NASA Science Internet (NSI) was a wide-area network established by ...
It’s important to understand a few key concepts when it comes to th...
The Mars analog experiments conducted by NASA in Antarctica were de...
In 1992, NASA developed an underwater Remotely Operated Vehicle (RO...
### Ross Sea Ice Shelf The Ross Sea Ice Shelf, is the largest ice ...
INTELSAT, which stands for the International Telecommunications Sat...
Tracking satellites in inclined orbits presents unique challenges d...
A multiplexer (MUX) is an electronic device that combines multiple ...
### LNB An LNB, or Low Noise Block downconverter, is an essential ...
### T1 Microwave Link A T1 microwave link is a type of digital tra...
You can watch the ABC segment [here](https://www.youtube.com/watch?...
In this context, the occultation is caused by the sun's infrared ra...
### Demarc A **demarc**, short for demarcation point, is the physi...
### Motion Compensation Motion compensation is a technique used ...
Establishing
a
Real-Time
video
link
to
Antarctica
On November
24,
1992,
NASA
engineers implemented a real-time video link between McMurdo
Station in the Antarctic and the continental United States. The problems encountered and the
solutions developed in establishing a network in a harsh and isolated environment provide valuable
insights into the conditions space explorers will encounter in planetary exploration. These efforts
have enabled subsequent breakthroughs in technology applications, education, and telepresence.
Mark
Leon
MARK LEON is deputypro-
ject
manager for the NASA
Information Infrastructure
Technology and Applications
Project at Ames Research
Center and deputy program
manager for the NASA IITA
K-12Program.
8
n November 24,1992, NASA Science
,Internet (NSI) engineers implement-
ed the world’s first real-time video
link between McMurdo Station in the
Antarctic and the Continental United
States; this link was also the first real-time video
transmission accomplished from such a low latitude.
The effort, which built upon NSI’s existing Antarc-
tic high-speed data communications infrastructure,
was a response to last-minute requests from
major television networks for live coverage of the
National Aeronautics and Space Administration’s
(NASA) Mars analog experiments in Antarctica. To
meet broadcast requirements for bi-directional
video, NSI employed laser, microwave, and satellite
communication links, as well as a variety of video
codecs and multiplexers. NSI implemented sever-
al different network configurations within a short
period of time to accommodate requirements for
both live broadcasts and scientific experimenta-
tion with a remotely operatedvehicle. The problems
encountered and the solutions developed in
establishing a communications network, in a
harsh and isolated environment equipped with
World War I1 vintage equipment, provide valu-
able insights into the conditions space explorers
will encounter in planetary exploration. These
ground-breaking efforts have enabled subse-
quent breakthroughs in technology applications,
education, and telepresence.
NASA Science Internet engineers at NASA
Ames Research Center (ARC) in California have
implemented four different communication con-
figurations in the Antarctic to date: one was part
of NSI’s original Three-Year Plan; one was the
result of an urgent request by the ABC network,
NASA, and the National Science Foundation
(NSF); and
two
arose as a result of accomplishing
the second requirement.
NSI’s
Three-Year Plan included initiation of a 56-
Kb/s data link for Internet service in the first
year, 1991, with an increase to 128 Kb/s in the
second year. When the repositioning of a satellite
from inclined to geosynchronous orbit achieved
bit error rates of at 768 Kb/s, plans to increase
bandwidth for telepresence applications and
compressed video were accelerated. The increased
bandwidth performance indicated that proof-of-
concept testing at McMurdo Station could be
accomplished in 1992 instead of 1993.
An experiment simulating operation of a
Remotely Operated Vehicle (ROV) was there-
fore conducted in July 1992, and in November,
ABC presented an urgent request to use the
video circuit for a live broadcast for “Night Line”
and “Good Morning America”
15
days hence.
Because of the short deadline, NSI engineers
worked around the clock to implement the
requirement. The effort to establish the bi-direc-
tional real-time video link is described herein.
