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Quiet-Sun Explosive Events Observed in He ii λ304 with MOSES-06
Author(s) -
Thomas Rust,
C. C. Kankelborg
Publication year - 2019
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.3847/1538-4357/ab12e2
Subject(s) - physics , astrophysics , explosive material , magnetic reconnection , context (archaeology) , jet (fluid) , redshift , doppler effect , solar flare , line (geometry) , emission spectrum , spectrograph , astronomy , extreme ultraviolet , spectral line , event (particle physics) , plasma , optics , galaxy , paleontology , laser , chemistry , geometry , mathematics , organic chemistry , quantum mechanics , biology , thermodynamics
In this paper the unique data from the Multi-Order Solar Extreme-Ultraviolet Spectrograph ( MOSES ) are used to investigate transition region explosive events in the He ii λ 304 spectral line. Particular attention is paid to two example events: one blueshifted jet and one bidirectional jet. Observations suggest that these events consist exclusively of high-velocity (∼100 km s −1 ) plasma. These two and other examples presented here exhibit a striking lack of emission in the line core. No acceleration phase is observed at the onset of either event. In total, 41 examples of explosive events are identified, including 5 blueshifted jets, 2 redshifted jets, and 10 bidirectional jets. The remaining 24 events resist simple classification, but observations indicate compact, highly Doppler-shifted emission. Event spatial scales and lifetimes are consistent with published explosive event characteristics. Data from the Michelson Doppler Imager provide magnetic context to the MOSES observations. Bidirectional jets lacking line core emission are interesting because they are predicted in models of Petschek reconnection in the transition region. 

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