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Mir,Sputnik,ISS Status Nov 20, 1998

Mir Amateur Radio Status:  Nov 20, 1998

Zarya - Control Module has Launched

by Miles Mann WF1F,
MAREX-NA (Manned Amateur Radio Experiment, North American Division)

The U.S.-funded and Russian-built Zarya, "Sunrise" in English, was launched
today on
November 20, 1998.  This is the first module of the International Space
Station (Alpha).
The Zarya module will be remotely controlled by Mission control in Russia.
For more information on the specific modules and the launching sequence of
the modules,
check out the NASA web pages about ISS.

ISS Amateur Radio Status:
MAREX-NA is actively working with Energia and other organizations to design
and deliver
useful and educational Amateur Radio projects for ISS.
The tentative plan is to have a manned crew arrive on ISS to live on ISS
around January - March in the year 2000.  Amateur Radio 2-meter Packet
operations should
begin a few months after the crews arrive.
A space walk (EVA) will be required to install the Amateur Radio antennas
to the bulk-head feed-through antenna connector ports.  There will be 4
antenna ports located on the Russian Service module and two more ports on
the Universal Docking Adapter.
Many more Amateur Radio projects are currently being reviewed.  With 6
separate antenna ports, it will be possible to run several different
educational amateur radio projects at the same time.

SPOUTNIK 41 or RS-18
Sputnik is on the Air.
Sputnik was launched on the evening of November 10, 1998 from the Russian
Station Mir.  The new Sputnik can be heard on 145.815 (Adjust for Doppler).
Listen closely and you will hear the three messages, repeated in three
different languages, French, English and Russian.

Listening for Sputnik:
Sputnik is operating on the frequency 145.815.
Earlier I passed on a different frequency, but after analyzing today

Sputnik pass and compensating for Doppler, the frequency appears to be on
145.815 FM.  Of course
the frequency will appear to drift due to normal Doppler effects.

Because of Doppler shift, the signal may appear anywhere between 145.811 -
(I rounded a little).  When Sputnik first comes in range for its 10 minute
pass, the initial frequency plus
Doppler will be approximately 145.818 (145.815 TX freq., plus 3.5k Doppler
When Sputnik is directly over head, the frequency will be approximately
Then as Sputnik passes away and nears the horizon, the frequency will be
approximately 145.812 (145.815, minus Doppler 3.5k).
If you have an FM receiver which can tune only in 5k Channels, try to
listen for Sputnik on 145.820 at the beginning of the pass, then step down
to 145.815 and 145.810 towards the end of the pass. Sputnik can be heard
with most receivers, FM, CW or SSB.

For more information about this project, please check out the Amsat-France
Web page and
follow the links to the Sputnik

The 200 mw beacon can be heard in either FM, CW or SSB modes.
Give it a try and if you hear the Beep Beep Beep  or Recorded voices of the
satellite, you can send away for a special Short Wave Listener SQL card.

Please use one of the following QSL managers and follow the directions for
that Manager
and included the following information:
Return Name and Address, country
Date and time you heard RS-18 (use the UTC time and date)
Signal report (Best guess)
Radio Station and Antenna (optional)

This address is for the SWL cards for the Sputnik-41 Amsat-France project.

QSL manager RS18
14 bis rue des Gourlis
92 500 Rueil-Malmaison

Send an ETSA + 1 IRC.
Self Address Envelope, plus an IRC coupon


All Mir contacts, including SWL, Two-way voice or Packet connections
and including the new Sputnik Satellite RS-18 / Sputnik 41

Envelopes should be well sealed and do not include cash.
Send a SAE (Self Addressed Envelope ) and one or two IRC coupons
(which can be purchased at major US post offices).
Do not make any notes on the out side of the envelope with Amateur Radio
Call signs visible.

QSL Information for SWL (Short Wave Listener)
Sergej Samburov
PO Box 73
Korolev-10 City
Moscow Area, 141070, Russia


For Two-way contacts with Mir ONLY.  Just for the call sign R0MIR and
No SWL (Short Wave Listener) cards will be issued at this address.

Dr. Dave Larsen - N6CO/K6MIR
PO Box 311
Pine Grove, California

Please include a SASE (Business Size Envelope) and two IRCís  for
international. If you are sending an IRC, Please make sure it is dated
1998, as the post office won't accept IRC's dated over 1 year old.
Make sure the cancel stamp is in the right place on the IRC.
"Green Stamps" (USA ONLY) are appreciated for covering additional costs.

Note: Dave Larsen MIREX / N6CO is not handling SWL cards for Sputnik,
please use the other addresses


Mir Crew Members:
The current crew consists of:

Current Crew
SOYUZ TM-28 arrived at Mir on August 16. Mir Soyuz TM-28 crew consisted of
Sergei Avdeyev, Gennadiy Padalko and Yuri Baturin.  (Sergei and Gennadiy
both received training on the MAREX-NA SSTV system in Star City).

Web Page information:
For information about the MAREX-NA SSTV project, check the web page at:


For general information about some of the Mir Projects, check the web page

     http://www.ik1sld.org/mirex.htm  OR

Tracking Mir, Sputnik and Zarya

The best way to track satellites is to get access to a good satellite
tracking program.  There are numerous programs on the market, both for sale
and share ware.

The orbit of Mir is constantly changing a little each week.  If you want to
know exactly where Mir is located, you should be updating you tracking data
Kep files weekly.
The best place for current Kep data is at the CelesTrak web page

     1 25533U 98062C   98323.18888093  .00127001  00000-0  89557-3 0   273
     2 25533  51.6641 338.6711 0008429 359.0778   1.0193 15.73122399  1236
     1 16609U 86017A   98323.53720729  .00014305  00000-0  11568-3 0  9777
     2 16609  51.6600 336.9641 0007934 351.0257 147.2211 15.71085548728425
     1 25544U 98067A   98324.45674522 -.00043259  11566-4 -18040-4 0    32
     2 25544  51.5914 167.4317 0125858  91.3429 269.4598 16.05134416    30

Copyright 1998 Miles Mann, All Rights Reserved.  This document may be
freely distributed via the following means - Email (including listservers),
Usenet, and WorldWideWeb.  It may not be reproduced for profit including,
but not limited to, CD ROMs, books, and/or other commercial outlets without
prior written consent from the author.

Miles WF1F