Deep Space Communication
Deep Space Communication
Deep Space Communication
DEEP SPACE
COMMUNICATION
PRESENTED BY:
P.MOHANA SAI GEETHA , K.GOWTHAMI,
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antennas on Earth must be very large and be • The Madrid Deep Space
equipped with highly sensitive receivers. Communication Complex, 60
The two main antennas in a spacecrafts are kilometers (37 miles) west of
high gain antenna and a low gain antenna. Madrid, Spain; and
• The Canberra Deep Space
• Low Gain Antenna Communications Complex (CDSCC)
• High Gain Antenna in the Australian Capital Territory,
40 kilometers (25 miles) southwest
DEEP SPACE NETWORK:The of Canberra, Australia near the
NASA Deep Space Network - or DSN - is Tidbinbilla Nature Reserve.
an international network of huge antennas
that allows people on the ground to Each facility is situated in semi-
radio and radar astronomy observations for interference. This strategic placement
the exploration of the solar system and the permits constant observation of
universe. It is best known for its large radio spacecraft as the earth rotates, and helps
antennas. The network also supports to make the DSN the largest and most
(JPL).
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data is the important data because the 5 Radio Science :The field of Radio
mission success depends on this data. Science improves our knowledge of the
engineering data contains the health and solar system and the theory of general
positional information of the spacecraft. relativity through radio frequency
2. Spacecraft Command: The purpose of experiments performed between spacecraft
the Command System is to provide the and the Deep Space Network's (DSN) Radio
means by which a Project controls the Science System. In the past, Radio Science
activities of its spacecraft. Control has performed experiments which have
information (Command Data), provided by allowed scientists to characterize planetary
the Project, is modulated on the RF carrier atmospheres and ionospheres, characterize
and transmitted to a spacecraft by a DSN planetary surfaces, characterize the
station. The Command System functions as planetary rings, characterize the Solar
a transfer medium between the Project corona, confirm general relativity,
Control Center and its spacecraft. characterize interplanetary plasma, search
3 Radiometric Tracking : The for gravitational waves, characterize
purpose of the Tracking System is to planetary gravity , and determine the mass
provide two-way communication between of the planets, moons, and asteroids.
Earth based equipment and spacecraft, to 6 Monitor and Control :The purpose of
make measurements that will allow the state the Monitor and Control System is two-fold:
vector (position and velocity) of spacecraft to provide real time monitor data to projects
to be determined. which reflect the status of project support by
4 Very Long Baseline Interferometry DSN systems, and to provide monitor and
control capabilities to operators of DSN
The purpose of the Very Long Baseline
systems' components.
Interferometry (VLBI) System is to provide
the means of directly measuring plane-of-
WORKING OF DSN:
the-sky angular positions of radio sources
(natural or spacecraft), DSN station The theory and challenges of deep
locations, interstation time and frequency space communications:Distance is the
offsets, and Earth orientation parameters. main problem in space communications,
since the intensity of electromagnetic
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radiation decreases according to 1/r2, that is radiated energy. A low gain antenna radiates
why signals from deep space probes are in a wide angle, while a high gain antenna
usually very weak when they reach the radiates in a narrow beam. On spacecraft
Earth. In order to receive the faint signal high gain antennas are used to send
back on Earth large parabolic disc antennas scientific measurements at high data rates
are used. To collect as much as possible of back to earth as well as receiving steering
the faint signal the antenna dish must be big. commands from earth; these antennas are
Since the electromagnetic radiation cannot highly directional and require very accurate
move faster than the speed of light there are aiming. Spacecraft are always equipped with
considerable time lag introduced in the at least one low gain antenna often two.
communications making real time These low gain antennas are very important
communications impossible. since they can intercept signals from almost
It takes over 5 hours for a signal any direction, this is useful if the spacecraft
from earth to reach the orbit of Pluto in the gets disoriented and the main high gain
outer part of the solar system. In order to antenna doesn’t point towards Earth. If the
communicate with the Earth the spacecraft spacecraft only had a high gain antenna it
must have a free line of sight to the Earth, would then not be able to receive any more
since radio waves cannot pass through large instructions from Earth. The low gain
solid objects such as planets and moons. A antennas are used in these kinds of situations
space probe orbiting a planet will therefore as a backup to receive the appropriate
lose contact with earth every time it gets on commands that will turn the spacecraft so
the far side of the planet. This means that the that the main antenna gets properly aligned
spacecraft will not be able to communicate to earth again. However, the low gain
with the Earth at all times. Even if the probe antenna can only handle a fraction of the
has a free line of sight to the Earth the data rate compared to the high gain antenna.
