2019
DOI: 10.1029/2019gl086145
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Subauroral Green STEVE Arcs: Evidence for Low‐Energy Excitation

Abstract: Subauroral emissions known as STEVEs (Strong Thermal Emission Velocity Enhancements) are sometimes accompanied by green arcs containing magnetic field‐aligned “picket fence” structures. In a newly published spectrum of a green picket fence arc Gillies et al. (2019, https://doi.org/10.1029/2019GL083272) showed that the visible emission in such arcs is mostly OI 557.7 nm with minimal N2+ 1N. This finding is consistent with the color ratios found in digital camera photos (Mende & Turner, 2019, https://doi.org/10.… Show more

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Cited by 39 publications
(80 citation statements)
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“…One other interesting result in their theories is that they 10.1029/2020GL088980 predict a parallel electric field on order of a fraction of 1 mV/m, over an altitudinal range of several tens of km between the ionospheric E and lower F region (see, e.g., Figure 6 in Noël et al, 2000). Assuming an average E // of~0.2 mV/m that spans an altitude range of~50 km, the resulting electron acceleration would be sufficient to excite the 557.7 nm green line (~4.19 eV) and N2 1PG emissions (~7.35 eV) (Mende et al, 2019), yet not enough to excite the N 2 + 1 N 427.8 nm emission (~18.75 eV). This is consistent with the absence of blue-line 427.8 nm emissions in the Picket Fence spectra (Gillies et al, 2019;Mende et al, 2019).…”
Section: Summary and Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…One other interesting result in their theories is that they 10.1029/2020GL088980 predict a parallel electric field on order of a fraction of 1 mV/m, over an altitudinal range of several tens of km between the ionospheric E and lower F region (see, e.g., Figure 6 in Noël et al, 2000). Assuming an average E // of~0.2 mV/m that spans an altitude range of~50 km, the resulting electron acceleration would be sufficient to excite the 557.7 nm green line (~4.19 eV) and N2 1PG emissions (~7.35 eV) (Mende et al, 2019), yet not enough to excite the N 2 + 1 N 427.8 nm emission (~18.75 eV). This is consistent with the absence of blue-line 427.8 nm emissions in the Picket Fence spectra (Gillies et al, 2019;Mende et al, 2019).…”
Section: Summary and Discussionmentioning
confidence: 99%
“…With the TREx RGB camera, it is particularly straight forward to identify the Picket Fence. Besides their characteristic morphological features, the Picket Fence exists predominantly in the green channel and shows only a faint imprint (presumably from N2 1PG; see Mende et al, 2019) in the red channel, yet nothing on the blue channel. Due to their primarily green nature, only the green channel of the RGB image was used for the Picket Fence structures.…”
Section: Apparent Motion Of the Picket Fencementioning
confidence: 99%
“…A picket fence was observed at a location magnetically conjugate to a Defense Meteorological Satellite Program observation of detached precipitation and far ultraviolet aurora (Nishimura et al, 2019). However, precipitation should create N + 2 first negative emissions, while there is no evidence for this emission in the picket fence spectrum observed by Gillies et al (2019) (Mende et al, 2019). The horizontal structuring (∼18-km spacing) and magnetic field-aligned structure of the picket fence are suggestive of precipitation and stand in contrast to the purple arc, which appears much less structured.…”
Section: 1029/2020gl087102mentioning
confidence: 95%
“…However, based on the limited evidence thus far obtained, it is also possible that the streaks and the picket fence are not causally connected but, rather, represent two distinct responses to the same free energy source. Mende et al (2019) conjectured that the magnetic field-aligned features could be produced by wave heating induced by the extreme electric fields in the SAID region (Streltsov & Mishin, 2003). Fine-scale green emissions at lower conjugate altitudes could be excited by these same extreme fields.…”
Section: Formation Of Field-aligned Features From Point Sourcesmentioning
confidence: 99%
“…The whitish color is attributed to lower‐altitude events, where the metastable O ( 1 D ) state responsible for the red line component is collisionally quenched (Liang et al, 2019). The companion picket fence region has been found to be predominantly oxygen 557.7‐nm green line, with a trace contribution from N 2 first positive emissions (Mende et al, 2019). The lack of emissions from higher energy N2+ transitions has argued against precipitating magnetospheric electrons as a source of the green features (Mende et al, 2019), although the role of precipitation in STEVE remains a subject of debate (Nishimura et al, 2019).…”
Section: Introductionmentioning
confidence: 99%