Background
n 1990, NSI engineers met with the National
I
Science Foundation (NSF) to pose NASA’s
Antarctic communication requirements for ’91, ’92,
and ’93. At that time, NSI envisioned high band-
width requirements to support compressed video
for the purpose of returning vision from a robot
exploring beneath the Ross Sea Ice Shelf. NSF
did not, however, include NSI’s requirements in
its bid for a communications implementation due
five years later, in 1995.
As a result, NASA developed its own Three-
Year Plan. The first year of the plan, 1991, includ-
ed requirements for 56 Kbis of data for Internet
service; the second year involved higher band-
width, also to support data; and the third year
was to involve yet higher bandwidth for telep-
resence applications and compressed video.
In 1991, NSI had a link to IntelSat 177 East,
which had an inclined orbit of 3”. This link pro-
0890-8044/95/$04.00
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Network
March/April
1995
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Figure
1
.
Otvivicw
ofAntarctic
video
circuit
vided approximately six hours of dedicated real-
time connectivity between McMurdo Station
and the Sylmar Tracking Station in California. How-
ever, because the satellite was in an inclined
orbit, it was difficult to keep a lock
on.
Its aver-
age bit error rate of
as
it
entered the horizon prior
to
setting. Many
problems were experienced with this particular
implementation, including outages of several
hours at a time without
good explanation. The
service was run in its entirety for only about two-
and-a-half weeks of the originally planned two
months. The difficulties NSI experienced in
establishing the satellite link were exacerbated
by
the conditions in Antarctica, and in Black
Island and McMurdo Station, specifically. This
link, however, provided the infrastructure which
would be used in 1992.
In
the 1991 configuration, the entire 128-KbIs
circuit was channeled through the multiplexer
(MUX) into a voice multiplexer (RLX) for four
voice channels, and into the data router (Proteon)
for
56
Khis
of data (Fig.
2).
This particular imple-
mentation was jointly funded by NASA and NSF.
The 1992 configuration was originally planned
to
be much like that for 1991, and in 1993, NSI
planned to upgrade to higher bandwidths to pro-
vide compressed video. The compressed video
would be used
to
return video from the ROV
underneath the frozen lakes in the Taylor Valley
and to allow operation of the ROV remotely
from ARC. What actually occurred differs con-
siderably from the original plan.
dropped sharply to
W
Figure
2.
1991
Antarctic communications configuration.
Safeellife
Move
After the experiences in 1991 with the inclined
satellite, it became evident to NSI engineers that
a geosynchronous satellite would be required.
By organizing a contract with Comsat through
IDBISTARS, an inclined satellite was moved from
177"
East to 180" East, and a geosynchronous
satellite was moved from 180" East to
177"
East.
By switching the
two,
NSI gained access to a satel-
lite with much greater capability. NSI used an
LNB
with an ultra-high gain step on the antenna
assembly to communicate with this satellite, a
configuration which is much more powerful than
what is normally used.
On
the down-link we
received a 42.5 db signal-to-noise (SIN) ratio.
Aftcr moving the satellites and establishing
the link to the receiving stations at Vallejo, Cali-
fornia and Black Island, Antarctica, NSI was able
to get bit error rates of
10-8
operating at a total
bandwidth speed of
768
Kbis.
From Black Island
lEEE
Network
March/April
1995
9
to McMurdo Station, NSF employed a T1
microwave link operating with a bit error rate of
10-10.
This preparation established the infrastructure
for subsequent communications at McMurdo Sta-
tion. As a result of having additional bandwidth
available, NSI decided to advance the testing
of
a
full-motion video link, originally scheduled for
1993, to 1992 in preparation for the telepresence
objective. NASA performed a swift procurement
of video codec/s, infrared lasers, and other com-
munications equipment required to perform the
basic test at McMurdo Station.
ROV
Simulation
In July 1992, NSI simulated video transmission
from the ocean under the frozen Ross Sea Ice
Shelf by placing the ROV in the Navy pool at
ARC (Fig. 3). Base-band amplifiers were used to
send a signal to the roof of the pool house, and
IR lasers and a cable TV network then brought
the video to the NASA ARC ground station.
