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[jamsat-news:634] ANS-250 WEEKLY BULLETINS


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SB SAT @ AMSAT  $ANS-250.01
PHASE 3D UPDATE

HR AMSAT NEWS SERVICE BULLETIN 250.01 FROM AMSAT HQ
SILVER SPRING, MD, SEPTEMBER 07,1997
TO ALL RADIO AMATEURS BT
BID: $ANS-250.01

It was announced in ANS Bulletin 208.01 of July 27, 1997 that, due to the
necessity of performing a number of significant structural modifications to
the Phase 3D spaceframe made necessary by a late change in ESA launch
environment specifications, the schedule for the launch of Ariane 502 and
the Phase 3D schedule were no longer compatible. Unfortunately, that
situation has not changed. As a result, ESA has concluded that Phase 3D
would not be able to fly on that mission.

This announcement prompted several derogatory comments regarding ESA and
its action to be posted to AMSAT-NA's Internet open mail service, AMSAT-BB.
It must be emphasized  that such comments do not represent the opinions of
AMSAT-NA or any other AMSAT organization. More important, they may be
harmful to on-going efforts to identify another launch for Phase 3D.

It should be remembered, and appreciated, that ESA has been very supportive
of AMSAT for almost twenty years.  The first Phase 3 satellite was a
passenger on an Ariane vehicle which, unfortunately, ended in a launch
failure in 1980.  ESA made amends for this loss by launching AO-10 three
years later.  This was followed by AO-13 in 1988, the four Microsats and
two UoSats in 1990, and later, KO-23, KO-25, IO-26 and AO-27.  All of these
satellites were launched  by ESA on Ariane vehicles. So, it is clear
that, since the early 80s,  the European Space Agency has been responsible
for the launch of ALL the long life amateur spacecraft, other than those
orbited by the Russians and the Japanese.

There is no reason to believe that ESA's support for AMSAT projects has
waned. The decision made with respect to Phase 3D is apparently one of
schedule incompatibility only. It should be clear to everyone that it is
vital to ESA that the Ariane 502 flight goes well; and that it is launched
in accordance with the established schedule, if at all possible. Needless
to say, it is also in AMSAT's best interest that it is a great success,
even without Phase 3D aboard.

A Phase 3D Program Board meeting was held at the Orlando Phase 3D
Integration Lab Saturday August 30, during which similar sentiments were
expressed. Participants in that meeting were AMSAT-DL President and Phase
3D Project Leader Dr. Karl Meinzer DJ4ZC, Werner Haas DJ5KQ AMSAT-DL Vice
President, Peter Guelzow, DB2OS, representing the Command Station Team, Ron
Broadbent, G3AAJ, AMSAT-UK Secretary, Joel Harrison, W5ZN, 
representing ARRL, Keith Baker KB1SF AMSAT-NA Executive Vice President and
Bill Tynan W3XO AMSAT-NA President.  The Program Board is the body which
will establish broad policies with respect to the Operation of Phase 3D,
once it is safely in orbit and checked out. In addition to reviewing the
launch situation, the meeting dealt with mechanisms for communicating board
recommendations to the Command Station Team and the current status of the
spacecraft. It was noted that the structural modifications, already
mentioned, have had a significant impact on the schedule, just as they were
expected to.  For example, electronic modules have had to be installed and
un-installed several times in order to conduct  both electronic testing and
perform the drilling and riveting necessary to complete the structural
modifications.. Not surprisingly, this process has been quite time
consuming.  Nevertheless, the Board was informed that the structural work
should be completed soon. In addition to the schedule slippage the
structural modifications have caused, it has been estimated that they have
cost about $25,000 over and above expenses previously contemplated.

Other recent events at the Orlando facility involved a two week visit by a
contingent of folks from Germany, Belgium, the Czech Republic, Slovenia and
Japan to accomplish much of the electronic integration work. Just prior to
that, the RUDAK team were there to install and check out that interesting
and important sub-system. 

