-2315. Test fee for 1994 is $5.00.
K = Koolau ARC, 45-529 Nakuluai St, Kaneohe, HI 96744;
808-235-4132
L = Laurel ARC Inc., PO Box 3039, Laurel, MD 20709-0039;
(d) 301-572-5124, 301-317-7819, (n) 301-588-3924
M = The Milwaukee RAC Inc., 1737 N 116th St, Wauwatosa, WI 53226;
414-774-6999. Test fee for 1994 is $5.00.
H = Mountain ARC, PO Box 10, Burlington, WV 26710; 304-289-3576,
301-724-0674
P = PHD ARA Inc., PO Box 11, Liberty, MO 64068; 816-781-7313
R = Sandarc-VEC, PO Box 2446, La Mesa, CA 91943-2446; 619-465-3926
S = Sunnyvale VEC ARC, PO Box 60307, Sunnyvale, CA 94088-0307;
408-255-9000
T = Triad Emergency ARC, 3504 Stonehurst Pl, High Point, NC 27265;
919-841-7576
W = Western Carolinas ARS VEC, 5833 Clinton Hwy - Suite 203,
Knoxville, TN 37912-2500; 615-688-7771.
The 1994 test fee is $5.75.
5 = W5YI-VEC, PO Box 565101, Dallas, TX 75356-5101; 817-461-6443
The 1994 test fee is $5.75.
EXAMINATION OPPORTUNITIES OUTSIDE THE UNITED STATES:
GUAM
03/20/94,A,Adelup,,627-646-7611,Harry Y Taguchi
06/19/94,A,Adelup,,627-646-7611,Harry Y Taguchi
US VIRGIN ISLANDS
04/09/94,A,St Croix,,809-778-3156,Frank Jaeger
05/14/94,A,ST Thomas,,809-774-4740,Ronald A Hall Sr
OTHER:
03/19/94,A,Australia,,089-531-305,Maury Hatfield
04/03/94,A,England,,144-423-870,Mike Parker N6SVL
03/19/94,A,Germany,,06561-18202,George L Hoke
03/26/94,A,Japan,,243-6092,Paul W Jackson USN
03/26/94,A,Japan,,098-633-1728,Alice Kottmyer
03/26/94,A,Papua New Guinea,,FAX-77-3504,Randall Pearson
04/17/94,A,Saipan,,670-234-6323,David Hardt
*EOF
------------------------------
Date: Sun, 20 Mar 1994 13:13:11 MST
From: ihnp4.ucsd.edu!mvb.saic.com!news.cerf.net!usc!howland.reston.ans.net!math.ohio-state.edu!cyber2.cyberstore.ca!nntp.cs.ubc.ca!alberta!ve6mgs!usenet@network.ucsd.edu
Subject: WARNING: Potential Satellite Anomaly Warning Update - 20 March
To: info-hams@ucsd.edu
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
POTENTIAL SATELLITE ANOMALY WARNING
ENDED: 05:00 UT, 20 MARCH
/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\
ATTENTION:
Energetic electrons at greater than 2 MeV are finally abating back
toward quieter levels. This disturbance lasted 11 days and is expected to
recur around 04 or 05 April when the coronal hole associated with this
activity returns to a geoeffective position.
** End of Warning **
------------------------------
Date: Mon, 21 Mar 94 11:48:23 GMT
From: mnemosyne.cs.du.edu!nyx!dtock@uunet.uu.net
Subject: What is (and how do I make) a diplexer?
To: info-hams@ucsd.edu
I know I could go and buy a diplexer ( to drive a VHF and a UHF antenna from
the single output of my dual bander) but they seem very expensive for what
should only be a couple of coils and a couple of capacitors (OK a few of each).
I have checked all my antenna and radio books, and all those I can find in
the library, but none of them even mentions diplexers.
Can someone please point me towards or provide design details, or a circuit
description, or ANYTHING. Maybe even a different (i.e.correct) name so I can
find them in the index. I don't believe there is nothing written about them.
Incidentally, I am UK based, so UK magazines (i.e. RadCom or PW) would do...
Thanks
David (GM0SYA)
------------------------------
End of Info-Hams Digest V94 #314
******************************
******************************