Date: Sun, 23 Jan 94 23:40:04 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 #69
To: Info-Hams


Info-Hams Digest            Sun, 23 Jan 94       Volume 94 : Issue   69

Today's Topics:
                                 ???
                Are there any RS232C cards for PCMCIA?
                   Bird Problems with Yagi Antenna
                           callsign servers
                               CW Books
                    CW filters and DSP-9 (2 msgs)
      Daily Summary of Solar Geophysical Activity for 22 January
                    International Callsign Server
               The differences in CW filter performance

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: Thu, 20 Jan 1994 01:32:18 GMT
From: usenet.coe.montana.edu!netnews.nwnet.net!ns1.nodak.edu!plains!drusteba@decwrl.dec.com
Subject: ???
To: info-hams@ucsd.edu



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

Date: 21 Jan 94 10:00:22 GMT
From: ucsnews!sol.ctr.columbia.edu!howland.reston.ans.net!cs.utexas.edu!swrinde!sgiblab!sgigate.sgi.com!olivea!koriel!sh.wide!wnoc-tyo-news!aist-nara!ccsparc01!icspub!ce-gw!ee!kitagawa@network.ucsd.
Subject: Are there any RS232C cards for PCMCIA?
To: info-hams@ucsd.edu

Thank you everyone who responded by mail or news.

I> Are there any RS232C cards for PCMCIA slot?

   > you may want to consider "dockable" laptops.

Unfortunately I've never heard of the docking station for my favorite
T1950. I am told that there are some serial interface cards for PCMCIA
(by IBM and others) but still don't have specific model numbers.

I> I'm also looking for PCMCIA Ethernet cards for 10base-2 (Coax)

I've got the info that there is one for T1950;
NWETH02 Noteworthy 10base2 PCMCIA type II Ethernet card.

   > You could go with the old, yet trusty Xircom 10-Base2 external LAN
   >  adapter....

Oh, it might be even better if I can save a PCMCIA slot. Thanks!

I> FYI (to Hams only, probably contesters only): Why do I need so many
I> serial ports? Yes, I want to run CT (by K1EA) in multi-multi station.

I am informed that CT ver 8.47 has implemented a single-directional
loop which requires only one serial port per computer. If it works
fine, I don't need a serial port card nor an Ethernet card, i.e. the
best solution for me.

Masahiro Kitagawa  <kitagawa@ee.es.osaka-u.ac.jp>
Electrical Engineering, Engineering Science, Osaka University

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

Date: Sun, 23 Jan 1994 06:28:08 GMT
From: sdd.hp.com!nigel.msen.com!usenet.ins.cwru.edu!ukma!news2.uunet.ca!iceonline!icebox!janc@network.ucsd.edu
Subject: Bird Problems with Yagi Antenna
To: info-hams@ucsd.edu

>This produces a messy roof and a serious hazard to parked cars, cats and 
>small children on the ground :-)
>
>Also, however, the elements have been getting torqued seriously out of 
>plane by the weight of the lil' chirpers. They seem not to have an eye 
>for symmetry and apparently don't understand about balanced loads, 
>balanced feed lines, or the like.
>

Some of the local hams in this area have mounted plastic Owls atop the antenna
and tuned to compensate (if and when necessary).  It seems to keep the real
feathered fiends at bay.

 -----------------------------------------------------------------------------
                            : If you eat a live toad first thing in the
 janc@icebox.iceonline.com  : morning, nothing worse will happen to you all
                            : day.
                            : To you or the toad.
 -----------------------------------------------------------------------------

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

Date: Fri, 21 Jan 1994 21:34:58 GMT
From: utcsri!newsflash.concordia.ca!sifon!clouso.crim.ca!hobbit.ireq.hydro.qc.ca!barde!vaillan@uunet.uu.net
Subject: callsign servers
To: info-hams@ucsd.edu

In article 7Fy@ucdavis.edu, ez006683@othello.ucdavis.edu (Daniel D. Todd) writes:
>Hi all,
>I was trying to access the buffalo callsign server but I keep getting an 
>error.  Is this a network problem a local problem or an operator problem.
>
>othello% telnet electra.cs.buffalo.edu 2000
>telnet: service to this port is not available
>othello% telnet callsign.cs.buffalo.edu 2000
>telnet: service to this port is not available
>othello% telnet 128.205.32.2 2000
>telnet: service to this port is not available
>othello% 
>
>Thanks for the help,
>Dan
>
>--
>*---------------------------------------------------------------------*
>* Daniel D. Todd      Packet: KC6UUD@KE6LW.#nocal.ca.usa              *
>*                   Internet: ddtodd@ucdavis.edu                      *
>*                 Snail Mail: 1750 Hanover #102                       *
>*                             Davis CA 95616                          *
>*---------------------------------------------------------------------*
>*       I do not speak for the University of California....           *
>*       and it sure as hell doesn't speak for me!!                    *
>*---------------------------------------------------------------------*
>      


You must have network problems...