The Program Board issued a statement saying that it is imperative that all
of us do everything we can to promote the successful launch of Phase 3D,
particularly being  especially careful of what we say on public forums such
as AMSAT-BB or in letters to the editors of various magazines. It was 
emphasized that all of us should avoid doing anything that could possibly
hinder Phase 3D Project Leader and AMSAT-DL President Karl Meinzer 
DJ4ZC in his continuing negotiations with ESA representatives. 

Keep tuned to ANS for further information.

/EX

SB SAT @ AMSAT  $ANS-250.02
MIREX 70 CM PACKET PT. 1

HR AMSAT NEWS SERVICE BULLETIN 250.02 FROM AMSAT HQ
SILVER SPRING, MD, SEPTEMBER 07,1997
TO ALL RADIO AMATEURS BT
BID: $ANS-250.02

MIR International Amateur Radio Experiment (MIREX) will be conducting a
three (3) week 70 cm experiment with the MIR PMS station. The PMS station
will be switched from the 2-meter band to the 70cm band on 437.650 FM
Simplex world wide.

Information they expect to gain from the three week experiment:
1.Is the 70cm  band  interfered with by the existing commercial VHF
equipment.
2.How many stations around the world have access to 70 cm FM
capabilities?
3.Does the 70 cm MIR operations cause any interference to any of the
equipment on MIR?
4.Can simple ground stations compensate for 70 cm Doppler and work MIR
on Voice?
5.Can simple ground stations compensate for 70 cm Doppler and work MIR
on Packet?

MIREX will be running  the test from September 6, until September 28 1997
world wide. After the completion of the test, they will switch the MIR PMS
frequency back to the current 2-meter frequency on September 29th.

Interference from MIR's VHF Commercial communications Links:
In 1993 the MIREX team began to hear there were problems with 2-meter
packet, when MIR was transmitting on their commercial channel 143.625. The
rumors  indicated  the  2-meter station on 145.550 would become deaf. The
information that MIREX received about this problem was very limited, and
the problems only happened over Europe. They did not have problems with
143.625 over the USA and were not able to analyze the problem until 1996.
Then NASA began to install remote communications links with MIR in 1996.
Now MIR was active on 143.625 as it flew across the USA. More Ground links
were being added world wide. Soon many populated areas of the world, would
have remote MIR VHF ground links. MIREX began testing with the MIR crews
late 1996. It was confirmed that when the commercial link was active on
143.625, it was impossible to work the MIR space station on any frequency
below 145.900.  The frequency 145.940, was barley usable when the ground
station was transmitting more than 3000 watts of ERP. Theses uplink power
levels are just not realistic, a better solution needed to be found. MIREX
is  working on a filter project, that if approved, will solve the comm link
interference  problem.  The MIREX filter project is still waiting extensive
paper  work approvals, etc. No date has been confirmed for delivery of the
filter.

MIREX still encourages stations to use as little power as possible.
Another possible solution is to try to use the 70 cm equipment already on
board MIR. The existing external  antenna is a dual band 2-meter/70
centimeter antenna. The existing radio, a Kenwood TM-733 (European
version) supports both  2-meters and  the  435-437 MHz portion of the
satellite sub band. MIREX began testing of the 70 cm operations for voice
and  packet during the spring of 1997. The equipment appears stable enough
to allow  access  to  the  general  public. They originally had planned to
operate both bands simultaneously, but they have run into equipment and 
power limitations. So the test is being scaled back to test just the 70cm
band for a limited time.

For the  duration of the 70cm test (up to 3 weeks) the 2-meter operations
will be turned off. After the 70cm test is completed the
frequency will be moved back to the 2-meter band. MIREX believes that
2-meter mono-band operations should always be the primary system because it
allows the greatest access to the most  users. Other modes should be
experimented with, and if successful additional equipment could be 
installed, just as long as you never permanently turn off 2-meter mono
band support.

[ANS thanks Miles Mann, WF1F, and Dave Larsen, N6CO, 
MIREX President for this information.]

