Data and software resources at the Satellite Situation Center
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Abstract
The Satellite Situation Center (SSC) is a unit of the National Space Science Data Center at GSFC. A key goal of SSC is "to allow prediction of advantageous positions for a spacecraft, relative to: (i) magnetospheric or interplanetary features, (ii) the position of other spacecraft, or (iii) the position of ground facilities. The Center resources include data and software for plotting spacecraft orbits. The software emphasizes Earth-centered orbtts, but heliocentric displays are also supported. Detailed listings of key orbit characteristics as well as graphical output may be generated. Pre-computed mes with listings of wide interest are available online in a publicly accessible accounL Programs " are executed by SSC staff on request, but in the future will be available as portable software or executed remotely by users via network connections. Support to nonU. S. users is provided through the World Data Center A for Rockets and Satellites, co-located at NSSDC. The capabilities of several programs currently in use at the Center are illustrated. Finally, remote access to the Center is discussed.
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References
FAIRFIELD, D. H. 1971. Average and unusual locations of the earth's magnetopause and bow shock. JGR, 76, 6700-6716. DOI: https://doi.org/10.1029/JA076i028p06700
FAIRFIELD, D. H., 1980. A statistical determination of the shape and position of the geomagnetic neutral sheet. JGR, 85, 775-780. DOI: https://doi.org/10.1029/JA085iA02p00775
MEAD, G. D. and D. H. FAIRFIELD, 1975. A Quantitative Magnetospheric Model Derived from Spacecraft Magnetometer Data. JGR, 80, 523-534. DOI: https://doi.org/10.1029/JA080i004p00523
OLSON, W. P. and K. A. PFITZER, 1974. A Quantitative Model of the Magnetospheric Magnetic Field. JGR, 79, 3739-3748. DOI: https://doi.org/10.1029/JA079i025p03739
SIBECK, D. G., R. E. LOPEZ and E. C. ROELOF, 1991. Solar Wind Control of the Magnetopause Shape, Location and Motion. JGR, 96, 5489. DOI: https://doi.org/10.1029/90JA02464
SUGIURA, M. and J. I. VETTE, 1977. The IMS Satellite Situation Center. EOS Transactions of the American Geophysical Union, 58, 70-74. DOI: https://doi.org/10.1029/EO058i002p00070
TEAGUE, M. J., D. M. SAWYER and J. I. VETTE., 1982. The Satellite Situation Center. In: The IMS Source Book. Guide to the International Magnetospheric Study Data Analysis, C. T. Russell and D. J. Southwood, Eds., American Geophysical Union, Washington, D. C., U.S.A., pp. 112-116. DOI: https://doi.org/10.1029/SP020p0112
TSYGANENKO, N. A., 1987. Global Quantitative Models of the Geomagnetic Field in Cislunar Magnetosphere for Different Disturbance Levels. Planet. Space Sci., 35, 1347-1358. DOI: https://doi.org/10.1016/0032-0633(87)90046-8
TSYGANENKO, N. A., 1989. A Magnetospheric Magnetic Field Model with a Warped Tail Current Sheet. Planet. Space Sci., 37, 5-20. DOI: https://doi.org/10.1016/0032-0633(89)90066-4
VETTE, J. I., R. H. HILBERG and M. J. TEAGUE, 1976. Identification of Satellites Possibly Active During the IMS and their Orbital Configurations. In: The Scientific Satellite Programme During the International Magnetospheric Study. Knott and Battrick, Eds., D. Reidel Publishing Company, Dordrecht-Holland, pp. 45-59. DOI: https://doi.org/10.1007/978-94-010-1892-0_3