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\title{\LARGE \bf
Prospects for a Next-Generation Deep-Space Network
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%\author{ \parbox{3 in}{\centering Huibert Kwakernaak*
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% \parbox{3 in}{ \centering Pradeep Misra**
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\author{Ms. Renu Kesharwani${ M.Tech Computer Science}$% <-this % stops a space
\thanks{I would like to Express my Thanks to }% <-this % stops a space
\thanks{$^{}$ Mr.Darmendra Sir Faculty of United college of Engineering and Research ,Allahabad U.P.
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\begin{abstract}
When it comes to making a long-distance call, it's hard to top NASA's Deep Space Network. It’s the largest and most sensitive scientific telecommunications system in the world.
so our objective is (1) To archive knowledge of operations procedures.
( 2) provide a capability to assist in execution monitoring;
(3) Provide a capability for automatically
Constructing the plan to be executed and monitored.
This paper describes the application area of DSN
antenna operations, describes the plan to reduce the distance.
\end{abstract}
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\section{INTRODUCTION}
The Deep Space Network - or DSN - is NASA’s international array of giant radio antennas that supports interplanetary spacecraft missions, plus a few that orbit Earth. The DSN also provides radar and radio astronomy observations that improve our understanding of the solar system and the larger universe.
The antennas of the Deep Space Network are the indispensable link to explorers venturing beyond Earth. They provide the crucial connection for commanding our spacecraft and receiving their never before seen images and scientific information on Earth, propelling our understanding of the universe, our solar system and ultimately, our place within it.
\section{Functional area of Deep Space network}
\subsection{Domain Area of DSN}
The Deep Space Network, or DSN, is much more than a collection of big antennas. It is a powerful system for commanding, tracking and monitoring the health and safety of spacecraft at many distant planetary locales. The DSN also enables powerful science investigations that probe the nature of asteroids and the interiors of planets and moons
\subsection{
DSN Complexes}
Each of the three Deep Space Network, or DSN, sites has multiple large antennas and is designed to enable continuous radio communication between several spacecraft and Earth. All three complexes consist of at least four antenna stations, each equipped with large, parabolic dish antennas and ultra-sensitive receiving systems capable of detecting incredibly faint radio signals from distant spacecraft.
The DSN's large antennas are focusing mechanisms that concentrate power when receiving data and when transmitting commands. The antennas must point very accurately towards the spacecraft, because an antenna can "see" only a tiny portion of the sky – not unlike looking at the sky through a soda straw.
\section{Telecommunications Deep Space Network }
The main terminal of the DSN is located at JPL (Jet PropulsionLaboratory) headquarters in Pasadena, California. There are three primary antennas, spaced equally on a great circle that slants around the world. All three are large paraboloid (dish) antennasthat can be used for transmitting and receiving signals over a wide range of radio frequencies. One antenna is located in California, another is in Spain, and another is in Australia. Theantennas are located in such a way that all existing operational spacecraft can be monitored and controlled, and communications maintained with them, almost 100 percent of the time. This is true of both earth-orbiting satellites and interplanetary space vehicles.
Signals transmitted and received by DSN equipmentinclude satellite control and telemetry, e-mail (including text,graphics, video, programs, and sound attachments), communicationswith the Space Shuttles, and radio-frequency emanations fromdistant celestial objects.
\subsection{Radio Astronomy Deep Space Network - Radio Astronomy}
Radio Astronomy and the role of the DSN in exploring the Universe using radio waves. Color illustrations on the front show radio images of a galaxy and of Jupiter's radiation belts. The reverse side describes how we can use radio astronomy to further our understanding of the Solar System and the Universe
\subsection{Speaking in Phases - a Classroom Activity}
\begin{itemize}
\item How do spacecraft put actual information into the radio signals they send back to Earth? Beat out rhythms on drums or desks and send messages using the same principles used in space exploration.
\item Avoid combining SI and CGS units, such as current in amperes and magnetic field in oersteds. This often leads to confusion because equations do not balance dimensionally. If you must use mixed units, clearly state the units for each quantity that you use in an equation.
\item Related disciplines: physics (EM wave modulation), math (binary codes), space technology, music!
Activity: Entire class, indoor, game-type demonstration.
\end{itemize}
\subsection{Long-Range Planning}
While there are many similarities between the mid- and
long-range planning and scheduling functions for DSN,
there are also significant differences. Underlying both is
the set of current and future DSN assets, including antennas
and equipment, some coming into service and others
being decommissioned. Both are based on DSN usage requirements
from a varying mission set with a wide range of
time-dependent tracking and navigation needs. Both are
charged with arriving at an ultimately feasible allocation of
DSN resources by balancing user needs and resolving periods
of resource contention.
\subsection{long-range planning significant
differences from mid-range:}
\begin{itemize}
\item unpredictable spacecraft locations for some missions
and trajectory types, leading to uncertainties
in visibility times from the different DSN antennas.
\item unknown science targets beyond some time horizon
in the future
\item uncertainties in the mission set, due to funding
changes, launch date changes, or mission extensions.
\item In your paper title, if the words that uses can accurately
replace the word using, capitalize the u; if not, keep
using lower-cased.
