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References

  • Armstrong, J., and R. Woo (1980), Contribution to Starprobe report, JPL Internal Memo. 3331-80-070, Jet Propul. Lab., Pasadena, Calif., 15 Dec.
  • Armstrong, J. W., and R. Woo (1981a), Solar wind motion within 30 Ro: Spacecraft radio scintillation observations, Astron. Astrophys., 103, 415421.
  • Armstrong, J., and R. Woo (1981b), Temporal autocorrelation functions and fluctuation power spectra of amplitude scintillations: Starprobe-Earth communications geometry, JPL Internal Publ. IOM 3333-81-048, Jet Propul. Lab., Pasadena, Calif., 29 May .
  • Coles, W. A., and J. K. Harmon (1989), Propagation observations of the solar wind near the Sun, Astrophys. J., 337, 10231034.
  • Coles, W. A., W. Liu, J. K. Harmon, and C. L. Martin (1991), The solar wind density spectrum near the Sun: Results from Voyager radio measurements, J. Geophys. Res., 96, 17451755.
  • Coles, W. A., R. R. Grall, M. T. Klinglesmith, and G. Bourgois (1995), Solar cycle changes in the level of compressive microturbulence near the Sun, J. Geophys. Res., 100, 17,06917,080.
  • Feria, Y., M. Belongie, T. McPheeters, and H. Tan (1997), Solar scintillation effects on telecommunication links at Ka-band and X-band, Telecommun. Data Acquisition Prog. Rep. 42-129, Jet Propul. Lab., Pasadena, Calif., 15 May .
  • Fremouw, E. J., R. L. Leadabrand, R. C. Livingston, M. D. Cousins, C. L. Rino, B. C. Fair, and R. A. Long (1978), Early results for the DNA wideband satellite experiment: Complex signal scintillation, Radio Sci., 13(1), 167187.
  • Fu, W., S. Han, C. Rizos, M. Knight, and A. Finn (1999), Real-time ionospheric scintillation monitoring, paper presented at 12th International Technical Meeting of the Satellite Division of the Institute of Navigation (ION GPS-99), Inst. of Navig., Nashville, Tenn.
  • Harmon, J. K., and W. A. Coles (2005), Modeling radio scattering and scintillation observations of the inner solar wind using oblique Alfvén/ion cyclotron waves, J. Geophys. Res., 110, A03101, doi:10.1029/2004JA010834.
  • Hayes, A. P., A. Vourlidas, and R. A. Howard (2001), Deriving the electron density of the solar corona from the inversion of total brightness measurements, Astrophys. J., 548, 10811086.
  • Ishimaru, A. (1978), Wave Propagation and Scattering in Random Media, vol. 2, Elsevier, New York.
  • Marians, M. (1975), Theory of scintillations due to propagation through a turbulent medium, Ph.D. dissertation, Univ. of Calif., San Diego, Calif.
  • Morabito, D. D. (2002), Ka-band and X-band observations of the solar corona acquired during the Cassini 2001 superior conjunction, paper presented at 8th Ka-Band Utilization Conference, Ist. Int. delle Commun., Baveno, Italy, 25 – 27 Sept.
  • Morabito, D. (2003), Solar corona amplitude scintillation modeling and comparison to measurements at X-band and Ka-band, IPN Prog. Rep. 42-153, Jet Propul. Lab., Pasadena, Calif.
  • Morabito, D. D., and R. Hastrup (2002), Communicating with Mars during periods of solar conjunction, 2002 IEEE Aerospace Conference: Proceedings: Big Sky, Montana, March 9–16, IEEE Press, Piscataway, N. J.
  • Morabito, D., S. Butman, and S. Shambayati (1999), The Mars Global Surveyor Ka-band link experiment (MGS/KaBLE-II), Telecommun. Mission Oper. Prog. Rep. 42-137, pp. 141, Jet Propul. Lab., Pasadena, Calif.
  • Morabito, D. D., S. Shambayati, S. Butman, D. Fort, and S. Finley (2000), The 1998 Mars Global Surveyor solar corona experiment, TDA PR 42-42, Jet Propul. Lab., Pasadena, Calif.
  • Morabito, D. D., S. Shambayati, S. Finley, D. Fort, J. Taylor, and K. Moyd (2001), Ka-band and X-band observations of the solar corona acquired during solar conjunctions of interplanetary spacecraft, paper presented at 7th Ka-band Utilization Conference, Ist. Int. delle Commun., Santa Margherita Ligure, Italy, 26 Sept.
  • Morabito, D., S. Shambayati, S. Finley, and D. Fort (2003), The Cassini May 2000 solar conjunction, IEEE Trans. Antennas Propag., 51(2), 201219.
  • Rebold, T. A., A. Kwok, G. E. Wood, and S. Butman (1994), The Mars Observer Ka-band link experiment, TDA PR 42-117, pp. 250282, Jet Propul. Lab., Pasadena, Calif.
  • Rickett, B. (1977), Interstellar scattering and scintillation of radio waves, Annu. Rev. Astron. Astrophys., 15, 479504.
  • Scott, S. L., B. J. Rickett, and J. W. Armstrong (1983), The velocity and the density spectrum of the solar wind from simultaneous three-frequency IPS observations, Astron. Astrophys., 123, 191206.
  • Woo, R. (1977), Measurements of the solar wind using spacecraft radio scattering observations, in Study of Traveling Interplanetary Phenomena, edited by M. Shea, D. Smart, and S. Wu, pp. 81100, Springer, New York.
  • Woo, R. (1995), Structure in the solar corona from radio scintillation measurements, Astrophys. Space Sci., 243(1), 97104.
  • Woo, R., and J. W. Armstrong (1979), Spacecraft radio scattering observations of the power spectrum of electron density fluctuations in the solar wind, J. Geophys. Res., 84, 72887296.
  • Woo, R., and J. W. Armstrong (1992), Observations of large-scale structure in the inner heliosphere with Doppler scintillation measurements, in Solar Wind, edited by E. Marsch, and R. Schwenn, pp. 319322, Elsevier, New York.
  • Woo, R., and R. M. Goldstein (1994), Latitudinal variation of speed and mass flux in the acceleration region of the solar wind inferred from spectral broadening measurements, Geophys. Res. Lett., 21, 8588.
  • Woo, R., F. Yang, and A. Ishimaru (1977), Probing the solar wind with radio measurements of the second moment field, Astrophys. J., 218, 557568.
  • Woo, R., J. W. Armstrong, M. K. Bird, and M. Pätzold (1995), Variation of fractional electron density fluctuations inside 40 Ro observed by Ulysses ranging measurements, Geophys. Res. Lett., 22, 329332.