The Mysterious Green Streaks Below STEVE
The Mysterious Green Streaks Below STEVE
复制标题
史蒂夫脚下神秘的绿色条纹
DOI:
10.1029/2020av000183
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发表时间:
2020
期刊:
影响因子:
8.4
通讯作者:
Wang, Jun
中科院分区:
文献类型:
--
作者:
Semeter, Joshua;Hunnekuhl, Michael;MacDonald, Elizabeth;Hirsch, Michael;Zeller, Neil;Chernenkoff, Alexei;Wang, Jun
Strong thermal emission velocity enhancement (STEVE) is an optical phenomenon of the subauroral ionosphere arising from extreme ion drift speeds. STEVE consists of two distinct components in true‐color imagery: a mauve or whitish arc extended in the magnetic east–west direction and a region of green emission adjacent to the arc, often structured into quasiperiodic columns aligned with the geomagnetic field (the “picket fence”). This work employs high‐resolution imagery by citizen scientists in a critical examination of fine‐scale features within the green emission region. Of particular interest are narrow “streaks” of emission forming underneath field‐aligned picket fence elements in the 100‐ to 110‐km altitude range. The streaks propagate in curved trajectories with dominant direction toward STEVE from the poleward side. The elongation is along the direction of motion, suggesting a drifting point‐like excitation source, with the apparent elongation due to a combination of motion blur and radiative lifetime effects. The cross‐sectional dimension is <1 km, and the cases observed have a duration of20–30 s. The uniform coloration of all STEVE green features in these events suggests a common optical spectrum dominated by the oxygen 557.7‐nm emission line. The source is most likely direct excitation of ambient oxygen by superthermal electrons generated by ionospheric turbulence induced by the extreme electric fields driving STEVE. Some conjectures about causal connections with overlying field‐aligned structures are presented, based on coupling of thermal and gradient‐drift instabilities, with analogues to similar dynamics observed from chemical release and ionospheric heating experiments.
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影响因子:
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作者:
M. Zettergren;J. Semeter;P. Blelly;M. Díaz
通讯作者:
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影响因子:
5.2
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DOI:
10.1016/j.jastp.2004.07.006
发表时间:
2004
影响因子:
1.9
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影响因子:
5.2
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通讯作者:
D. Eurich