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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 5.

Zoomed-in views of Table 1 event 4, at AIA and XRT wavelengths. The basic layout of the panels is as described in Figure 3. Green arrows show a cool-material erupting minifilament, at about the same time in (a) and (e), and at a later time in (g) and (k). Blue arrows in (i) and (l) show a brightening similar to a JBP. White arrows in (h) and (i) point to a faint feature that resembles a coronal-jet spire. The accompanying animation shows the evolution of these panels, covering 2020 March 7 over 14:00–14:48 UT. The entire movie runs for 3 s. From Table 1 the center of the blueshift contour is at about 14:29 UT, at which time the movies still show apparent outflow.

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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