This Pioneer 11 UV photometer data set contains daily averages of the spin-averaged short and long wavelength channels from
April 6, 1973 onward. These data are used to study the interaction of the solar wind with the interstellar medium by measurements of spatial and temporal
variations of the intensity of backscattered solar Lyman alpha emission at 1216 A and of the solar Helium line at 584 A.
Version:2.2.2
This Pioneer 11 UV photometer data set contains daily averages of the spin-averaged short and long wavelength channels from
April 6, 1973 onward. These data are used to study the interaction of the solar wind with the interstellar medium by measurements of spatial and temporal
variations of the intensity of backscattered solar Lyman alpha emission at 1216 A and of the solar Helium line at 584 A.
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Darrell.L.Judge |