/EX

SB SAT @ AMSAT  $ANS-250.03
MIREX 70 CM PACKET PT. 2

HR AMSAT NEWS SERVICE BULLETIN 250.03 FROM AMSAT HQ
SILVER SPRING, MD, SEPTEMBER 07,1997
TO ALL RADIO AMATEURS BT
BID: $ANS-250.03

The ERP requirements on 70 cm are a little higher for this band.  
Stations should try for an ERP rating of greater than 25 watts. 
Doppler will b  biggest challenge. The Doppler on 70 cm is + and - 10,000
cycles.  Most radios made today can only make tuning steps in 5k channel
steps. To  work MIR on voice, a station  will  need to get within 
3 KHz of the receiver frequency on MIR. To work MIR on the packet  
frequency error must be less than 2.0 KHz. A 5 KHz radio, is not 
recommend for running 70 cm packet during this test.

The Doppler change is not linear. What this means, is that during the
first 3 minutes of the pass the Doppler will be approximately 10-9k KHz 
and will drift 1 KHz in three minutes. However during pass minutes 
4 - 6, the Doppler will swing 14 KHz in 3 minutes.
 
A radio which can step in 2 KHz  or less can program in a set of 11
channels. MIREX  has  tested  this  configuration for both voice and packet
with good results. Use channel 1 at the beginning of the pass. Then 
monitor the FM signal meter for discriminator center tuning on the radio 
and changes channels to keep the FM discriminator center tuning meter 
centered.

On 70cm Both the TX and RX MUST change!

Program in these 11 channels in this order.
TX channel          RX channel
1    437.640   437.660   +10
2    437.642   437.658   +8
3    437.644   437.656   +6
4    437.646   437.654   +4
5    437.648   437.652   +2
6    437.650   437.650   0
7    437.652   437.648   -2
8    437.654   437.646   -4
9    437.656   437.644   -6
10   437.658   437.642   -8
11   437.660   437.640   -10
 
Dave Larsen N6CO and Mile Mann WF1F have been conducting may packet upload
and down load tests on 70cm with MIR. If a station can compensate for 
Doppler correctly the reliability should be equal to 2-meter packet.  
The MIR receiver seems to work better if the uplink channel is a little  
lower than or equal to the calculated RX channel. Going above the  
calculated  RX  channel  may  cause  packet performance to drop off more 
quickly. Based the testing using  the listed 2 KHz channels steps, It 
has determined that a mobile radio can not work 70cm packet with any 
amount of reliability and should be avoided. 

[ANS thanks Miles Mann, WF1F, and Dave Larsen, N6CO, 
MIREX President for this information.]

/EX

SB SAT @ AMSAT  $ANS-250.04
SPECIAL EVENT STATION PLANNED

HR AMSAT NEWS SERVICE BULLETIN 250.04 FROM AMSAT HQ
SILVER SPRING, MD, SEPTEMBER 07,1997
TO ALL RADIO AMATEURS BT
BID: $ANS-250.04

The Virginia Air & Space Center, (VASC is located in Hampton, VA, USA),
Amateur Radio Group, Inc., will operate KE4ZXW as a Special Events
Station on September 27-28, 1997. The VASC Amateur Radio Group is
celebrating two years of uninterrupted 9600 baud automatic satellite
operation at the VASC Amateur radio exhibit. The Special Event Station
will operate via KO-23 or KO-25, on both days, from 0000 to 2200 UTC. 
We will also operate HF from 1500 to 2200 UTC on 7.265 MHz at the top of
the hour, and 14.265 MHz at thirty minutes past each hour. An
Anniversary QSL card will be issued to those sending a QSL and a SASE
to:
Ed Brummer, W4RTZ, 108 Oyster Cove Road, Yorktown, VA 23692. (USA).

[ANS thanks  Wally Carter, K4OGT/KE4ZXW, Control Operator
for this news item.]

