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1994-06-04
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31KB
Date: Sun, 12 Dec 93 06:12:54 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 V93 #1454
To: Info-Hams
Info-Hams Digest Sun, 12 Dec 93 Volume 93 : Issue 1454
Today's Topics:
Kenwood ts-820 questions
Life is too short WITH 2 KW!!!!!
Pasadena CA Special Event Station
Scratchi, January, 1960
Weekly Solar Terrestrial Forecast & Review for 10 December
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: Sat, 11 Dec 1993 06:57:06 GMT
From: news.service.uci.edu!cerritos.edu!news.Arizona.EDU!math.arizona.edu!noao!asuvax!gatech!swrinde!cs.utexas.edu!@network.ucsd.edu
Subject: Kenwood ts-820 questions
To: info-hams@ucsd.edu
HI, I have several questions regarding my Kenwood TS-820 (with
digital display) I am hoping you can all help me with this...
First, I am looking for some accesories. I don't have lots of money
so trades would be nice however I can supply cash if required..
I am looking for the following: External VFO, 2 meter transverter
and dc power adaptor. If you have any of these and want to
get rid of them please let me know.
I would also like to know where to get replacement output tubes for
this radio. Considering its age, I figure it would be a good idea to
get a few while the getting is good. What type of tubes does this
radio use? What brand/type would make the best replacement?
Now for some tech stuff..
I would like to know how to control the power output of the radio
during vocie transmission. I know how to on CW (Just reduce car) but
I don't know the proper way to do this on voice.
My radio does not seem to put out its full rated 200 watts. Any
ideas on this or any way to test it. It is possible that my MFJ d
eluxe versa tuner II power meter may be innacurate. I have been
told not to trust the readings on these meters.
I have a Cmos super keyer II which is NOT compatable with the negative
switching on the Kenwood. For any of you that have this problem, I have
found a simple fix, here it is.
1. remove the phono plug from the end of your keyer cable.
2. Reverse the wires, soldering the origonal center wire to the outer
connector of the plug.
3. To the center plug insert a resistor whos value is high enough
to reduce the voltage presented to the keyer terminals (use a VOM
and voltage divider equation) I used the higest possible value
that still allowed the keyer to make the radio transmit.
4. Solder the remaining wire to the other end of this resistor.
5. Attach a diode across the terminals. This protects the keyer
transistor from any potential spikes from the transmitter. (got
this from the Art of Electronics)
6. Thats all there is to it. I placed the resistor and diode right
in the case for the phono plug. Use some heat shrink for short
protection.
This seems to work fine and has not melted my keyer yet. If
anyone has any comments on this or improvements please let me
know.
Finaly, I would like to build a field strength meter. I was thinking
that an opamp based circuit would be ideal for this. If anyone
can help me with this I would appreciate it. I know I could buy one
cheaply, but I would like to build my own.
Thanks in advance for any comments or suggestions. Please email your
answers to lvin@cosmic.physics.utah.edu
I will summarize all responces.
Thanks again
Chris (KB7YOU)
------------------------------
Date: 9 Dec 93 18:44:18 GMT
From: pravda.sdsc.edu!usc!elroy.jpl.nasa.gov!swrinde!sgiblab!rtech!ingres!kerry@network.ucsd.edu
Subject: Life is too short WITH 2 KW!!!!!
To: info-hams@ucsd.edu
In article <2e55g6$no3@news.acns.nwu.edu> lapin@casbah.acns.nwu.edu (Gregory Lapin) writes:
>Do QRP operators live longer than QRO operators?
>
>What ever happened to that other stimulating thread ;)
>
:-) As long as the lights don't dim (too much) when you key the transmitter,
:-) aren't you operating QRP?
------------------------------
Date: Wed, 8 Dec 1993 20:46:11 GMT
From: nntp.ucsb.edu!library.ucla.edu!agate!howland.reston.ans.net!math.ohio-state.edu!usc!nic.csu.net!csun.edu!VFOAO007%VAX.CSUN.EDU@network.ucsd.edu
Subject: Pasadena CA Special Event Station
To: info-hams@ucsd.edu
On Sunday, 12 December 1993, the Pasadena Radio Club will field a special
event station to celebrate the rebuilding of the beautiful 80 year old
Colorado Street Bridge over the Arroyo Seco just south of the Rose Bowl.
