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Inconspicuous Solar Polar Coronal X-Ray Jets as the Source of Conspicuous Hinode/EUV Imaging Spectrometer Doppler Outflows

  • Authors: Alphonse C. Sterling, Conrad Schwanitz, Louise K. Harra, Nour E. Raouafi, Navdeep K. Panesar, Ronald L. Moore

Alphonse C. Sterling et al 2022 The Astrophysical Journal 940 .

  • Provider: AAS Journals

Caption: Figure 1.

EIS-observed Doppler outflow events for the five events studied here, in the Fe XII 195.12 Å emission line. These are the first five events studied in Schwanitz et al. (2021), with the event number (which also corresponds to the event numbers of this paper) given in the upper right of each panel, and with each event’s date and time of the center of the Doppler outflow observations given at the top of each panel in DD-MM-YYYY HH:MM format. Deep blue features inside the contours represent observed outflows in excess of Doppler velocity −6 km s−1. See Section 2 and Schwanitz et al. (2021) for other details.

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