Here is what I get:

telnet 128.205.32.2 2000
Trying 128.205.32.2 ...
Connected to 128.205.32.2.
Escape character is '^]'.
Callbook v1.3  Bug reports to bowen@cs.buffalo.edu  Type 'help' for help
>> call kc6uud
Call-Sign: KC6UUD                   Class: TECHNICIAN
Real Name: DANIEL D TODD            Birthday: DEC 19, 1966
Mailing Address: 1411 WAKE FOREST 6, DAVIS, CA  95616
Valid From: MAY 7, 1991             To: MAY 7, 2001
>>

73
Clem.
---
   Clement Vaillancourt,             |    Institut de Recherche d'Hydro-Quebec
   Analyste,                         |    Varennes, P. Quebec, Canada, J3X 1S1
   Informatique scientifique         | Tel:+1 514 652 8238 Fax:+1 514 652 8309
   vaillan@ireq.hydro.qc.ca          |  Radio-amateur: VE2HQJ@VE2CRL.PQ.CAN.NA

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

Date: Thu, 20 Jan 1994 21:57:04 GMT
From: library.ucla.edu!agate!howland.reston.ans.net!cs.utexas.edu!swrinde!sgiblab!pacbell.com!unet!white!johng@network.ucsd.edu
Subject: CW Books
To: info-hams@ucsd.edu

Ok, I've gone though the 200 or so unexpired articles, as well as
the FAQ (probably not closely enough) and below is the
closest my question has come to being answered.

In article <2hebl3$2l9@news.acns.nwu.edu> rdewan@casbah.acns.nwu.edu (Rajiv Dewan) writes:
>In article <CJqtFz.61@wri.com>, Bruce Pea <pea@wri.com> wrote:
>>Can anyone recommend some good books on copying code??
>>
>>Next test date is in March here, and I want to be ready
>>to "ace" the 13wpm general class code test. I'm using
>>SuperMorse and listening to code on my radio. I remember
>
>Noting the lack of a call sign in you sig, I assume that you
>are not a ham yet.  So I will not recommend getting on the air
>and using it.  ... [delete] ...

My question is:

If I pass the 13 wpm test, do I also have to pass the 5 wpm
test? Or in other words; Can I get a General class license
by passing the written tests for Novice, Technician and
General and then pass ONLY the General CW test?

I am interested in a General class license because of the
privileges it provides but I am not that hot about learning
CW at 5 wpm, then having to bump up to 13 wpm. I've listened
to 5 and 13 wpm and they sound like two different languages!

I'm pretty confident that I can be proficient at 13-15 wpm with
plenty of practice. Any thoughts on how 'practical' this ambition is?
Am I setting myself up for 'too much' work by skipping over the
5 wpm rate?
-- 
John Gratton                               |                      johng@net.com
Hans Christian 33 "Nakia"                  |                      (415)780-5774
  The last time an informal vote on "should we split rec.boats" was taken, the
 motion was defeated 67 to 18. Before you start it again, please consider that.

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

Date: 21 Jan 1994 22:36:55 GMT
From: ucsnews!sol.ctr.columbia.edu!howland.reston.ans.net!cs.utexas.edu!geraldo.cc.utexas.edu!astro.as.utexas.edu!oo7@network.ucsd.edu
Subject: CW filters and DSP-9
To: info-hams@ucsd.edu

yee@mipg.upenn.edu (Conway Yee) asks:

>>When I look at CW filters, I see advertised bandwidths of between circa
>>250Hz to 600Hz.  What are the difference?

The 250 Hz ones have a bandwidth of 250 Hz and the 600 Hz ones have a 
bandwidth of 600 Hz.  That are[sic] the difference.  What do you mean?

