High resolution global imaging from Polar is a critical element for determining solar influenced controls of the upper atmosphere
Global variations in energetic particle precipitation and global variations in the atmospheric O/N2 ratio at 100-300 km altitude.
PIXIE: auroral X-rays quantify global >5 keV electron precipitation
UVI: auroral UV (130.4, 135.6, 140-160, 160-175, 175-190 nm)
VIS: auroral visible & UV (130.4, 391.4, 557.5, 630.0, 656.3, 732.0 nm)
Swaths of nitric oxide density in the 100-200 km altitude lower thermosphere.
UVS: auroral UV (215, 237 nm)
Ring current decay precipitates energetic O and H. On reaching the atmosphere, neutral O ionizes again from collisions, and then radiatively recombines yielding the O emission. Here, the O/N2 ratio is drastically reduced during strong activity. Because N2 is relatively stable, oxygen outflow into the magnetosphere probably caused most of the variation.
Interpretation and Implications:
Separation of natural and human-induced effects on the abundance of stratospheric ozone and odd nitrogen species require understanding of the natural processes leading to the formation and destruction of NOx and Ox.
POLAR, together with SAMPEX and SNOE shows how auroral and geomagnetic activity have a significant impact on Earth's atmospheric chemistry during major space weather storms.
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