\item Be aware of the different meanings of the homophones
affect and effect, complement and compliment, discreet
and discrete, principal and principle.
\item The prefix non is not a word; it should be joined to the
word it modifies, usually without a hyphen.
\item The abbreviation i.e. means that is, and the abbreviation
e.g. means for example.
\item A graph within a graph is an inset, not an insert. The
word alternatively is preferred to the word alternately
(unless you really mean something that alternates).
\end{itemize}
\section{Space Networking:}
Future missions will make more use of multiple spacecraft and planetary
relays. If we continue to operate as we do now, the human cost of managing data flow will become
prohibitive. Disruption-Tolerant Networking (DTN), an advanced store and forward protocol,
extends the services provided by the terrestrial Internet into deep space and can recover from
outages due to weather, eclipses, etc. without loss of data. Information sent from a spacecraft can
automatically route itself through other science spacecraft, relays, and DSN antennas. At each
stage, custody of the information is updated so that the storage on the originating spacecraft can
be re-allocated to new science observations. DTN has been demonstrated with the EPOXI spacecraft
and it is in a fast development at NASA. Negotiations are also underway to make DTN an
international standard.
\subsection{Radio and Radar Science}
A powerful radar transmitter exists at the Gold stone 70m antenna for studies of solar system objects,
with the reflected signal being received either at that antenna, other antennas at Goldstone,
radio astronomy observatories, or some combination. Signals transmitted from the Arecibo radar
can also be received at the Gold stone 70m antenna. Many solar system missions use this DSN
radar facility to observe their target objects, both to enhance mission science and for engineering
purposes (e.g., landing site characterization). Radar studies of near-Earth asteroids provide precision
trajectory data and high-resolution structural information, which are key to predicting and
mitigating possible threats of Earth collision. Enhancements of the radar system are possible over
the next decade.
\subsection{Optical Communications:}
Optical communications is, perhaps, the most exciting and game changing
development that will occur over the next decade. NASA is committed to the operational
use of optical communications within 10 years. As such, NASA plans to fund the development
of a deep space optical terminal (DOT). NASA has a dedicated 1m optical communications
ground station at Table Mountain Observatory in California. This facility has already been
used for experiments with foreign Earth-orbiting spacecraft optical tests.
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\centering
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The existing DSN plan will address the requirements implied by NASA’s current model of the
future mission set (the AMPM). Substantial additional capability is possible, if desired and advocated
by the science community. We are seeking the Committee’s consideration of the following
as functions of time.
\section{CONCLUSIONS}
The DSN stands ready to play its part enabling future planetary missions. Plans already in place
will result in significant improvements – allowing scientists to expand their scientific horizons
and develop new mission concepts. NASA looks forward to working with the science community
to ensure appropriate investments are made to maximize the productivity of the exploration
of the solar system.The most important aspect of this technology is how we use all this technology that was invented or used in these facilities for commercial use like our cell phones, radar guns and GPS devices. Development of transport protocol for deep space communication is a highly challenging task. The research challenges and issues related to this field have been brought out in this paper.
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\section*{ACKNOWLEDGMENT}
Authors would like to thanks , Mr.Dharmendra Sir Head Of Department United College of Engineering and Research for their constant encouragement towards the realization of this work.
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\begin{thebibliography}{99}
\bibitem{c1} International Journal of Computer Applications (0975 – 8887)
Volume 31– No.8, October 2011
\bibitem{c2} Planning for Deep Space Network Operations
Randall Hill, Jr., Steve Chien, Crista Smyth, Kristina Fayyad, Trish Santos
Jet Propulsion Laboratory
California Institute of Technology.
\bibitem{c3} Automating Mid- and Long-Range Scheduling for the NASA Deep Space Network
Mark D. Johnston* and Daniel Tran*
*Jet Propulsion Laboratory, California Institute of Technology
4800 Oak Grove Drive, Pasadena CA USA 91109
\bibitem{c4} A Survey of Transport Protocols for Deep Space
Communication Networks
International Journal of Computer Applications (0975 – 8887)
Volume 31– No.8, October 2011
\bibitem{c5} H. Balakrishnan, V. N. Padmanabhan and R. H. Katz, “The Effects of Asymmetry on TCP Performance," Proc. ACM MOBICOM Hungary, pp. 77-89, September 1997.
\bibitem{c6} M.Allman, D.Glover, and L.Sanchez, “Enhancing TCP over satellite channels using standard mechanisms,” IETF, RFC 2488, January 1999.
\bibitem{c7}S.Burleigh, A.Hooke, et al., “Delay-Tolerant Networking: An Approach to Interplanetary Internet,” IEEE Communications Magazine, Vol.41, Issue 6, pp. 128-136, June 2003.
\bibitem{c8} O. B. Akan, J.Fang and I. F. Akyildiz, “TP-Planet: A Reliable Transport Protocol for InterPlaNetary Internet”, IEEE/SAC, Vol. 22, No. 2, pp 348-61, February 2004.
\bibitem{c9} M. Young, The Techincal Writers Handbook. Mill Valley, CA: University
Science, 1989.
\end{thebibliography}
\end{document}