The station will be active from 10:00 a.m. PST (1800 UTC) to 4:00 p.m. PST
(2400 UTC) on three bands:
21.335 MHz (+/-)
14.260 MHz (+/-)
147.150 MHz repeater (W6VIO) (+600 KHz, PL 131.8)
For a souvenir certificate, send a QSL and $1 to
W6KA
Post Office Box 282
Altadena CA 91003
+---------------------------------------------------------------------------+
| Michael Reagan KK6WO Circulation Unit Coordinator |
| MReagan@vax.csun.edu Oviatt Library /OLIB |
| (818) 885-2274 California State University |
| fax (818) 885-2676 Northridge CA 91328-1289 |
| packet KK6WO@W6VIO.#SOCA.CA.USA.NA |
| --... ...-- -.. . de gustibus non est disputandum -.- -.- -.... .-- --- |
+---------------------------------------------------------------------------+
------------------------------
Date: Fri, 10 Dec 1993 15:59:35 GMT
From: ucsnews!sol.ctr.columbia.edu!howland.reston.ans.net!math.ohio-state.edu!sdd.hp.com!hpscit.sc.hp.com!hplextra!hplb!hpwin052!hpqmoea!dstock@network.ucsd.edu
Subject: Scratchi, January, 1960
To: info-hams@ucsd.edu
I ENJOYED reading Myron's posting.
Scratchi was previously totally unknown to me, so I just read what was
there.
I interpreted it as a commentry on the different interests and
viewpoints of different generations. It said that two different
generations do not understand each other, and can fail to predict this.
It did not seem to attack either generation.
I thought there was a strong element of lampooning old fashioned
stereotype characterisation.
Perhaps Myron's parody is a little too subtle for everyone to
recognise it ? Even if he now states his intent, no matter what that
intent was, not everyone will believe him. We will never know with
certainty.
Foreigners and children have the ability to see things, and ask
questions that are too fundamental for others to notice (or dare)
Cheers
David GM4ZNX
------------------------------
Date: Thu, 9 Dec 1993 18:16:20 MST
From: pacbell.com!sgiblab!swrinde!elroy.jpl.nasa.gov!usc!math.ohio-state.edu!news.cyberstore.ca!nntp.cs.ubc.ca!alberta!adec23!ve6mgs!usenet@network.ucsd.edu
Subject: Weekly Solar Terrestrial Forecast & Review for 10 December
To: info-hams@ucsd.edu
--- SOLAR TERRESTRIAL FORECAST AND REVIEW ---
December 10 to December 19, 1993
Report Released by Solar Terrestrial Dispatch
P.O. Box 357, Stirling, Alberta, Canada
T0K 2E0
Accessible BBS System: (403) 756-3008
---------
SOLAR AND GEOPHYSICAL ACTIVITY FORECASTS AT A GLANCE
----------------------------------------------------
|10.7 cm|HF Propagation +/- CON|SID AU.BKSR DX| Mag| Aurora |
|SolrFlx|LO MI HI PO SWF %MUF %|ENH LO MI HI LO MI HI %|K Ap|LO MI HI|
--|-------|-----------------------|-------------------------|----|--------|
10| 095 | G G F F 25 00 70| 20 NA NA NA 00 00 10 35|2 07|NV NV LO|
11| 095 | G G F F 25 00 70| 20 NA NA NA 00 00 10 35|2 10|NV NV LO|
12| 095 | G G F F 25 00 70| 20 NA NA NA 00 00 10 35|2 12|NV NV LO|
13| 095 | G G F F 25 00 70| 20 NA NA NA 01 05 15 35|2 12|NV NV LO|
14| 095 | G G F F 25 00 70| 20 NA NA NA 01 05 15 35|2 12|NV NV LO|
15| 090 | G G F F 25 00 70| 20 NA NA NA 01 10 20 30|3 15|NV NV MO|
16| 090 | G G P P 25 -10 65| 20 NA NA NA 01 20 35 30|4 20|NV NV MO|
17| 090 | G G P P 25 -10 65| 20 NA NA NA 02 10 25 30|3 15|NV NV MO|
18| 085 | G G F F 25 -05 65| 20 NA NA NA 02 05 20 35|3 13|NV NV MO|
19| 085 | G G F F 25 00 65| 20 NA NA NA 02 05 15 35|2 10|NV NV LO|
PEAK PLANETARY 10-DAY GEOMAGNETIC ACTIVITY OUTLOOK (10 DEC - 19 DEC)
________________________________________________________________________
| EXTREMELY SEVERE | | | | | | | | | | | HIGH |
| VERY SEVERE STORM | | | | | | | | | | | HIGH |
| SEVERE STORM | | | | | | | | | | | MODERATE |
| MAJOR STORM | | | | | | | | | | | LOW - MOD. |
| MINOR STORM | | | | | | | | | | | LOW |
| VERY ACTIVE | | | | | | | | | | | NONE |
| ACTIVE | | | | | | * |***|** | | | NONE |
| UNSETTLED | * |** |** |***|***|***|***|***|** | * | NONE |
| QUIET |***|***|***|***|***|***|***|***|***|***| NONE |
| VERY QUIET |***|***|***|***|***|***|***|***|***|***| NONE |
|-------------------|---|---|---|---|---|---|---|---|---|---|------------|
| Geomagnetic Field |Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun| Anomaly |
| Conditions | Given in 8-hour UT intervals | Intensity |
|________________________________________________________________________|
CONFIDENCE LEVEL: 65%
NOTES:
Predicted geomagnetic activity is based heavily on recurrent
phenomena. Transient energetic solar events cannot be predicted reliably over
periods in excess of several days. Hence, there may be some deviations from
the predictions due to the unpredictable transient solar component.