Ref the DSP-9 postings, I have used mine a few times and am still not
sure that it is doing anything for me on CW.  It's cute having a 100 Hz
width filter but, as someone mentioned, when it cuts out your sidetone
you think twice about using it.  So far, I've found that the fiddling
around adjusting the receiver output for signals of different level as
well as playing with the gain on the DSP-9 is distracting when tuning
the bands.   There is a narrow range of signal strengths where the DSP
really helps.  If the signal/noise is already 10 I don't need it to be
100, and when it's 1, the DSP doesn't really help.   I need to play
with it some more, I'm sure.

It should be useful on phone, when I get around to that.  Taking out
the jammers and tuners-up on top of DX stations is useful, but it's
not saying much for the state of amateur radio if the DSP boxes are
primarily of use for removing deliberate human (or quasi-human) QRM.

As far better ops than I have said, sometimes the best filter is the
one between your ears.


Derek "up lid" Wills (AA5BT, G3NMX)
Department of Astronomy, University of Texas, 
Austin TX 78712.  (512-471-1392)
oo7@astro.as.utexas.edu 

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

Date: 21 Jan 94 18:34:27
From: ucsnews!newshub.sdsu.edu!usc!howland.reston.ans.net!vixen.cso.uiuc.edu!uwm.edu!msuinfo!netnews.upenn.edu!mipg.upenn.edu!yee@network.ucsd.edu
Subject: CW filters and DSP-9
To: info-hams@ucsd.edu

I ask a poorly phrased question:
>When I look at CW filters, I see advertised bandwidths of between circa
>250Hz to 600Hz.  What are the difference?

A poster replies:
>The 250 Hz ones have a bandwidth of 250 Hz and the 600 Hz ones have a 
>bandwidth of 600 Hz.  That are[sic] the difference.  What do you mean?

I am asking about the difference in CW performance.  Is a narrower
filter easier to copy or a wider one?


--
Medical Image Processing Group     |                  Conway Yee, N2JWQ
411 Blockley Hall                  |  EMAIL : yee@mipg.upenn.edu
418 Service Drive                  |  VOICE : 1 (215) 662-6780
Philadelphia, PA 19104-6021 (USA)  |  FAX   : 1 (215) 898-9145

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

Date: Sat, 22 Jan 1994 21:40:50 MST
From: sdd.hp.com!cs.utexas.edu!howland.reston.ans.net!sol.ctr.columbia.edu!destroyer!nntp.cs.ubc.ca!alberta!adec23!ve6mgs!usenet@network.ucsd.edu
Subject: Daily Summary of Solar Geophysical Activity for 22 January
To: info-hams@ucsd.edu

                /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\

                 DAILY SUMMARY OF SOLAR GEOPHYSICAL ACT

                                22 JANUARY, 1994

                /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\

                  (Based In-Part On SESC Observational Data)


SOLAR AND GEOPHYSICAL ACT
-----------------------------------------------------------

!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 022, 01/22/94
10.7 FLUX=113.0  90-AVG=103        SSN=102      BKI=3212 0022  BAI=005
BGND-XRAY=B2.1     FLU1=7.1E+05  FLU10=1.0E+04  PKI=3212 2122  PAI=007
  BOU-DEV=029,017,008,010,002,002,010,011   DEV-AVG=011 NT     SWF=00:000
 XRAY-MAX= C1.6   @ 0110UT    XRAY-MIN= B1.9   @ 1808UT   XRAY-AVG= B2.7
NEUTN-MAX= +002%  @ 1205UT   NEUTN-MIN= -002%  @ 2005UT  NEUTN-AVG= +0.0%
  PCA-MAX= +0.1DB @ 0745UT     PCA-MIN= -0.4DB @ 1500UT    PCA-AVG= -0.0DB
BOUTF-MAX=55348NT @ 0446UT   BOUTF-MIN=55328NT @ 1925UT  BOUTF-AVG=55341NT
GOES7-MAX=P:+000NT@ 0000UT   GOES7-MIN=N:+000NT@ 0000UT  G7-AVG=+060,+000,+000
GOES6-MAX=P:+127NT@ 1950UT   GOES6-MIN=N:-061NT@ 0601UT  G6-AVG=+081,+032,-031
 FLUXFCST=STD:110,110,110;SESC:110,110,110 BAI/PAI-FCST=005,005,005/010,010,010
    KFCST=1111 2111 0101 2111  27DAY-AP=007,005   27DAY-KP=2012 3223 1121 2211
 WARNINGS=*SWF
   ALERTS=
!!END-DATA!!

