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Title: | Space Exploration |
Notice: | Shuttle launch schedules, see Note 6 |
Moderator: | PRAGMA::GRIFFIN |
|
Created: | Mon Feb 17 1986 |
Last Modified: | Thu Jun 05 1997 |
Last Successful Update: | Fri Jun 06 1997 |
Number of topics: | 974 |
Total number of notes: | 18843 |
348.0. "Space Physics Analysis Network" by DICKNS::KLAES (Angels in the Architecture.) Fri Sep 25 1987 16:53
VNS TECHNOLOGY WATCH: [Mike Taylor, VNS Correspondent]
===================== [Nashua, NH, USA ]
SPAN
Planning for SPAN (the Space Physics Analysis Network) began in
1980, and operations commenced in 1981. SPAN was originally
oriented toward researchers in Solar Terrestial and Interplanetary
Physics, but is now expanding to serve other disciplines. SPAN is
a multimission, correlative data comparison network serving
projects and facilities of the American National Aeronautics and
Space Administration (NASA) in collaboration with the European
Space Agency (ESA). These agencies have traditionally set up data
collection networks to serve specific space missions, but SPAN is
mission independent, general purpose, low cost, and easy to
connect to. (However, it is sometimes used to support specific
missions, such as the ICE mission to the Giacobibi-Ainner comet
and the encounter with Comet Halley.) It is an operational
network in that it is not intended to promote the development of
network technology, but it is a research network in that it
provides an infrastructure for space-related research. It was not
created in order to access supercomputers, but supercomputers are
becoming more available through it.
Guidance for the networks is provided by the users through the
Data System Users Workers Group (DSUWG) and project scientists.
Direct administration is done by project managers, network
managers, and routing center managers. NASA pays for all the links
while other participating organizations pay for their own host
computers and network interfaces. Much of the original hardware,
such as the routing center computers, came from NASA.
The upper layer protocols are DECNET. The lower layers are
provided by NASA's Program Support Communications Network (PSCN)
and the NASA Packet-switch System (NPSS). PSCN is a circuit
switched network, that is, a collection of leased lines and
microwave links. NPSS consists of X.25 links, some of them over
public X.25 networks. The backbone of the network is four routing
centers at the Goddard Space Flight Center in Greenbelt, Maryland,
The Johnson Space Center in Houston Texas, the Jet Propulsion
Laboratory in Pasadena, California, and the Marshall Space Flight
Center in Huntsville, Alabama. These are connected by 56,000-bps
links to the other institutions on the network. Reliability is
becoming high.
DECNET addresses consist of 16 bits, 6 specifying an area and 10
specifying a node within the area. Since there are only 64
possible areas, management of the area numbers is very important.
Within Easynet, DEC's DECNET-based company network, all area
numbers are in use; thus direct gateways between Easynet and other
DECNETs are problematic.
There are many DECNETs other than SPAN outside of Easynet. They
cooperate in assigning area numbers, with SPAN management
providing a forum, especially for those networks interested in
joining SPAN (ESA provides a similar forum in Europe). A major
task of SPAN's routing centers is the assignment of nodes to
areas.
There are currently more than one hundred hosts connected directly
to SPAN, all of them DEC machines. Outside of NASA, there are
many participating universities and laboratories, such as the Los
Alamos National Laboratory. There are many LANs indirectly
connected to SPAN. Because other exiting DECNETs want to join
SPAN, the total number of hosts is expected to reach five hundred
within a year. There is a transatlantic X.25 link between
Marshall Space Flight Center in Huntsville, Alabama, and ESA's
Operations Centre (ESOC) in Darmstadt, West Germany. A 9,600-bps
link was installed in September from Goddard to Germany, and one
to Japan is expected by the end of the year.
{extract from Communications of the ACM, October 1986}
{contributed by Walt Lamia}
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