Date: Wed, 26 Jan 94 10:08:41 PST
From: Ham-Space Mailing List and Newsgroup <ham-space@ucsd.edu>
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Subject: Ham-Space Digest V94 #10
To: Ham-Space


Ham-Space Digest            Wed, 26 Jan 94       Volume 94 : Issue   10

Today's Topics:
                                Arsene
                     Daily IPS Report - 25 Jan 94
                Low Pass filter vs Band Pass - Mode JD
             Status of polar-orbiting weather satellites

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

Date: Mon, 24 Jan 1994 11:45:07 GMT
From: ucsnews!sol.ctr.columbia.edu!howland.reston.ans.net!torn!csd.unb.ca!upei.ca!UPEI.CA!seeler@network.ucsd.edu
Subject: Arsene
To: ham-space@ucsd.edu

Hi - Its been a long time since I've seen anything about Arsene and was
wondering if it has any funtions going at all at this time.

Tnx - Dave, VY2DCS
Internet : Seeler@upei.ca

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

Date: 24 Jan 94 23:29:06 GMT
From: swrinde!sdd.hp.com!think.com!cass.ma02.bull.com!syd.bull.oz.au!brahman!tmx!basser.cs.su.oz.au!metro!news.ci.com.au!eram!dave@network.ucsd.edu
Subject: Daily IPS Report - 25 Jan 94
To: ham-space@ucsd.edu

IPS RADIO AND SPACE SERVICES AUSTRALIA
Daily Solar And Geophysical Report
Issued at 2330 UT 24 January 1994
Summary for 24 January and Forecast up to 27 January
IPS Warning 02 was issued at 24/2200UT January and is current
for period January 27 - 29.
-----------------------------------------------------------

1A. SOLAR SUMMARY
Activity: low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number : 129/082

1B. SOLAR FORECAST
             25 January         26 January         27 January
Activity     Low                Low                Low
Fadeouts     None expected      None expected      None expected

Forecast 10.7 cm flux/Equivalent Sunspot Number : 130/084

1C. SOLAR COMMENT
None.
-----------------------------------------------------------

2A. MAGNETIC SUMMARY
Geomagnetic field at Learmonth : quiet

Estimated Indices : A   K           Observed A Index 23 January
    Learmonth       02  2111 0001
    Fredericksburg  02                          07
    Planetary       04                          05


2B. MAGNETIC FORECAST 
DATE      Ap    CONDITIONS
25 Jan    08    Quiet to unsettled.
26 Jan    08    Quiet to unsettled.
27 Jan    20    Unsettled to active.

2C. MAGNETIC COMMENT
Active periods expected during interval 27-29 Jan due to coronal
hole.

3A. GLOBAL HF PROPAGATION SUMMARY
             LATITUDE BAND
DATE        LOW            MIDDLE         HIGH 
24 Jan      normal         normal         normal         
PCA Event : None.
3B. GLOBAL HF PROPAGATION FORECAST
             LATITUDE BAND
DATE        LOW            MIDDLE         HIGH 
25 Jan      normal         normal         fair
26 Jan      normal         normal         fair
27 Jan      normal         fair           poor
3C. GLOBAL HF PROPAGATION COMMENT
Degraded comms expected at mid/high lats during interval 
27-29 January.

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

4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
MUFs at Sydney were about 15% above predicted monthly values

T index:  73

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
DATE   T-index  MUFs
25 Jan    75    About 15% above predicted monthly values.
26 Jan    75    About 15% above predicted monthly values.
27 Jan    75    About 15% above predicted monthly values.

Predicted Monthly T Index for January is 30.

4C. AUSTRALIAN REGION COMMENT
Degraded HF comms expected during Jan 27-29.
-- 
Dave Horsfall (VK2KFU)     VK2KFU @ VK2OP.NSW.AUS.OC     PGP 2.3
dave@esi.COM.AU           ...munnari!esi.COM.AU!dave    available

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

Date: Mon, 24 Jan 1994 11:53:17 GMT
From: ucsnews!sol.ctr.columbia.edu!howland.reston.ans.net!torn!csd.unb.ca!upei.ca!UPEI.CA!seeler@network.ucsd.edu
Subject: Low Pass filter vs Band Pass - Mode JD
To: ham-space@ucsd.edu

I have some desensing of my 440 rig on receive when the 2 meter rig fires 
up on Mode JD. This is not a MAJOR problem but I would like to resolve it.
I suspect that it involves the 3rd harmonic of the 2 meter Transmitter.

The books suggest using a low pass or band pass filter - but they differ as 
to which would be best ( opinion or operation differences?). I use the all 
IC275 for Dx and local operations as well and suspect that the low pass 
filter would be a good start. The filter in the VHF/UHF Dx book appears
to fit my needs - 35? db attenuation of the 2nd harmonic and 60 db
attenuation of the 3rd - with minimal (?) insertion loss. 