receiving antenna could be on the wrong Coding used in DSN:
side of the Earth, however by using several Most missions employ error
antennas in different places around the detecting – error correcting codes to
planet that could be solved. substantially improve telemetry link
The gain of an antenna is a measure performance. DSN users are reminded that
of how good the antenna is at focusing the their encoders should conform to the
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CCSDS Telemetry Channel Coding Blue adequacy of the link margin for
Book (CCSDS 231.0-B-1, September 2003. telemetry/dwell, tracking, telecommand
payload data reception. The IDSN station
Acceptable codes include:
has the responsibility of receiving the
1) Convolutional r = 1/2, k = 7 only. spacecraft health data as well as the payload
2) Reed-Solomon 223/255 only. data in real time. Later, conditioning of the
data takes place, before onward transmission
3) concatenated Convolutional / Reed-
of the same to Mission Operations Complex
Solomon at Bangalore. The tracking data
4) Turbo codes with rates: 1/2, 1/3, 1/4, or comprisingRange, Doppler and Angle data
will be transferred to the control center for
1/6, block sizes: 1784, 3568, 7136, and
the purpose of orbit determination. The
8920. payload data will be transmitted to the
INDIAN DEEP SPACE Indian Space Science Data Center (ISSDC)
NETWORK (IDSN):The Indian Deep as and when received by the payload data
Space Network consists of a 18-m and a 32- acquisition system, located at the station
m antennae that are established at the IDSN
campus, Byalalu, Bangalore. The Network is
CCSDS File Delivery Protocol (DSN) to
augmented witha couple of stations in the
western hemisphere in addition to the 64-m improve station utilization efficiency as well
antenna in Bearslake, Russia to improve the as reduce mission risk and costs, all DSN
visibility duration and to provide support
users should employ the CCSDS File
from the antipodal point.
Delivery Protocol (CFDP), to transfer data
The existing ISTRAC (ISRO to and from a spacecraft.
Telemetry Tracking and Command
Bandwidth Efficient Modulation
Network) S-Band Network stations will be
used to support the mission during Launch (DSN):Missions operating in the 2 and 8
and Early Orbit Phase (LEOP) that includes GHz bands, should employ bandwidth
Earth Transfer Orbit (ETO) up to a range of
about 1,00,000 km. Although the 18-m efficient modulation methods in
antenna is tailored for Chandrayaan-1 conformance with SFCG (space frequency
mission, the 32-m antenna can also support coordination group) and CCSDS
other planetary missions. The established
Recommendations.
IDSN is a state-of-the-art system, with its
base band system adhering to CCSDS Data Relaying:Some missions
(Consultative Committee for Space Data may propose dropping probes, landers, or
Systems) Standards, thus facilitating cross-
support among other TTC agencies. The even rovers to explore the surface of a
supporting network stations will ensure the planet/body. Others may insert orbiters
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around the same body. The result can be a problems where they are out of
multiplicity of spacecraft on or around a service for months at a time.
planet/body. While Mars has been the recent Furthermore, they are reaching the
focus, it is foreseeable that other planets or end of their lives. At some point they
objects in space could be of equal interest in will need to be replaced. The leading
the future. candidate is an array of smaller
dishes.
• By 2020, the DSN will be required to
support twice the number of
missions it was supporting in 2005.
CONCLUSION: Since all these
spacecraft are controlled by the DSN.
By 2015 NASA is planning for a
There are a number of limitations to
the current DSN, and a number of second Moon mission and by end of 2030 a
challenges going forward.
manned mission to Mars. These all require a
• There is only one DSN site in the powerful Earth communication Network.
Southern Hemisphere, Canberra.
There are no DSN network dishes in REFERENCE:
South America or Southern Africa, [1] How Spacecraft Will Communicate “on
so the DSN coverage of the Southern the Fly”, NASA CICT Program Office
Ames Research Center.
Hemisphere is limited.
www.cict.nasa.gov/infusion
• The need to support "legacy" [2] "NASA Tests First Deep-Space Internet."
missions that have remained PHYSorg.com. 18 Nov 2008.
www.physorg.com/news146245446.html
operational beyond their original
lifetimes but are still returning [3] http://deepspace.jpl.nasa.gov/dsn/
scientific data. Programs such as
[4] http://www.space.com/searchforlife/
Voyager have been operating long
past their original mission [5]http://www.spacetoday.org/SolSys/DeepS
termination date. They also need paceNetwork/DeepSpaceNetwork.
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