Next, SatCom F2R was used in loop-back mode
to send the signal back to ARC. From there it
was distributed to the researchers’ location
so
that they could get a sense of the video quality
and time delay which would be comparable to the
signal coming from Antarctica. The video signal
they saw was being compressed at 384 Kb/s, uti-
lizing a Rembrandt video codec made by Com-
pression Labs, Inc. (CLI). This video codec
equipment was inferior compared to the CLI
CTX plus planned for actual deployment to
Antarctica.
Navy pool area
Coax cable
base band
Infrared
modulator
Navy bldg.
19
Infrared
demodulator
New Urgent Re uirements
November
7
99
3
n November 9, 1992,
I
received a call from
0
the ABC network requesting use of NSI’s
video circuit for a live broadcast from Antarctica
back to the ABC national news network for their
“Night Line” and “Good Morning America” pro-
grams on November 24 and 25, respectively. Our
engineering team thus began working around the
clock to prepare
for
an “all-or-nothing” mission. One
of our engineers, Roxanne Streeter, had been
sent earlier to Antarctica to support the ROV
experiment; this new requirement, however, made it
necessary for me, as a design engineer, to travel
to Antarctica to modify the design
so
that ABC
could use it for the video broadcast, and also to
design audio into the original circuit.
I
worked 15 hours on Veteran’s Day to secure
as much equipment as I could before leaving
ARC. However, because of the last-minute
request, we did not have enough time either to
procure or to send all
of
the additional equip-
ment we would need for Antarctica, nor did we
have enough time to do the additional engineer-
ing designs necessary to achieve broadcast quali-
ty. Worst of all, we were going down
to
install
high-technology equipment in vastly outmoded
circumstances, with no Radio Shack for thousands
of miles. We had no guarantee that the broadcast
would work since this type of link had never been
done before.
Last minute, inadequate planning caused other
-
ARC
bldg. N-240
ATS-1
k
43
Satellite down-link
h
Satellite up-link
--
384
I
Kbps
1
384
Kbps
comp. comp.
encoder decoder
Base
I
1
Base
ARC
bldg.
N-245
demod.
base
band
band band
Channel
3
demod. mod.
-
Channel
50
RF
--
~-
___.
-
__
-__
-
-_
_--
~~
-~
~~ ~
~~ ~~~
I
Figure
3.
Remotely operated
vehicle
test: ARC navypool.
10
IEEE
Network
March/April
199s
Station
I
Microwave
to
I
1
ABC
trailer
I
Commbnications
house
(audidvideo power)
Phone Phone
I
Phone
--
Leaend
3
twisted pair
w
ww
I
/
I
I
I
/
t
B<
Base band signal
IR-T:
Infrared transmitter
IR-R:
Infrared receiver
=
Ross
ice shelf
=
McMurdo Station
Note: cables are not
under the ice shelf
~~
______-
.
-p
___~
~-
_-
Figure
4.
Configuration
1:
ABC
broadcast link.
unexpected problems beyond those concerning
equipment. Just before
I
left for Hawaii,
I
learned
that
I
had been given incorrect information on the
customs forms needed to transport equipment
through New Zealand, and that customs agents
there would not let me catch my connecting flight
to Christ Church, the staging base tohtarctica, until
my paperwork was in order. My wife had to go to
NASA in the middle of the night to get the cor-
rect forms and fax them to me in Honolulu
so
I
could make the flight to New Zealand.
Seven days after the initial request, on November
16,
I
finally deployed to Antarctica. The flight
seemed interminable in the spartan cargo plane,
but after losing one day crossing the date line and
surviving a bout with food poisoning,
I
arrived
November 20. After only one hour’s sleep,
I
pro-
ceeded to work around the clock to get the link up
and running for the November 24th full-motion
live broadcast for ABC’s “Night Line.” Nineteen-
to-22-hour work days were normal, and though
tiring, were made somewhat easier because of
the 24 hours of sunlight every day during the aus-
tral summer. Since it was impossible to make
scheduled mealtimes,
1
had to rely on coworkers
to bring food out
to
the work site.