60-DAY GRAPHICAL ANALYSIS OF GEOMAGNETIC ACTIVITY
____________________________________________________________
77 | J |
73 | J |
69 | J |
65 | J |
62 | J |
58 | J |
54 | J |
50 | J J|
46 | J J|
42 | J J|
39 | M J M J|
35 | M J MM J|
31 | M J MM J|
27 | A M JAA MM J|
23 |A A M JAA MM J|
19 |AA A M JAA A AMM J|
15 |AA AAMA JAAA AA AMM AJ|
12 |AAUU U AAMA JAAAU AA AMM AJ|
8 |AAUUU UUUAAMAU U UJAAAUUU UUUU AAU U U AMMU AJ|
4 |AAUUUQQQUQQUUUUAAMAUQUUQUJAAAUUUQQUUUUQAAUQQQQQUQQUQAMMUUQAJ|
0 |AAUUUQQQUQQUUUUAAMAUQUUQUJAAAUUUQQUUUUQAAUQQQQQUQQUQAMMUUQAJ|
------------------------------------------------------------
Chart Start Date: Day #283
NOTES:
This graph is determined by plotting the greater of either the planetary
A-index or the Boulder A-index. Graph lines are labelled according
to the severity of the activity which occurred on each day. The left-
hand column represents the associated A-Index for that day.
Q = Quiet, U = Unsettled, A = Active, M = Minor Storm,
J = Major Storm, and S = Severe Storm.
CUMULATIVE GRAPHICAL CHART OF THE 10.7 CM SOLAR RADIO FLUX
----------------------------------------------------------
____________________________________________________________
110 | |
109 | * |
108 | * |
107 | * * |
106 | * * * |
105 | * *** **|
104 | ****** **|
103 |* * ****** ***|
102 |* * * ****** ***|
101 |* * ** **********|
100 |* ****** ** **********|
099 |* ****** *** **********|
098 |** ****** *** **********|
097 |** * *********** **********|
096 |** *** *********** **********|
095 |*** * **** *********** **********|
094 |*** * ** ***** ************* ***********|
093 |*** * ** ****** ************** ************|
092 |*** * ***** * ******* ************** ************|
091 |****** ***** *********** *************** ************|
090 |******* ***** ************* ****************************|
089 |******* ****** * ******************************************|
088 |******* ****** * *******************************************|
087 |************************************************************|
086 |************************************************************|
------------------------------------------------------------
Chart Start: Day #284
GRAPHICAL ANALYSIS OF 90-DAY AVERAGE SOLAR FLUX
-----------------------------------------------
____________________________________________________________
098 | |
097 | **|
096 |****** ******|
095 |************* **********|
094 |********************** ***** **********************|
093 |************************************************************|
092 |************************************************************|
------------------------------------------------------------
Chart Start: Day #284
NOTES:
The 10.7 cm solar radio flux is plotted from data reported
by the Penticton Radio Observatory (formerly the ARO from
Ottawa). High solar flux levels denote higher levels of
activity and a greater number of sunspot groups on the Sun.
The 90-day mean solar flux graph is charted from the 90-day
mean of the 10.7 cm solar radio flux.
