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Hams in Space!

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Number 12 on your FHdbICk n rc!<br />

<strong>Hams</strong> <strong>in</strong> <strong>Space</strong>!<br />

SAREX II, the nextgeneration.<br />

by Philip Chien<br />

A<br />

II :4 1a.m. on December 2, the night sky<br />

lit up over Florida with a spectacular<br />

display of flame and smoke as the <strong>Space</strong><br />

Shuttle Col umbia headed for orbit. After a<br />

series of delays (caused ma<strong>in</strong>ly by a pcrstsra<br />

nt hyd rogen fuel leak). STS-35 and<br />

SA REX 11 -0 1 was f<strong>in</strong>ally o n its way!<br />

STS ·35's primary miss ion was 10 carry<br />

NASA's Astro-t spacelab with three ultraviolet<br />

telescopes to observe the universe<br />

<strong>in</strong> ways never viewed befo<br />

re . Operat<strong>in</strong>g NASA's own<br />

Goddard <strong>Space</strong>flight Cente r 's<br />

Ultraviolet Imag<strong>in</strong>g Telescope<br />

CU lT) was payload specialist Ron<br />

Parise WA4SIR. In 1978 un asrronomcr<br />

Ron, a ham s<strong>in</strong>ce 1962,<br />

was complet<strong>in</strong>g his grad uate studies<br />

at the University of Florida,<br />

and by 1980 he was pan ofthe UIT<br />

learn. Little did Ron realize then<br />

that he 'd be fly<strong>in</strong>g with the UIT<br />

<strong>in</strong>strument he helped develop.<br />

The UIT is best described as a<br />

so phistica ted tel ephoto camera<br />

with super-sensitive film and a violet<br />

filter. Imag<strong>in</strong>e a telephoto ca m­<br />

era with a field of view 2S% wider<br />

than the full moon with ultra-lowlight<br />

film with an effective ISO<br />

(ASAI o f a couple ofhu ndred thou ­<br />

sand (<strong>in</strong> compariso n with the 100­<br />

400 film you'd normally purchase).<br />

It has a filte r so violet the<br />

human eye can't see it. further <strong>in</strong>to<br />

ultraviolet than Hubble 's capabilities<br />

. Also, <strong>in</strong>stead of an 18 or 36<br />

exposure roll of film , you ha ve a<br />

film pack with over J()(X) exposures<br />

of 70mm fil m~ That's one<br />

heck o f a telephoto camera!<br />

SAREX II<br />

Photo B. Mission commander Vance Brand talks withfamify mem-<br />

hers via the SAREX 2 meter l<strong>in</strong>k. Photo courtesy ofNASA.<br />

The launch of the Astra I mission<br />

marked the beg<strong>in</strong>n<strong>in</strong>g ofa new<br />

se ries of SAREX (Shuttle Amateur<br />

Radio EXperiment) nights .<br />

The primary m issio n o f thi s<br />

SA REX was to communicate with<br />

a number o f classrooms across the<br />

U.S., as well as to pro vide hams<br />

worldw ide a way of directly con-<br />

54 73 Amateuf Radio Today . March, 1991<br />

nect<strong>in</strong>g up to the shuttle via a packet radio<br />

robot.<br />

In addition, Ron recommended try<strong>in</strong>g shipto-ship<br />

contact between Columbia and the<br />

Soviet space station Mir . He said, " The idea<br />

came to me some time ago, just because he re<br />

was Mir ope rat<strong>in</strong>g 2 meters and we were<br />

go<strong>in</strong>g to be operat<strong>in</strong>g 2 meters. and we ought<br />

to talk to each other...<br />

Any Columbia-to-Mi r contact would be<br />

Photo A. Ron Parise WA4SIR work<strong>in</strong>g the world from the SAREX<br />

operat<strong>in</strong>g position onboard STS-35. Phoro courtesy ofNASA.<br />

much eas ier from the Sov iet side than from<br />

the U.S. because Mir 's ham shack <strong>in</strong>cludes a<br />

25 watt transceiver and an outside antenna,<br />

while the Columbia has an <strong>in</strong>side antenna and<br />

5 walt transceiver .<br />

Contact between the IWO vehicles is complicated<br />

by two factors. The most obvious<br />

problem, the Doppler shift, actually turns out<br />

to be fairly <strong>in</strong>significant. More complicated<br />

is the motion of the two spacecraft. S<strong>in</strong>ce the<br />

spacecraft are <strong>in</strong> different orb its at<br />

different altitudes. and travel<strong>in</strong>g <strong>in</strong><br />

different di rections, the range between<br />

the spacecraft and the l<strong>in</strong>e of<br />

sight angle changes quickly: One<br />

m<strong>in</strong>ute you ' re several thousand<br />

kilometers fro m each other, the<br />

next you' re right next to each other,<br />

and then you' re several thou ­<br />

sand miles away aga<strong>in</strong>.<br />

Low Incl<strong>in</strong>ation<br />

Unlike the earl ier ham radio<br />

shuttle nights, Astra was launched<br />

<strong>in</strong>to an orbit with an <strong>in</strong>cl<strong>in</strong>ation of<br />

28 .5 deg rees , the typical orbit for<br />

most shutt le fli ghts . <strong>Space</strong>craft<br />

lau nched to the east gai n ex tra payload<br />

capacity due to the Earth 's rotation:<br />

A spacecra ft launched due<br />

east can carry the most payload; the<br />

orbit is <strong>in</strong>cl<strong>in</strong>ed to the equator at the<br />

same angle as the latitude of the<br />

launch site . The end result is that<br />

Astro flew no further north of the<br />

equator than the KSC launch site,<br />

and at the same latitude to the<br />

south, 28 .5 degrees. The <strong>Space</strong>lab<br />

I m ission w ith O wen Garriott<br />

W5LFL and <strong>Space</strong>lab 2 with Tony<br />

England W00RE flew <strong>in</strong>to higher<br />

<strong>in</strong>cli nation orbi ts for better Earth<br />

observation capabilities, the tradeoff<br />

be<strong>in</strong>g less payload.<br />

The iro ny is that the Sov iet space<br />

statio n Mir is <strong>in</strong> a 51.6 degree<br />

orbit, halfway between the <strong>Space</strong>lab<br />

2 and <strong>Space</strong>lab 1 orbits. Had<br />

Astra been launched <strong>in</strong>to a higher<br />

<strong>in</strong>cl<strong>in</strong>ed orbit, longer opportu nities<br />

for Mir contacts cou ld have been<br />

possible.

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