Space Science Reviews

, Volume 115, Issue 1–4, pp 1–70 | Cite as

Cassini Radio Science

  • A. J. Kliore
  • J. D. Anderson
  • J. W. Armstrong
  • S. W. Asmar
  • C. L. Hamilton
  • N. J. Rappaport
  • H. D. Wahlquist
  • R. Ambrosini
  • F. M. Flasar
  • R. G. French
  • L. Iess
  • E. A. Marouf
  • A. F. Nagy
Article

Abstract

Cassini radio science investigations will be conducted both during the cruise (gravitational wave and conjunction experiments) and the Saturnian tour of the mission (atmospheric and ionospheric occultations, ring occultations, determinations of masses and gravity fields). New technologies in the construction of the instrument, which consists of a portion on-board the spacecraft and another portion on the ground, including the use of the Ka-band signal in addition to that of the S- and X-bands, open opportunities for important discoveries in each of the above scientific areas, due to increased accuracy, resolution, sensitivity, and dynamic range.

Keywords:

atmospheres Cassini gravitational fields gravitational waves general relativity ionospheres occultations planetary rings radio science Saturn Titan 

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Copyright information

© Kluwer Academic Publishers 2004

Authors and Affiliations

  • A. J. Kliore
    • 1
  • J. D. Anderson
    • 1
  • J. W. Armstrong
    • 1
  • S. W. Asmar
    • 1
  • C. L. Hamilton
    • 1
  • N. J. Rappaport
    • 1
  • H. D. Wahlquist
    • 1
  • R. Ambrosini
    • 2
  • F. M. Flasar
    • 3
  • R. G. French
    • 4
  • L. Iess
    • 5
  • E. A. Marouf
    • 6
  • A. F. Nagy
    • 7
  1. 1.Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadenaUSA
  2. 2.Istituto di Radioastronomia CNRBolognaItaly
  3. 3.NASA-Goddard Space Flight CenterGreenbeltUSA
  4. 4.Wellesley CollegeWellesleyUSA
  5. 5.Università di Roma ‘La Sapienza’RomaItaly
  6. 6.San Jose State UniversityOne Washington SquareSan JoseUSA
  7. 7.University of MichiganAnn ArborUSA

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