NOTE: The Effective Sunspot Number for 21 JAN 94 is not available.
      The Full Kp Indices for 21 JAN 94 are: 2o 3- 1+ 1-   1+ 2- 3- 2o 


SYNOPSIS OF ACT
--------------------

             Solar activity was low during the past 24 hours. Region
       7654 (N09W06) produced the only C-class x-ray event observed
       but has lost its delta magnetic configuration. Two new regions
       were numbered. Region 7658 (N12E16) is a simple bipolar group.
       Region 7659 (S13E47) was spotted briefly but is presently only
       plage and an arch filament system. Several unassociated Type
       III radio sweeps, and discrete radio bursts were reported. A
       large, inactive prominence is rotating over the east limb.

            Solar activity forecast:  solar activity is expected to be
       low. Region 7654 retains the potential for occasional eruptive
       flares.

            The geomagnetic field has been at mostly quiet levels at
       middle geomagnetic latitudes for the past 24 hours. Some
       periods at active levels were observed at auroral latitudes.

            Geophysical activity forecast:  the geomagnetic field is
       expected to be quiet for the next three days. Active conditions
       are possible on 26 Jan in response to disturbed solar wind
       associated with a filament disappearance on 21 Jan and an
       equatorial coronal hole which will be near central meridian
       on 23 Jan.

            Event probabilities 23 jan-25 jan

                             Class M    05/05/05
                             Class X    01/01/01
                             Proton     01/01/01
                             PCAF       Green

            Geomagnetic activity probabilities 23 jan-25 jan

                        A.  Middle Latitudes
                        Active                05/10/10
                        Minor Storm           01/05/05
                        Major-Severe Storm    01/01/01

                        B.  High Latitudes
                        Active                05/10/10
                        Minor Storm           01/05/05
                        Major-Severe Storm    01/01/01

            HF propagation conditions were normal over all regions.
       Near-normal conditions should persist over the next 72 hours.
       High latitudes may begin seeing effects of the above-mentioned
       disturbance on 25 January.  Otherwise, near-normal conditions
       are expected to continue.


COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS
========================================================

REGIONS WIT
----------------------------------------------------------
NMBR LOCATION  LO  AREA  Z   LL   NN MAG TYPE
7652  N04W23  220  0090 HSX  02  001 ALPHA
7654  N09W08  205  0610 CKI  09  032 BET
7657  N12W37  234  0080 DAO  06  012 BET
7658  N12E14  183  0010 BXO  05  005 BET
7659  S13E47  150  0010 BXO  02  002 BET
7656  S22W62  259                    PLAGE
REGIONS DUE TO RET
NMBR LAT
7647 S15   096
7646 S09   087
7645 N13   085
7649 S19   079


LISTING OF SOLAR ENERGETIC EVENTS FOR 22 JANUARY, 1994
------------------------------------------------------
A.  ENERGETIC EVENTS:
BEGIN  MAX  END  RGN   LOC   XRAY  OP 245MHZ 10CM   SWEEP
 0102 0109 0114 7654  N10W00 C1.6  SF    280
 0246 0246 0246                          110
 0633 0633 0634                          310
 1911 1919 1926 7654  N08W10 B6.2  SF    290
 1928 1928 1928                          110



POSSIBLE CORONAL MASS EJECTION EVENTS FOR 22 JANUARY, 1994
----------------------------------------------------------
 BEGIN        MAX      END     LOCATION   TYPE   SIZE  DUR  II IV
     NO EVENTS OBSERVED


INFERRED CORONAL HOLES. LOCATIONS VALID AT 22/2400Z
---------------------------------------------------
               ISOLATED HOLES AND POLAR EXT
      EAST   SOUTH  WEST   NORTH  CAR  TYPE  POL  AREA   OBSN
57   N18W17 S10W57 S10W57 N18W17  250  ISO   NEG   008 10830A
58   N20E29 S15E22 N02E07 N30E17  190  ISO   POS   016 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
------  ----  ----  ----  ----  -- ------ ------  --------- --------- ---------
21 Jan: 0324  0328  0332  B4.5                                         
        0758  0802  0809  B3.5                                         
        0816  0821  0838        SF  7654  N07E17                       
        1019  1023  1025  B6.6                                         
        1140  1146  1155  B4.5                                         
        1610  1613  1616  B4.0  SF  7654  N08E12                       
        2059  2103  2106  B4.6  SF  7654  N07E08                       
        2308  2330  2340  B7.8  SF  7654  N06E07                       


REGION FLARE STATISTICS FOR THE PREVIOUS UTC DAY
------------------------------------------------

                C   M   X     S   1   2   3   4   Total   (%)
               --  --  --    --  --  --  --  --    ---  ------
  Region 7654:  0   0   0     4   0   0   0   0    004  (50.0)
Uncorrellated: 0   0   0     0   0   0   0   0    004  (50.0)

 Total Events: 008 optical and x-ray.