CUMULATIVE GRAPHICAL CHART OF SUNSPOT NUMBERS
---------------------------------------------
____________________________________________________________
105 | |
101 | * |
097 | * ** ** * |
093 | * ** ** ** |
089 | * * *** ***** |
085 | *** ********* |
081 | * **** **********|
077 | * **** * * **********|
073 | * * **** ** * ***********|
069 |** * **** * **** ***********|
065 |** * **** *** **** ***********|
061 |*** * ********* ***** ***********|
057 |*** ** ********* * ******* ***********|
053 |*** ** ********* ********* ************|
049 |*** ************* **********************|
045 |*** ************** * ***********************|
041 |*** ************** * **** ************************|
037 |*** *************** * **** ** *************************|
033 |**** *************** ** **** ** *************************|
029 |*********************** **** ** **************************|
025 |************************ ******** **************************|
021 |************************ ******** **************************|
017 |********************************* **************************|
013 |************************************************************|
------------------------------------------------------------
Chart Start: Day #283
NOTES:
The graphical chart of sunspot numbers is created from the
daily sunspot number counts as reported by the SESC.
HF RADIO SIGNAL PROPAGATION PREDICTIONS (10 DEC - 19 DEC)
High Latitude Paths
________________________________________________________
| EXTREMELY GOOD | | | | | | | | | | |
| VERY GOOD | | | | | | | | | | |
CONFIDENCE | GOOD | | | | | | | | | | |
LEVEL | FAIR |***|***|***|***|***|***| * | * | **|***|
------- | POOR | | | | | | |* *|* *|* | |
70% | VERY POOR | | | | | | | | | | |
| EXTREMELY POOR | | | | | | | | | | |
|----------------|---|---|---|---|---|---|---|---|---|---|
| PROPAGATION |Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun|
| QUALITY | Given in 8 Local-Hour Intervals |
--------------------------------------------------------
Middle Latitude Paths
________________________________________________________
| EXTREMELY GOOD | | | | | | | | | | |
| VERY GOOD | | | | | | | | | | |
CONFIDENCE | GOOD |***|***|***|***|***|***| **| **|***|***|
LEVEL | FAIR | | | | | | |* |* | | |
------- | POOR | | | | | | | | | | |
65% | VERY POOR | | | | | | | | | | |
| EXTREMELY POOR | | | | | | | | | | |
|----------------|---|---|---|---|---|---|---|---|---|---|
| PROPAGATION |Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun|
| QUALITY | Given in 8 Local-Hour Intervals |
--------------------------------------------------------
Low Latitude Paths
________________________________________________________
| EXTREMELY GOOD | | | | | | | | | | |
| VERY GOOD | | | | | | | | | | |
CONFIDENCE | GOOD |***|***|***|***|***|***|***|***|***|***|
LEVEL | FAIR | | | | | | | | | | |
------- | POOR | | | | | | | | | | |
75% | VERY POOR | | | | | | | | | | |
| EXTREMELY POOR | | | | | | | | | | |
|----------------|---|---|---|---|---|---|---|---|---|---|
| PROPAGATION |Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun|
| QUALITY | Given in 8 Local-Hour Intervals |
--------------------------------------------------------
NOTES:
NORTHERN HEMISPHERE SOUTHERN HEMISPHERE
High latitudes >= 55 deg. N. | High latitudes >= 55 deg. S.
Middle latitudes >= 40 < 55 deg. N. | Middle latitudes >= 30 < 55 deg. S.
Low latitudes < 40 deg. N. | Low latitudes < 30 deg. S.