Problems, Makeshift
lm
plem
en
tation,
and
Con
fig
ura
tion
Breakthrough
he network configuration, which we engi-
1
neered to accommodate ABC’s request for a
live broadcast, is shown in Fig. 4.
lack
of
Resources
The most serious problem we faced was the lack
of time to adequately plan a task of this complex-
ity, since detailed planning is essential if parts are
to be available at remote areas such as McMurdo
Station. We faced a serious lackof resources to imple-
ment the task, ranging from audio connectors to
interface cables, and even to wrong circuit boards.
Tuning the
infrared laser
eq
u
ipm
e
n
t
was too
awkward
in
my
bulky
gloves,
so
I
often removed
them, which
caused
my
skin
to stick to
the controls
and
rip
off
in
the cold.
---
.__-
--
--
__
i
I
Baseband video in
I
Baseband video out
,
Baseband audio in
I
Baseband audio
out
Video
cod=
512
or
384
Kb/s
compressed video ckt.
9.6
Kb/s
remote access ckt
I
128
Kb/s
digitized voice and
fax
ckts.
I
t
9.6
Kb/s
remote access ckt.
Channel
ba>
768
KWs
data ckt.
-
Black
1
link
I
$%?ck.
1
9
6
Kb/s
data ckt
Lpp*-
~.___--
-
--
____
___.
-
-
~
_-~
Figure
5.
Communications infrastructure atMcMurdo station.
IEEE
Network March/Aprill995
11
This
eight-
minute
oculation
happened
seven minufes
before ”Good
Morning
America” was
to go live, and
although
if
cleared
up
in
eight minutes,
the
ABC
staff
was somewhat
frantic.
Microwave
to
Black Island
Legend
BB: Base band signal
IR-T: Infrared transmitter
IR-R: Infrared receiver
ROV: Remotely operated vehicle
m
Ross ice shelf
=
McMurdo Station
W
Figure
6.
Configwatiori
2:
ROVlink.
The most serious problem was the lack of a 768
Kbis
interface card to connect the
T1
microwave link
from Black Island to the half-T1 channel bank at
McMurdo Station.
So
I
had hand-carried a 768 Khis
card to Antarctica to replace the defective part
(Fig.
5).
From that point on, we began deploying
IR laser, video codec, etc.
Harsh Environment
The extreme cold and wind of the Antarctic envi-
ronment presented unexpected problems in
achieving our mission. Black cables would melt
their way into the ice, then as the temperature
dropped, freeze over, making it difficult to move
them. Tuning and stabilizing the delicate infrared
laser equipment to transmit the signal was too
awkward in my bulky gloves,
so
I
often removed
them
for
tuning, which caused my skin to stick to
the controls and rip off in the cold.
E
quipmen
t
Isolation
The power supply in Antarctica is severely limited.
Because of the general lack of power, we were
using two different phases of electricity in the
same building. Unfortunately, it was not made
clear to
us
that multiple phase sources were being
used until it was too late. We would use all of the
current on one breaker, then go to the other.
However, any connection between some pieces
of equipment without an isolation transformer
produced a two-phase delta of
120
degrees.
In
the power cycle, the potential difference of about
60
V
between the two points produced 60
V
shocks. We had to
do
a lot of equipment isolation,
resulting in burned out boards, physical shocks,
and short tempers.
Oculation Period
The sun orbits low on the horizon,
so
at one point
between the IR transmitter and the IR receiver it
overcomes the transmission signal for about
8
minutes out of every
24
hours. This eight-minute
oculation happened seven minutes before “Good
Morning America” was to
go live, and although it
I
Trailer
14
1
Microphone
rideo
Under ice shelf
-
cleared
up
in eight minutes, the ABC staff was
somewhat frantic. Even though
I
had tested it,
I
did not know how much the sun’s position changes
with respect to rotational aspects -which could
change a few minutes a day.
I
could only move
the equipment a certain amount in any direction
because the sun had to
be
in the right spot for the
camera. The oculation period
is
the only timeslot
when, because of the low-look angle, no signal can
be received. The set
up
was good for “Night Line,”
but for “Good Morning America” it was very close
(actually a matter of luck). Later, when there was
more time,
I
did a statistical analysis to determine
the oculation period of the sun.