/EX

SB SAT @ AMSAT  $ANS-250.05
ANNUAL MEETING IN TORONTO

HR AMSAT NEWS SERVICE BULLETIN 250.05 FROM AMSAT HQ
SILVER SPRING, MD, SEPTEMBER 07,1997
TO ALL RADIO AMATEURS BT
BID: $ANS-250.05

Just a reminder - if attending the Annual meeting in Toronto,
the registration fee rises to $30.00 US after Monday September 15 1997.
The organizing committee also need to know how many people plan to
attend the banquet, several days before the meeting, so they will be
unable to provide banquet tickets at the registration desk ( or after
Wednesday October 15).

The block of hotel rooms will be available until September 26.
however they are going fast! The committee have had to increase 
the number of rooms already! For visitors to Canada, some of the local 
Taxes are re-fundable, keep receipts and pickup sales tax pamphlets,
available at the border and in airports, there will be some in the hotel,
but maybe not enough for all!.

U.S. residents returning home are allowed $400 U.S. duty free each
person per month, at last count! Please check and confirm this.

For the winner(s) of major prize(s) the committee will try and have a 
certificate available to trade in if you live outside of Canada.

For details of the 3 day agenda see  www.amsat.org

The committee looks forward to seeing you in Toronto on Friday October
17, Saturday October 18 and Sunday October 19.

Just a final reminder - if coming by Air book to Toronto Canada
(YYZ) not the Ontario airport which is in California.

[ANS thanks Robin Haighton, VE3FRH, for this news.]

/EX

SB SAT @ AMSAT  $ANS-250.06
WEEKLY SATELLITE REPORT PT 1

HR AMSAT NEWS SERVICE BULLETIN 250.06 FROM AMSAT HQ
SILVER SPRING, MD, SEPTEMBER 07,1997
TO ALL RADIO AMATEURS BT
BID: $ANS-250.06

MIR:

MIREX will be running  the test from September 6, until September 28 1997
world wide. After the completion of the test, they will switch the MIR PMS
frequency back to the current 2-meter frequency on September 29th.
See ANS Bulletin ANS-250.02 for more information.

Tom Keller, KB0MDQ, of Lakeville, MN reports he had both
a voice QSO with Mike Foale, KB5UAC, and on a later pass connected to
the MIR packet station on the test frequency of
437.650 MHz.


SAFEX, MIR 70 cm Repeater
(Uplink 435.750 MHz FM, Downlink 437.950 MHz FM,
Subaudible tone 141.3 Hz)
Not operational at this time.

RS-10
(Uplink 145.865-145.905 MHz CW/SSB, Downlink 29.36-29.4 MHz CW/SSB)
RS-10 Still silent.

RS-12
(Uplink 21.21-21.25 MHz CW/SSB, Downlink 29.41-29.45 MHz or
145.91-145.95 MHz CW/SSB)
Operational.

RS-15
(Uplink 145.858-145.898 MHz CW/SSB, Downlink 29.354-29.394 MHz CW/SSB)
Operational.
(Hint: If SSB doesn't work for you, try CW. CW is very easy
to hear on the downlink!)

RS-16
IW9ELR,  heard the 435.504 MHz beacon-telemetry of
RS16.
Transponder information on RS-16.
Uplink = 145.915 - 145.948 MHz
Downlink = 29.415 - 29.448 MHz
Beacons = 29.408 , 29.451 MHz
Pwr 29 MHz Down = 1.2 W /4 W

Beacon 1 = 435.504 MHz
Beacon 2 = 435.548 MHz
Pwr 435 MHz Beacons = 1.6 W

FO-20
(Uplink 145.9-146.0 MHz CW/LSB, Downlink 435.8-435.9
MHz CW/USB)
Operational. FO-20  in mode JA continuously.
[ANS thanks Kazu Sakamoto, JJ1WTK, for this report.]

KO-23
(Uplink 145.85, 145.9 MHz FM, Downlink 435.175 MHz FM,
9600 Baud FSK.)
KO-23 operating normally.

