Figure 9 from The Solar Probe ANalyzers—Electrons on the Parker Solar Probe

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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 9.

First PSP encounter as a function of time. Top to bottom: PSP distance from the solar center Sun in solar radii; combined SPAN-E PADs for the passband at 302 eV and normalized by the average flux; the R component of the ambient magnetic field in a heliocentric reference frame in nT; summed energy spectra (SF1) from SPAN-Ae in differential energy flux units; summed energy spectra from SPAN-B in differential energy flux units. During most of the first encounter, the magnetic field is pointed sunward, and hence, the PADs for the 302 eV channel that corresponds to the sense of the electron strahl are found at 180°.

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