Still, at altitudes above roughly 80 kilometers (50 miles) lunar tides have been detected in winds, temperature,
airglow emissions and a number of ionospheric parameters.
Not exact matches
Fundamental experimental data were derived from the observations of
airglows by the Spectroscopy for Investigation of Characteristics of the Atmosphere of Mars (SPICAM) instrument on - board Mars Express: while NO is useful to constrain dynamics around the 100 km level (Gagné et al. 2013), CO and CO2 + UV
emissions allow the direct monitoring of the efficiency of ionization processes (Stiepen et al. 2015).
A similar scheme applies to the NO
airglow UV
emission, ultimately generated after the UV dissociation of CO2 and N2 at the dayside (Stiepen et al. 2013).