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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 12.

Obstructions to SPAN-B’s FOV. The inner boundary of the instrument’s full, unobstructed FOV is shown by the beige boundary, within which the instrument does not measure electrons. The spacecraft intrusions to the SPAN-B FOV are substantially greater than SPAN-Ae and are shown in blue, including Sun sensors, solar panels, fuel filling ports, FIELDS antennas, hi-gain antenna, and more. An estimate of the actual blockage, thermal blankets included, is shown in gray.

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