EVENTS WIT
----------------------------------------------------------------

 Date   Begin  Max   End  Xray  Op Region  Locn    Sweeps/Optical Observations
------  ----  ----  ----  ----  -- ------ ------   ---------------------------
21 Jan: 0758  0802  0809  B3.5                     III
        2308  2330  2340  B7.8  SF  7654  N06E07   Continuum

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: 24 Jan 94 03:38:02 GMT
From: news-mail-gateway@ucsd.edu
Subject: International Callsign Server
To: info-hams@ucsd.edu

Does anyone know of a server that can be TELNET'd that has a
INTERNATIONAL callsign data base or CD-ROM on it?  Whats
the address?  Buffalo.edu does not support international
that I know of.


/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\
!        JD DELANCY              | Lizzie Borden took an axe        !
!  VM:  1-800-862-4511 Box 9276  | And plunged it deep in to the    !
!  VOICE: 301-763-4943 or 3474   | VAX..                            !
!                                | Don't you just hate people who   !
!  Email:   k1zat@bah.com        | do all the things YOU wanted to  !
!  AX25: K1ZAT@K3HKI.#SOMD.MD.NA | do ??                            !
/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\/*\

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

Date: 21 Jan 94 17:16:54
From: ucsnews!sol.ctr.columbia.edu!howland.reston.ans.net!agate!msuinfo!netnews.upenn.edu!mipg.upenn.edu!yee@network.ucsd.edu
Subject: The differences in CW filter performance
To: info-hams@ucsd.edu

When I look at CW filters, I see advertised bandwidths of between circa
250Hz to 600Hz.  What are the difference?

--
Medical Image Processing Group     |                  Conway Yee, N2JWQ
411 Blockley Hall                  |  EMAIL : yee@mipg.upenn.edu
418 Service Drive                  |  VOICE : 1 (215) 662-6780
Philadelphia, PA 19104-6021 (USA)  |  FAX   : 1 (215) 898-9145

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

Date: 23 Jan 1994 08:28:40 +0200
From: vixen.cso.uiuc.edu!howland.reston.ans.net!xlink.net!zib-berlin.de!netmbx.de!Germany.EU.net!EU.net!sunic!trane.uninett.no!news.eunet.no!nuug!news.eunet.fi!elvis.clinet.fi!@sdd.hp.com
To: info-hams@ucsd.edu

References <1994Jan11.150658.25191@ke4zv.atl.ga.us>, <940118.46856.LEEVANKOTEN@delphi.com>, <2hihn7$1vs@news.u.washington.edu>.unin
Subject : Re: BRAIN CANCER, LEUKEMIA FROM HAM RADIO

Man has a high risk to get at least brain cancer if listening too
much 2m repeater OH2RAA in Helsinki.
-- 
Jukka Salomaa     jukka@clinet.fi     OH2BUA
phone +358 400 315 444  puhelin 9400 315 444

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

Date: 22 Jan 1994 18:26:34 +0200
From: library.ucla.edu!agate!howland.reston.ans.net!pipex!sunic!news.funet.fi!butler.cc.tut.fi!lehtori.cc.tut.fi!not-for-mail@network.ucsd.edu
To: info-hams@ucsd.edu

References <2hple7$ti@geraldo.cc.utexas.edu>, <YEE.94Jan21183427@mipgsun.mipg.upenn.edu>, <2hpqci$m30@safety.ics.uci.edu>ht
Subject : Re: CW filters and DSP-9



Clark Savage Turner (turner@safety.ics.uci.edu) wrote:

> Most IF filters don't have much ring, though some, many audio filters
> (except DSP I understand) can ring pretty badly.

What should the audio filter frequency (and phase response) look like
to avoid ringing. A high-Q single stage bandpass sounds horrible, but
how does a filter with flat passband (eg. Butterworth or elliptic)
sound like or is it really required to use Bessel-response in order
to get rid of the hollow sound produced by noise peaks.