POTENTIAL VHF DX PROPAGATION PREDICTIONS (10 DEC - 19 DEC)
INCLUDES SID AND AURORAL BACKSCATTER ENHANCEMENT PREDICTIONS
HIGH LATITUDES
__________________________________________________ ___________________
| FORECAST | Given in 8 hour local time intervals | |SWF/SID ENHANCEMENT|
|CONFIDENCE|Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun| |F|S|S|M|T|W|T|F|S|S|
|__________|___|___|___|___|___|___|___|___|___|___| |-|-|-|-|-|-|-|-|-|-|
| 0% |***|***|***|***|***|***|***|***|***|***| 0%|*|*|*|*|*|*|*|*|*|*|
| 20% |***|***|***|***|***|***|***|***|***|***| 20%|*|*|*|*|*|*|*|*|*|*|
| 40% |***|***|***|***|***|***|***|***|***|***| 40%| | | | | | | | | | |
| 60% | * | * | * | * | * | * | * | * | * | * | 60%| | | | | | | | | | |
| 80% | | | | | | | | | | | 80%| | | | | | | | | | |
| 100% | | | | | | | | | | |100%| | | | | | | | | | |
|==========|===|===|===|===|===|===|===|===|===|===| |-------------------|
| 100% | | | | | | | | | | |100%| | | | | | | | | | |
| 80% | | | | | | | | | | | 80%| | | | | | | | | | |
| 60% | | | | | | | | | | | 60%| | | | | | | | | | |
| 40% | * | * | * | * | * | * | * | * | * | * | 40%| | | | | | | | | | |
| 20% |***|***|***|***|***|***|***|***|***|***| 20%| | | | | | |*|*| | |
| 0% |***|***|***|***|***|***|***|***|***|***| 0%|*|*|*|*|*|*|*|*|*|*|
|----------|---|---|---|---|---|---|---|---|---|---| |-|-|-|-|-|-|-|-|-|-|
|CHANCE OF |Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun| |F|S|S|M|T|W|T|F|S|S|
| VHF DX | Given in 8 hour local time intervals | |AURORAL BACKSCATTER|
|__________|_______________________________________| |___________________|
MIDDLE LATITUDES
__________________________________________________ ___________________
| FORECAST | Given in 8 hour local time intervals | |SWF/SID ENHANCEMENT|
|CONFIDENCE|Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun| |F|S|S|M|T|W|T|F|S|S|
|__________|___|___|___|___|___|___|___|___|___|___| |-|-|-|-|-|-|-|-|-|-|
| 0% |***|***|***|***|***|***|***|***|***|***| 0%|*|*|*|*|*|*|*|*|*|*|
| 20% |***|***|***|***|***|***|***|***|***|***| 20%|*|*|*|*|*|*|*|*|*|*|
| 40% |***|***|***|***|***|***|***|***|***|***| 40%| | | | | | | | | | |
| 60% |***|***|***|***|***|***|** |** |***|***| 60%| | | | | | | | | | |
| 80% | | | | | | | | | | | 80%| | | | | | | | | | |
| 100% | | | | | | | | | | |100%| | | | | | | | | | |
|==========|===|===|===|===|===|===|===|===|===|===| |-------------------|
| 100% | | | | | | | | | | |100%| | | | | | | | | | |
| 80% | | | | | | | | | | | 80%| | | | | | | | | | |
| 60% | | | | | | | | | | | 60%| | | | | | | | | | |
| 40% | **| **| **| **| **| **| * | * | **| **| 40%| | | | | | | | | | |
| 20% |***|***|***|***|***|***|***|***|***|***| 20%| | | | | | |*| | | |
| 0% |***|***|***|***|***|***|***|***|***|***| 0%|*|*|*|*|*|*|*|*|*|*|
|----------|---|---|---|---|---|---|---|---|---|---| |-|-|-|-|-|-|-|-|-|-|
|CHANCE OF |Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun| |F|S|S|M|T|W|T|F|S|S|
| VHF DX | Given in 8 hour local time intervals | |AURORAL BACKSCATTER|
|__________|_______________________________________| |___________________|
LOW LATITUDES
__________________________________________________ ___________________
| FORECAST | Given in 8 hour local time intervals | |SWF/SID ENHANCEMENT|
|CONFIDENCE|Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun| |F|S|S|M|T|W|T|F|S|S|
|__________|___|___|___|___|___|___|___|___|___|___| |-|-|-|-|-|-|-|-|-|-|
| 0% |***|***|***|***|***|***|***|***|***|***| 0%|*|*|*|*|*|*|*|*|*|*|
| 20% |***|***|***|***|***|***|***|***|***|***| 20%|*|*|*|*|*|*|*|*|*|*|
| 40% |***|***|***|***|***|***|***|***|***|***| 40%| | | | | | | | | | |
| 60% |***|***|***|***|***|***|***|***|***|***| 60%| | | | | | | | | | |
| 80% | | | | | | | | | | | 80%| | | | | | | | | | |
| 100% | | | | | | | | | | |100%| | | | | | | | | | |
|==========|===|===|===|===|===|===|===|===|===|===| |-------------------|
| 100% | | | | | | | | | | |100%| | | | | | | | | | |
| 80% | | | | | | | | | | | 80%| | | | | | | | | | |
| 60% | * | * | * | * | * | * | * | * | * | * | 60%| | | | | | | | | | |
| 40% |***|***|***|***|***|***|***|***|***|***| 40%| | | | | | | | | | |
| 20% |***|***|***|***|***|***|***|***|***|***| 20%| | | | | | | | | | |
| 0% |***|***|***|***|***|***|***|***|***|***| 0%|*|*|*|*|*|*|*|*|*|*|
|----------|---|---|---|---|---|---|---|---|---|---| |-|-|-|-|-|-|-|-|-|-|
|CHANCE OF |Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun| |F|S|S|M|T|W|T|F|S|S|
| VHF DX | Given in 8 hour local time intervals | |AURORAL BACKSCATTER|
|__________|_______________________________________| |___________________|
NOTES:
These VHF DX prediction charts are defined for the 30 MHz to 220 MHz
bands. They are based primarily on phenomena which can affect VHF DX
propagation globally. They should be used only as a guide to potential
DX conditions on VHF bands. Latitudinal boundaries are the same as those for
the HF predictions charts.
