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Box 47

 Container

Contains 15 Results:

Fortran Coding Forms, n.d.

 File — Box: 47, Folder: 11
Scope and Contents From the Series:

This series includes early SH printouts, calculations, and Fortran computer runs such as Betulia ephemeris, Icarus ephemerides, Geographos, planetary coordinates, and two-body problems.

Much of the computer printouts were created by Gary R. Smith, who received his Ph.D. in astrodynamics at UCLA in 1972 from Herrick.

Dates: Other: n.d.

Computer Card Decks, n.d.

 File — Box: 47, Folder: 12-14
Scope and Contents From the Series:

This series includes early SH printouts, calculations, and Fortran computer runs such as Betulia ephemeris, Icarus ephemerides, Geographos, planetary coordinates, and two-body problems.

Much of the computer printouts were created by Gary R. Smith, who received his Ph.D. in astrodynamics at UCLA in 1972 from Herrick.

Dates: Other: n.d.

Computer Card Decks: Orient (Elements), [Ephe AA], n.d.

 File — Box: 47, Folder: 15
Scope and Contents From the Series:

This series includes early SH printouts, calculations, and Fortran computer runs such as Betulia ephemeris, Icarus ephemerides, Geographos, planetary coordinates, and two-body problems.

Much of the computer printouts were created by Gary R. Smith, who received his Ph.D. in astrodynamics at UCLA in 1972 from Herrick.

Dates: Other: n.d.

Computer Card Decks: Stats, n.d.

 File — Box: 47, Folder: 16
Scope and Contents From the Series:

This series includes early SH printouts, calculations, and Fortran computer runs such as Betulia ephemeris, Icarus ephemerides, Geographos, planetary coordinates, and two-body problems.

Much of the computer printouts were created by Gary R. Smith, who received his Ph.D. in astrodynamics at UCLA in 1972 from Herrick.

Dates: Other: n.d.

Notes, 1971, 1972

 File — Box: 47, Folder: 17
Scope and Contents From the Series:

This series includes early SH printouts, calculations, and Fortran computer runs such as Betulia ephemeris, Icarus ephemerides, Geographos, planetary coordinates, and two-body problems.

Much of the computer printouts were created by Gary R. Smith, who received his Ph.D. in astrodynamics at UCLA in 1972 from Herrick.

Dates: Other: 1971, 1972