Unacceptable Audio Signal
The video codec box we had at McMurdo caused
an audio problem for
ABC,
because while other
video codec boxes had been recalled because of
unacceptably high audio output, the one they had
at McMurdo had not been recalled.
I
had to
attenuate the audio signal by
15
dB
so
that it would
be within the normal acceptable audio ranges for
ABC. We had no indication that its signal was too
hot until the signal reached New York.
I
back-
tracked it to the output of the video codec and
discovered that
I
had to internally insert a
15
dBpad;
I
found this out when there were only
14
minutes
of satellite time remaining in which to solve the
problem. Since there was nothing available to
use
there,
I
finally lifted something from the ABC
sound man that would work.
Video Codec
(CH)
Interfaces
In the process of interfacing the video codec boxes,
a blocking processor on the CLI blew out.
I
was
able to replace it only because
I
had taken redun-
dant boards down.
Dealing with
a
large Number
of
Demarcs
NSI had to interface with seven different groups to
get from Antarctica to ARC, including: the com-
munication trailer on the ice; the fire house (the
location of the communication hub); Black Island
12
~
IEEE
Network MarchiApril
1995
W
Figure
8.
Configurution
4:
ROVtelepresence
link.
link. On another occasion while in Antarctica,
I
had
to redesign an audio circuit. Because of the
World War
11
vintage equipment in the Antarctic,
I
had to engineer from scratch several of the criti-
cal links to facilitate the transmissions.
Conneciors
The audio level was too low for the press confer-
ence coming from Antarctica,
so
I
had to amplify it.
I
shanghaied
a
1950s
PA
system they had at
McMurdo, which was used by an entcrtainment
group. The connectors were not compatible,
so
I
shoved large paper clips into the holes, and
sol-
dered alligator clips to the dissected
XLR
jack
(three-pronged). Another problem with the con-
nectors was that they could not be laid
on
the ice
because they would melt the ice and subsequently
get water in them.
Cold
Solder Joinis
When you are sitting
on
a
-20" surface trying to
solder something, the slightest breeze will turn it
into
a
cold solder. The solution is to have
a
hair dryer
on
while soldering
to
keep the air around the sol-
der warm. A good solder is essential for a homo-
geneous bond or poor connectivity will result. If
the outside of
a
bond cools too fast, it will break
connectivity and produce high resistance.
Cable lsolaiion
Because the preparations were
so
rushed,
NSI
had a 60 Hz hum (power cycle) during the press
conference. This was because the video, audio,
and power cables were wrapped inside the con-
duit going to the roof
of
the fire house. This
implementation was the result of a rushed job.
The 60
Hz
on
the power cable induced 60
Hz
on
both the video and the audio cables, although the
interference is significant only
on
the audio. We
were not able to isolate the 60 Hz hum because
we couldn't separate the cables which should
have been isolated or shielded to begin with.
Telepresence Experiment Moved
up
from
'93
io
'92
The mission of the entire
NSI
Antarctic operation
has always been to support the communication
requirements for Mars Analog research. We were
to have provided telepresence support in 1093,
but when Carol Stoker of the ExobiologyiMars
Analog Project at ARC saw what had been done
for the broadcast and press conference, she asked
whether or not we could go ahead with support
for a telepresence experiment instead of waiting
until 1993.
Therefore,
I
analyzed the McMurdo configura-
tion and decided that one of the existing 9.6 Kbis
data circuits could be reconfigured to meet that
requirement. Two of the 9.6 Kbis circuits were
being used
for
remote control of the video codec
and the NSI router. Since these circuits are
meant
only
for secondary access for control of
the equipment,
NSI
engineer
Roxanne
Streeter
disabled the NSI 9.6
Kbis out-of-band circuit and
borrowed
a
couple of 9.6 Kb/s modems from
people at McMurdo, using the phone lines that
NSI
had used for the ABC broadcast. ABC had
needed three sets of twisted pair to communicate
with the producer, the camera man, and the audio
man, each of whom had his own head set. Streeter
took one of those twisted pairs, hooked it to
a
modem, used
RS
232 interface to plug into the
9.6 Kb/s circuit, then was able to get it out to the
trailer, and from the trailer, plug in the
RS
232
to the outputs of the remote control for the ROV.
