Image Details

Choose export citation format:

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 10.

Left panel: time-series plot of the SPAN-E mechanical attenuators being engaged in the first encounter. Top to bottom: attenuator Status, SPAN-Ae, Total Counts per accumulation period, SPAN-Ae (generated onboard instrument), Summed Energy Spectra for SPAN-Ae, Attenuator Status, SPAN-B, Total Counts per accumulation period, SPAN-B (generated onboard instrument), and Summed Energy Spectra for SPAN-B. The attenuator moves to the “In” position at approximately 0310, with ground software constructing an artificial increase in “background” electron flux thereafter. Right panel: single energy spectrum produced by SPAN-Ae before (blue) and after (red) the mechanical attenuator is engaged (same time period). An artificial increase in electron flux below approximately 25 eV is apparent.

Other Images in This Article

Show More

Copyright and Terms & Conditions