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The Solar Probe ANalyzers—Electrons on the Parker Solar Probe

  • Authors: Phyllis L. Whittlesey, Davin E. Larson, Justin C. Kasper, Jasper Halekas, Mamuda Abatcha, Robert Abiad, M. Berthomier, A.W. Case, Jianxin Chen, David W. Curtis, Gregory Dalton, Kristopher G. Klein, Kelly E. Korreck, Roberto Livi, Michael Ludlam, Mario Marckwordt, Ali Rahmati, Miles Robinson, Amanda Slagle, M.L. Stevens, Chris Tiu, and J.L. Verniero

2020 The Astrophysical Journal Supplement Series 246 74.

  • Provider: AAS Journals

Caption: Figure 11.

Obstructions to SPAN-Ae’s FOV. The instrument’s full, unobstructed FOV is contained inside the beige rectangular area, with un-blanketed spacecraft intrusions to the FOV show in blue. The mag boom is seen at the left (10°–60°, −15°) and the heat shield and FIELDS Antenna are seen radiating from the sunward direction (center). At (165°, 40°), the solar panel is indicated. An estimate of the actual blockage, thermal blankets included, is shown in gray.

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