-
14
IEEE
Network
MarchiApril
19%
Additional problems with DTE and DCE inter-
faces and with signal inversion were all overcome.
After the ABC broadcast, we moved the laser
to point at the ROV hut (Bldg. 14). This was the
same configuration as the ABC broadcast, but
instead
of
using the input from the cameras, it
used input from the ROV. Video quality for the
ROV experiment was not as good as that for the
ABC broadcast. The 25 dB
SIN
ratio on the base-
band signal coming from the ROV was inferior;
65
dB SIN ratio is standard for broadcast quality.
Even though we had designed the system to
operate at a
50
dB
S/N
ratio, the system was limited
to the poorest link, which in this case was
25
dB.
The main reason for the drop in video quality is
that their communications medium utilizes video
going over
1000
ft of twisted pair, which has sub-
stantial attenuation causing signal loss.
Thus, on Friday, December 5,1992, NASA
accomplished its first telepresence application.
This event marked a historical first when a
researcher at ARC experienced moving through
the water, hundreds of feet under the Ross Sea Ice
Shelf in the Antarctic, as though hewere on the back
of the robot. This was accomplished by fitting the
researcher with a virtual reality headset; with
each movement of his head, the tracking cameras
on the robot moved and transmitted the images
directly to him.
Conclusion
s
a direct result of the
NSI’s
ground-breaking
A
efforts in November 1992, several historical
breakthroughs have occurred, not only in tech-
nology applications, but in historic “firsts” for
education and telepresence. For example, NASA
has provided remotely operated telepresence
applications as demonstrated in the National Air
and Space Museum in December 1993, in which
students were able to wear stereovision virtual
reality helmets and guide a robot and its arm
operating beneath the frozen surface of the
Ross
Sea at the bottom of the planet. We were able to
send back high quality video compression algo-
rithms at half-T1, we were able to send back
freeze-frame video from the South Pole, we have
recently sent back live video from places like the
remote Dry Valleys in Antarctica, and we will
soon be sending back live video from the South
Pole. These are all the direct result
of
technology
applications that were implemented in the win-
ter of 1992. This technology is not unique; it is
turn-key technology
-
self-contained systems
sold by a vendor which and used intact by the
customer. The unique and unprecedented
aspects were NASA’s rigor and the innovative
fashion in which this historic first was implement-
ed at a time when it was thought to be technically
unfeasible. As technology advances, several
issues must be addressed.
In
teroperabihy
The equipment described in this article must be
more universally interoperable if it is to be more
widely utilized. Industry needs to develop inter-
operability standards for equipment and inter-
faces
so
that if a card in a codec fails, for example,
or if an interface fails, it can be successfully
replaced from a similar vendor. However, until stan-
dards are agreed upon and resolution at those
standards is acceptable for dynamic applications,
that will not be possible. Existing standards are too
low in resolution to support these types of appli-
cations-industry standards for interoperability
in image quality and frame rate are
so
low that
we are still forced to use proprietary solutions.
Clearly the success of a specific vendor will not
be based on a single user like NASA but will be
based on its ability to integrate and interoperate
with other equipment.
Multiplexing
Requirements are growing for technology that can
integrate voice, data, and video. Until off-the-shelf
technology can ensure a superior mean time to
failure (of several thousand hours) for self-con-
tained pieces of equipment such as routers that
could handle data muxing internally, we will have
to use proprietary equipment in Antarctica. The
direction technology is currently taking is to make
compressed data in the form of voice and video
readily available over the Internet. Therefore, rather
than having a router that would incorporate data or
video muxing, industry should continue to devel-
op packet video software and packet audio soft-
ware that run over TCP/IP. These softwares will
command themarketwhen the wide area network
backbones mature to speedsof2Gbh. Proprietary
solutions will become obsolete.
Biography
MARK
LEON
received a B.S. in electrical engineering from San Jose State
University and
is
working toward an M.B.A. ot Santa Clara University.