KO-25
(Uplink 145.980 MHz FM, Downlink 436.5 MHz FM,
9600 Baud FSK.)
KO-25 operating normally.
[ANS thanks Jim Weisenberger, AA7KC, for his reports on
KO-25 and KO-23.]

AO-27
(Uplink 145.85 MHz FM, Downlink:
436.792 MHz FM (As of April 1, 1997)
Operating normally.
This information can be found at www.umbra.com
AO-27 TEPR (Timed Eclipse Power Regulation) States are as follows
As of July 6, 1997
  TEPR STATE      Time      TX Status
----------------------------------------
       1           n/a         OFF
       2           n/a         OFF
       3           ---         OFF

       4           21          OFF
       5           17          ON at Med Power
       6           ---         OFF

The TEPR States are defined as follows:

Tepr 1, Started when the satellite Enters the Eclipse
Tepr 2, Started at (tepr 1 time) after the satellite enters the eclipse
Tepr 3, Started at (tepr 1 time) + (tepr 2 time).

Tepr 4, Started when the satellite enters the Sun
Tepr 5, Started at (tepr 4 time) after the satellite enters the Sun
Tepr 6, Started at (tepr 4) + (tepr 5).

It should noted that TEPR states 1,2 and 3 happen during the Night Time
passes and TEPR states 4,5 and 6 happen during the Day time passes.
These occur during EVERY pass, not just over the U.S.A.

The times assigned to the TEPR states are chosen for the health of the
satellite over operation convenience.  Therefore, during parts of the
year the satellite will turn on late or turn off early as seen by ground
stations.

Users are asked not to transmit on 145.85 MHz if they do not hear the
satellite's downlink so as to avoid possible interference to other
satellite uplinks and downlinks on adjacent frequencies.
[ANS thanks Michael Wyrick, N4USI, AO-27 Control-op, for this update.]

FO-29
Voice/CW Mode JA
(Uplink 145.9-146.0 MHz CW/LSB, Downlink 435.8-435.9 MHz CW/USB)
Digital Mode JD
(Uplink 145.85, 145.87, 145.910 MHz FM, Downlink 435.910 MHz FM 9600
baud BPSK)
Operational.
The latest FO-29 Schedule.
Sept  5 (Fri)    01:18z  JA
Sept 12 (Fri)    00:13z  JD1200
Sept 19 (Fri)    00:51z  JD9600
Sept 26 (Fri)    08:09z  JA
[ANS thanks Kazu Sakamoto, JJ1WTK, for this report.]

/EX

SB SAT @ AMSAT  $ANS-250.07
WEEKLY SATELLITE REPORT PT 2

HR AMSAT NEWS SERVICE BULLETIN 250.07 FROM AMSAT HQ
SILVER SPRING, MD,SEPTEMBER 07,1997
TO ALL RADIO AMATEURS BT
BID: $ANS-250.07

AO-10
(Uplink 435.030-435.18 MHz CW/LSB, Downlink 145.975-145.825 MHz
CW/USB)
Operational. Very active over North America, with good downlink
signals

OSCAR-11
(Downlink 145.825 MHz. FM, 1200 Baud PSK. Beacon 2401.500 MHz..)
Operating normally.  


A single WOD survey of channels 10, 20, 30,  40  (+Y,  -X,  +X  array

The operating schedule is unchanged.

        ASCII status (210 seconds)
        ASCII bulletin  (60 seconds)
        BINARY SEU (30 seconds)
        ASCII TLM (90 seconds)
        ASCII WOD (120 seconds)
        ASCII bulletin (60 seconds)
        BINARY ENG (30 seconds)

There are also additional status blocks after each bulletin is
transmitted, and between ASCII TLM and WOD.

The mode-S beacon is ON, transmitting an unmodulated carrier, but
telemetry indicates that it has partially failed, and delivering half
power. Any reports of reception on 2401 MHz. would be most welcome.
Please e-mail g3cwv@amsat.org.