AURORAL ACTIVITY PREDICTIONS (10 DEC - 19 DEC)
High Latitude Locations
________________________________________________________
| EXTREMELY HIGH | | | | | | | | | | |
CONFIDENCE | VERY HIGH | | | | | | | | | | |
LEVEL | HIGH | | | | | | | | | | |
------- | MODERATE | | | | | * |***| * | * | | |
70% | LOW |***|***|***|***|***|***|***|***|***|***|
| NOT VISIBLE |***|***|***|***|***|***|***|***|***|***|
|----------------|---|---|---|---|---|---|---|---|---|---|
| AURORAL |Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun|
| INTENSITY | Eve.Twilight/Midnight/Morn.Twilight |
--------------------------------------------------------
Middle Latitude Locations
________________________________________________________
| EXTREMELY HIGH | | | | | | | | | | |
CONFIDENCE | VERY HIGH | | | | | | | | | | |
LEVEL | HIGH | | | | | | | | | | |
------- | MODERATE | | | | | | | | | | |
75% | LOW | | | | | | * | | | | |
| NOT VISIBLE |***|***|***|***|***|***|***|***|***|***|
|----------------|---|---|---|---|---|---|---|---|---|---|
| AURORAL |Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun|
| INTENSITY | Eve.Twilight/Midnight/Morn.Twilight |
--------------------------------------------------------
Low Latitude Locations
________________________________________________________
| EXTREMELY HIGH | | | | | | | | | | |
CONFIDENCE | VERY HIGH | | | | | | | | | | |
LEVEL | HIGH | | | | | | | | | | |
------- | MODERATE | | | | | | | | | | |
90% | LOW | | | | | | | | | | |
| NOT VISIBLE |***|***|***|***|***|***|***|***|***|***|
|----------------|---|---|---|---|---|---|---|---|---|---|
| AURORAL |Fri|Sat|Sun|Mon|Tue|Wed|Thu|Fri|Sat|Sun|
| INTENSITY | Eve.Twilight/Midnight/Morn.Twilight |
--------------------------------------------------------
NOTE:
Version 2.00b of our Professional Dynamic Auroral Oval Simulation
Software Package is now available. This professional software is
particularly valuable to radio communicators, aurora photographers,
educators, and astronomers. For more information regarding this software,
contact: "Oler@Rho.Uleth.CA", or "COler@Solar.Stanford.Edu".
For more information regarding these charts, send a request for the
document, "Understanding Solar Terrestrial Reports" to: "Oler@Rho.Uleth.Ca"
or to: "COler@Solar.Stanford.Edu". This document, as well as others and
related data/forecasts exist on the STD BBS at: (403) 756-3008.
** End of Report **
------------------------------
Date: 8 Dec 1993 22:22:31 GMT
From: munnari.oz.au!sgiblab!sgigate.sgi.com!olivea!hal.com!darkstar.UCSC.EDU!cats.ucsc.edu!haynes@network.ucsd.edu
To: info-hams@ucsd.edu
References <2e26th$e1s@nntpd.lkg.dec.com>, <gregCHooL3.Jt7@netcom.com>, <1993Dec8.192104.23873@TorreyPinesCA.ncr.com>ynes
Subject : Re: Scratchi, January, 1960
Just to point out that the Scratchi column was controversial during the
time it was being published too. I distinctly remember an exchange of
letters to the editor arguing over the point.
Anyone remember the "Heinrich Schnibble" items from Saturday Evening Pest of
the same period?
--
haynes@cats.ucsc.edu
haynes@cats.bitnet
"Ya can talk all ya wanna, but it's dif'rent than it was!"
"No it aint! But ya gotta know the territory!"
Meredith Willson: "The Music Man"
------------------------------
End of Info-Hams Digest V93 #1454
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