He
is
currently deputy project manager for the NASA Information Infra-
structure Techno1 y and Applications Project at Ames Research Center,
Moffet Field, Ca??ornia, and deputy program manager for the NASA
IITAK-I2 Program. During histenureasEngineerin Manogerofthe NASA
Science Internet, he designed and implemente! the first audio/vidw
link to Antarctica.
His
e-mail address
is:
leon@nsipo.nasa.gov.
The
equipment
described
in
this
article
must
be more
universally
interoperable
if
it
is
to
be
more widely
utilized.
IEEE
Network
March/April
1995
__
_-
-
--I
15

Discussion

### LNB An LNB, or Low Noise Block downconverter, is an essential component of a satellite communication system. If you have a satellite dish at home, the LNB is typically the only part of the satellite dish that contains electronic components and is located at the front of the metal arm. The LNB serves two crucial functions: it acts as a low-noise amplifier, taking the extremely weak satellite signal and amplifying it, and it also serves as a block downconverter, converting the high-frequency satellite signals to lower frequencies. The satellite signals are very weak by the time they they reach the dish. The large, round, "dish" part of the antenna acts as a lens, focusing as much signal as possible onto the LNB. The LNB then amplifies that signal and sends it down the cable to the satellite receiver or modem. In the case of the NSI configuration, they used an LNB with an ultra-high gain step, which provided an additional amplification stage, allowing them to communicate with a satellite that might otherwise be difficult to reach. ![](https://i.imgur.com/LBVnqwj.png) ### Motion Compensation Motion compensation is a technique used to reduce the amount of data required to represent a video sequence by exploiting the temporal redundancy between adjacent frames. In a video, consecutive frames often contain similar content, with only small changes or movements occurring between them. Motion compensation takes advantage of this similarity by predicting the content of a current frame based on the information from one or more previous frames. Instead of encoding each frame independently, the encoder identifies the motion or displacement of objects between frames and encodes only the differences (known as residuals) along with the motion information. In this context, upgrading the video segment from 384 Kb/s to 512 Kb/s allowed for better motion compensation. The higher bitrate provides more data for the encoder to work with, enabling more accurate motion estimation and compensation. This results in faster tracking of moving objects and improved overall video quality, especially in scenes with significant movement. NASA Science Internet (NSI) was a wide-area network established by NASA in the late 1980s to support scientific research and collaboration, in other words, non-mission critical computer networking. Its purpose was to connect NASA centers, research facilities, and educational institutions, enabling them to share data, resources, and communicate more effectively. NSI played a significant role in the early development of the Internet, contributing to networking technologies and protocols. It supported a variety of services like email, file transfer, and remote login, and it connected to other major networks of that era, such as the ARPANET and NSFNET, furthering the growth of the Internet. The Mars analog experiments conducted by NASA in Antarctica were designed to simulate conditions on Mars, utilizing the extreme and isolated environments of Antarctica as a stand-in for the Martian landscape. These experiments focused on understanding how humans could survive, work, and conduct scientific research in such harsh conditions. Key aspects of these experiments included testing life support systems, space suits, habitat designs, and scientific equipment that might be used on Mars. They also studied human behavior and performance under prolonged isolation and extreme conditions, crucial for long-duration space missions. In this context, the occultation is caused by the sun's infrared radiation interfering with the IR communication system when the sun is low on the horizon. The sun emits a significant amount of infrared radiation, which can overwhelm the IR sensors designed to detect the specific infrared signal used for communication. As a result, when the sun is in a particular position relative to the IR transmitter and receiver, its infrared emission overpowers the communication signal. You can watch the ABC segment [here](https://www.youtube.com/watch?v=E03JpFVvX5s) In 1992, NASA developed an underwater Remotely Operated Vehicle (ROV) designed to explore undersea environments in Antarctica. This ROV was notable for being controlled via a Virtual Reality headset. This pioneering technology allowed operators to control the ROV as if they were navigating underwater themselves, offering an immersive experience and precise control. You can see a video of the ROV in action [here](https://youtu.be/E03JpFVvX5s?t=783). ### Demarc A **demarc**, short