| 000 | 01740cam a2200385 i 4500 | ||
|---|---|---|---|
| 001 | rnd000000000048599 | ||
| 003 | RAND | ||
| 008 | 920212s1991 cauab b 000 0 eng d | ||
| 020 | _a0833019295 | ||
| 027 | _aRAND/N-3437-JPL | ||
| 035 | _a(Sirsi) a190705 | ||
| 037 | _c$20.00 | ||
| 040 |
_aCstmoR _cCstmoR |
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| 050 | 4 |
_aQB621 _b.D38 1991 |
|
| 100 | 1 |
_aDavies, Merton E. _eauthor. |
|
| 245 | 1 | 4 |
_aThe preliminary geodetic control network of Venus / _cMerton E. Davies, Patricia G. Rogers. |
| 264 | 1 |
_aSanta Monica, CA : _bRAND, _c1991. |
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| 300 |
_axi, 17 pages : _billustrations, maps ; _c28 cm |
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| 336 |
_atext _btxt _2rdacontent |
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| 337 |
_acomputer _bc _2rdamedia |
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| 337 |
_aunmediated _bn _2rdamedia |
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| 338 |
_aonline resource _bcr _2rdacarrier |
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| 338 |
_avolume _bnc _2rdacarrier |
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| 490 | 1 |
_aA RAND note ; _v3437 |
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| 504 | _aIncludes bibliographical references (p. 17). | ||
| 520 | _aThis Note was written in preparation for the Magellan mission to Venus and presents the coordinate system adopted for the project. Control points have been identified on Venera 15, 16 pictures and 1983 Arecibo pictures, and their coordinates given in the Magellan coordinate system. Transformation matrices are presented. The control points are identified as craters, hills, or central peaks in craters. | ||
| 530 | _aAlso available on the internet via WWW in PDF format. | ||
| 588 | _aDescription based on print version record. | ||
| 650 | 0 |
_aPlanets _vMaps. |
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| 651 | 0 |
_aVenus (Planet) _vMaps. |
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| 700 | 1 |
_aRogers, Patricia G. _q(Patricia Grizzaffi) _eauthor. |
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| 710 | 2 | _aRand Corporation. | |
| 710 | 2 | _aJet Propulsion Laboratory (U.S.) | |
| 830 | 0 |
_aRand note ; _v3437. |
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| 856 | 4 | 1 |
_yOnline Access _uhttp://www.rand.org/pubs/notes/N3437/ |
| 999 |
_c599348 _d599348 |
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