My questio is this - is the low pass filter the best way to solve this
particular issue - and if so - does anyone have any suggestions as to
any particular filter design / schematics - and comments as to how they/it
works?

Thanks for considering this post.

Dave, VY2DCS
Internet: Seeler@upei.ca

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

Date: Tue, 25 Jan 94 17:46:00 +0200
From: swrinde!cs.utexas.edu!howland.reston.ans.net!pipex!uknet!EU.net!news.eunet.fi!gate.compart.fi!compart!leo.wikholm@network.ucsd.edu
Subject: Status of polar-orbiting weather satellites
To: ham-space@ucsd.edu

   STATUS OF POLAR-ORBITING WEATHER SATELLITES
   ===========================================
   No. 2, January 25, 1994
   Station: Helsinki, +60.2N +25.1E

   ------------------------------------------------------
   NOAA 9        137,62 MHz  normal
   NOAA 10       137,50 MHz  VHF conflict with NOAA 12?
   NOAA 11       137,62 MHz  normal
   NOAA 12       137,50 MHz  normal
   Meteor 3-5    137,30 MHz  not actice in North
   Meteor 2-21   137,30 MHz  not active in North
   ------------------------------------------------------

   Leo Wikholm
   internet: leo.wikholm@compart.fi
   fidonet : 2:220/861

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

Date: 24 Jan 94 09:24:44 -0700
From: ucsnews!newshub.sdsu.edu!usc!howland.reston.ans.net!europa.eng.gtefsd.com!news.umbc.edu!eff!news.kei.com!sol.ctr.columbia.edu!hamblin.math.byu.edu!yvax.byu.edu!physc1.byu.edu!peterson@
To: ham-space@ucsd.edu

References <2hd6ji$q5e@hpavla.lf.hp.com>, <1994Jan17.145311.25166@ke4zv.atl.ga.us>, <CK0E5n.LG9@world.std.com>tr.colu
Subject : Re: Vacuum tubes in spacecraft?

In article <CK0E5n.LG9@world.std.com>, dts@world.std.com (Daniel T Senie) writes:
> In article <1994Jan17.145311.25166@ke4zv.atl.ga.us> gary@ke4zv.atl.ga.us (Gary Coffman) writes:
>>Note also that program bloat can be traced almost completely to having
>>excess RAM available. Programs naturally expand to fill the space available,
>>witness Wordstar. It was a great fast program on a 48 kb Z-80 system, but
> 
> common misconception. Wordstar NEVER fit in 48K. Sure it would run in a
> machine that had 48K, but every time you hit ^Y to delete a line, it
> had to swap in an overlay from disk to do the function, then swap back
> to the main code. When more memory is available, it is possible to
> improve performance.
> 
>>now it's a multi-megabyte dog on a Windows PC with 8+ megs of RAM. And
>>that's 166 times more RAM to develop a bit error that can crash the system.
>>To a large degree, reliability is a function of parts count. The fewer
>>parts, the less to go wrong.
>>
> 
> Actually in software the less is better philosopy does not always hold. To
> get program size smaller, one could always skip the bounds checking and input
> parameter checking. Fewer parts, but less reliability...
> 
>>Gary
>>-- 
>>Gary Coffman KE4ZV          |    You make it,     | gatech!wa4mei!ke4zv!gary
> 
> -- 
> ---------------------------------------------------------------
> Daniel Senie                 Internet:     dts@world.std.com
> Daniel Senie Consulting                    n1jeb@world.std.com
> 508-365-5352                 Compuserve:   74176,1347

Actually there are two other driving forces in the software bloat that are only 
allowed to operate because of the cheap RAM:  1)  The demand for software that 
requires no thought or training.  Some of this is good and some of it is 
useless "creeping featurism" (I have yet to understand why a top quality word
processing package would require you to remove your hands from the keyboard to
perform basic formatting functions).  And 2) the trend toward using high-level 
languages for all software development.  Most of those "lean and mean" packages 
of the past were written in optimized assembly code because RAM was tight.  Now 
they don't have to put any effort into optimizing the code and are able to 
write using high-level languages and compilers that generate absolutely 
horrendous code (from an efficiency standpoint).  Yes, that allows them to meet 
the demands of (1) above more quickly but at a tremondous cost in storage space 
(just for grins look at the bloat in the distribution disks for ANY package 
over the last few years - things that used to be delivered on 2 360K floppies 
now require 4 to 6 1.44M floppies and add data compression to boot).  Whether 
this whole trend is good or bad is a totally religious argument (hardware is 
cheap and features are nice versus why do I need so much hardware just to run 
a simple application).

However, any way you look at it my hat goes off to the programmers who are able
to  fit the entire control program for the Shuttle into the memory on those 
computers.  I can guarantee they are not using the bloated high-level languages 
that you normally see in the PC world to do that.

Bryan Peterson, ki7td
peterson@physc1.byu.edu

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

End of Ham-Space Digest V94 #10
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