                Paul OH3LWR
                

--------------------------------------------------------------------
Phone   : +358-31-213 3657                                 
X.400   : G=Paul S=Keinanen O=Elisa-Tampere A=ELISA C=FI 
Internet: Paul.Keinanen@Telebox.tele.fi
Telex   : 58-100 1825 (ATTN: Keinanen Paul)            
Mail    : Hameenpuisto 42 A 26
          FIN-33200 TAMPERE
          FINLAND

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

Date: 22 Jan 1994 18:25:41 +0200
From: library.ucla.edu!agate!howland.reston.ans.net!pipex!sunic!news.funet.fi!butler.cc.tut.fi!lehtori.cc.tut.fi!not-for-mail@network.ucsd.edu
To: info-hams@ucsd.edu

References <2hple7$ti@geraldo.cc.utexas.edu>, <YEE.94Jan21183427@mipgsun.mipg.upenn.edu>, <2hpqci$m30@safety.ics.uci.edu>ht
Subject : Re: CW filters and DSP-9


Clark Savage Turner (turner@safety.ics.uci.edu) wrote:

> In <YEE.94Jan21183427@mipgsun.mipg.upenn.edu> yee@mipg.upenn.edu 
> (Conway Yee) writes:

> >I am asking about the difference in CW performance.  Is a narrower
> >filter easier to copy or a wider one?

> This is a matter of personal taste for many of us.  

[deleted]

> The filter can do two things for you :
>
> 1.  Eliminate QRM nearby
> 2.  Quiet down the background noise.
>
> Reference number 2, some filters don't do so well at this, 

The filter bandwidth (which is usually defined as the bandwidth between
the points where the frequency is -6 dB down from the maximum in the pass 
band) is not the only figure-of-merrit to look for. Equally important is 
the shape of the frequency response above and below the quoted bandwidth.
This is usually specified with the -60 dB bandwidth and it indicates how
much background noise will get through. 

There are 250 Hz (at -6 dB) filters with a 1.2 kHz -60 dB bandwidth
and there are 500 Hz filters with a 800 Hz -60 dB bandwidth, so
look carefully at the specifications. Despite broader passband, the latter
filter is more effective to quiet down background noise and interfering
signals a few hundred Hertz or more above or below the passband.

Some manufacturers specify the passband bandwidth and the frequency
offset from the center of the passband where the frequency response is
-60 dB down, in the previous example +/- 600 Hz resp. +/- 400 Hz.
Some even omit the +/- signs so that the figures look better. You
can easily get the impresion that (+/-) 600 Hz is better than 800 Hz
(total) bandwidth, so be carefull.

Instead of the -60 dB bandwidth, sometimes the shape factor is given,
which is simply the ratio of the -60 dB bandwidth to the -6 dB bandwith.
The shape factor for the first example is 4.8 and 1.6 for the latter.

In some cases the shape factor is given at a smaller attenuation e.g.
50 dB/6 dB to get smaller (and better) figures.

Thus, it is very hard to select filters solely on the basis of passband
bandwidth.

As Clark pointed out in the begginning it is also a matter of personal 
taste. 

                Paul OH3LWR
                

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

Date: 21 Jan 1994 17:21:00 GMT
From: ucsnews!sol.ctr.columbia.edu!howland.reston.ans.net!agate!linus!linus.mitre.org!mwvm.mitre.org!m14494@network.ucsd.edu
To: info-hams@ucsd.edu

References <2hk4tpINN125@abyss.West.Sun.COM>, <CJwDLy.4wz@news.direct.net>, <2hkd5iINN15h@abyss.West.Sun.COM>
Subject : Re: Ramsey FX Transceivers

Dana Myers writes:
> The difference is that the IC24AT was factory built and then adjusted
> by the factory to specified tolerances.

I don't know about Icom specifically, but this is generally
not true of consumer electronics. The published specs for
most electronics represent an average based on samples
taken from the production run. The statement at the end of
the specs that says "Specifications subject to change without
notice" really means "Your radio may not do this well". Only 
a very few manufacturers offer "guarenteed specs", in which
each and every unit is guarenteed to meet the spec. When I
bought a stereo receiver a while back, I went with Tandberg 
because unlike almost every other manfacturer, they 
guarentee their specs. Check the spec sheet for the radio in
question; if it doesn't say they're guarenteed, they aren't.

*****************************
* These are my opinions only*
*****************************

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End of Info-Hams Digest V94 #69
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