for demarcation point, is the physical point where the responsibility for a telecommunications network or circuit changes from one party to another. Tracking satellites in inclined orbits presents unique challenges due to their orbital characteristics. Unlike geostationary orbits, which are on the same plane as the Earth's equator, inclined orbits are tilted relative to the equatorial plane. This tilt causes the satellite to appear to move in a figure-eight pattern as seen from the Earth's surface. As a result, antennas on the ground must constantly adjust their alignment to track the satellite's movement across the sky, which is more complex and challenging than tracking satellites in a stable, geostationary orbit. This constant adjustment is what makes maintaining a lock on a satellite in an inclined orbit more difficult. ### Ross Sea Ice Shelf The Ross Sea Ice Shelf, is the largest ice shelf in Antarctica, covering an area of approximately the size of France. The shelf can be anywhere from 300 to 6,000 feet thick. McMurdo’s station sits on the shelf’s western edge. ![ross sea](https://i.imgur.com/fWIWtaI.png) A multiplexer (MUX) is an electronic device that combines multiple input signals into a single output signal. In this case the MUX takes the separate voice and data streams and interleaves them, allowing them to be transmitted together over the same communication link. ### T1 Microwave Link A T1 microwave link is a type of digital transmission system commonly used in telecommunications. Microwave links are limited by the line of sight between antennas. This range is typically up to about 50 miles, but can vary based on factors like antenna height, frequency band, and environmental conditions. In this case, McMurdo station is about 22 miles from Black Island - well within the range of T1 link. ![](https://i.imgur.com/umwXpkO.png) *Distance between McMurdo station and Black Island* INTELSAT, which stands for the International Telecommunications Satellite Organization, was founded in 1964 as an intergovernmental consortium. Initially, it had 11 member countries, but its membership grew over time. The primary goal of INTELSAT was to create a global satellite communications system that would facilitate international telecommunications and media broadcasting. In 1965, INTELSAT launched its first satellite, called Early Bird (Intelsat I), which provided the first two-way connection between Europe and North America. IntelSat played a crucial role in enabling live broadcasts of major world events, such as the Olympics and the Apollo 11 moon landing, to a global audience. This helped to connect people around the world and foster a sense of global community. Before the widespread adoption of fiber-optic cables and the internet, satellites like those operated by INTELSAT served as a vital backbone for international phone calls and television transmission. They provided a reliable means of communication across vast distances, even in areas where terrestrial infrastructure was lacking. In 2001, INTELSAT underwent a significant change as it was privatized, becoming a private company. The IntelSat 177 East that Mark León references in the paper is likely [Intelsat VA F-11](https://en.wikipedia.org/wiki/Intelsat_VA_F-11) (then named Intelsat 511), which operated at a Longitude of 177.0° East from 1992 to 1995. It’s important to understand a few key concepts when it comes to the orbits that satellites can assume: - **Inclined Orbit**: An inclined orbit is an orbit that is tilted with respect to the Earth's equator. The angle between the orbit plane and the equatorial plane is called the inclination. Satellites in inclined orbits do not maintain a constant position relative to the Earth's surface. They move in a sinusoidal pattern, oscillating between the northern and southern hemispheres. The inclination of the orbit determines how far north and south the satellite will travel. - **Geosynchronous Orbit**: A geosynchronous orbit is an orbit where the satellite's orbital period matches the Earth's rotational period. This means that the satellite completes one orbit around the Earth in the same time it takes the Earth to complete one rotation on its axis. Satellites in geosynchronous orbits have an altitude of approximately 35,786 kilometers above the Earth's surface. However, geosynchronous orbits can be inclined, meaning that the satellite may not maintain a constant position over a specific point on the Earth's equator. - **Geostationary Orbit**: A geostationary orbit is a special type of geosynchronous orbit that has an inclination of nearly zero degrees. Satellites in geostationary orbits remain at a fixed position relative to the Earth's surface, appearing stationary to ground observers. These orbits are located directly above the Earth's equator and have the same altitude as geosynchronous orbits (approximately 35,786 kilometers). Geostationary orbits are particularly useful for communications, television broadcasting, and weather monitoring, as the satellites can continuously cover a specific region of the Earth.