The objective of this radio science investigation is to determine the density, turbulence spectrum, and velocity of the coronal plasma in the acceleration regime of the solar wind. Dual-frequency ranging and Doppler data are recorded during phases of the ULYSSES superior conjunction using the spacecraft transmitters and the NASA DSN.
Version:2.0.0
The objective of this radio science investigation is to determine the density, turbulence spectrum, and velocity of the coronal plasma in the acceleration regime of the solar wind. Dual-frequency ranging and Doppler data are recorded during phases of the ULYSSES superior conjunction using the spacecraft transmitters and the NASA DSN.
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Michael.K.Bird |
Information about the Coronal Sounding (radio science) (SCE) experiment on the Ulysses mission.