The 435.025 MHz. beacon is normally OFF. However it can sometimes be
heard when the satellite is being commanded by ground control, i.e.
within range of Guildford, UK. When the 435 beacon is transmitting,
the 145 MHz beacon is normally  OFF.  he data transmitted is mainly
binary.

OSCAR-11 users are welcome to visit Clive Wallis' web site. It
contains some software for capturing data, and decoding ASCII  telemetry 
and WOD. There is an archive of raw data (mainly WOD) for analysis, which 
is continually being expanded, as new data is captured. The URL is -
http://www.users.zetnet.co.uk/clivew/

[ANS thanks  Clive Wallis, G3CWV, for this information.]

AMSAT-OSCAR-16 (PACSAT)
(Uplink 145.9, 145.92, 145.94, 145.86 MHz FM, 1200 bps Manchester FSK
Downlink 437.0513 MHz SSB, 1200 bps RC-BPSK 1200 Baud PSK.
Beacon 2401.1428 MHz.)
Operating normally.

Graphic information about WOD/Telemetry values can be found at:
http://www.arrakis.es/~ea1bcu/wod.htm

[ANS thanks Miguel A. Menendez, EA1BCU, for this report.]

DO-17(DOVE)
( Downlink 145.825 MHz FM, 1200 Baud AFSK.
Beacon 2401.220 MHz.)
No report available.

WEBERSAT (WO-18)
(Downlink 437.104 MHz SSB, 1200 Baud PSK AX.25.)
No report available.

LUSAT-OSCAR-19
(Uplink 1200 bps Manchester FSK Uplinks:
145.84, 145.86, 145.88, 145.9 MHz FM, Downlink 437.125  MHz SSB,
1200 bps RC-BPSK.)
Operating normally.

<To add 6,83 minutes to the clock of the satellite>Graphic and general 
information about Telemetry values can be found at:
http://www.arrakis.es/~ea1bcu/lo19.htm
[ANS thanks Miguel A. Menendez, EA1BCU, for this report.]

UO-22:
(Uplink: 145.9 or 145.975 MHz FM. Downlink 435.120 MHz FM
9600 Baud FSK.)
UO-22 is operating normally.
Chris Jackson, G7UPN / ZL2TPO, has reloaded the Store and Forward
communications task on the UO-22 On-Board Computer. This task includes
incremental checksums which should make uploading slightly faster.
In the old task, once an upload was complete, the spacecraft had to
perform the checksum on the complete file. Depending on the file
length, this could take quite a long time. With the new task, the
checksum is computed on the fly - while the data is actually being 
uploaded. Thus there is no need to recompute it at the end of the 
transfer and this checksum delay is then removed.

However, all files that were started before Chris Jackson, G7UPN /
ZL2TPO, loaded the task around 1000 UTC on the 19th will receive a corrupt 
body checksum error when the upload is completed. If the file is uploaded 
again, it should be accepted. If trying to upload a large file that was
started before the above time, then start again.

If anyone gets persistent body checksum errors while uploading files to
UO-22 would they please let Chris Jackson know as soon as possible

[ANS thanks Chris Jackson, G7UPN / ZL2TPO,
Groundstation and Operations Manager, for this report.]

IO-26 ( ITAMSAT)
Uplink 145.875, 145.9, 145.925, 145.95 MHz FM, Downlink 435.822 MHz SSB,
1200 Baud PSK.)
The satellite is in good shape.
[ANS thanks Daniele Piercarlo, IK2XRO, ITMSAT Command Station for this
report.]

[Please send your Satellite or News reports to ANS Editor B.J. Arts,
WT0N, via e-mail, at bjarts@the-bridge.net or to wt0n@amsat.org]

/EX

 


BJ Arts  
Amateur callsign: WT0N  
ARMY MARS callsign: AAR5EL
Grid Square EN-37mk
Hibbing, Minnesota. U.S.A. 
e-mail bjarts@the-bridge.net or wt0n@amsat.org
Amsat News Service Bulletin Editor