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It is found that the lidar-observed temperatures are in qualitative agreement with the temperature observed by satellites, though quantitatively there are significant differences.
(b) Magnetic field intensity, electron temperature observed by ESA, solar wind ion temperature observed by IEA and reflected ion temperature observed by IMA.
The experiment confirmed that transitory baffle heating accounted for the background bias found in the brightness temperature observed by LIR.
The effect of temperature observed by different authors demonstrates different degrees of enhancement for the same volume fraction.
This study compares the electron density and temperature observed by the CHAMP satellite and those predicted by the International Reference Ionosphere (IRI) model.
Though the temperatures in this study did not meet any of the international requirements, they were higher than the maximum 45 °C temperature observed by Kala et al. (2012).
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Nee et al. (2002) showed that the observed temperatures over Gadanki are higher than the temperatures observed by HALOE onboard UARS.
Lidar-observed temperatures, over both the locations, are compared with the temperatures observed by SABER (Sounding of the Atmosphere using Broadband Emission Radiometry; onboard TIMED (Thermosphere Ionosphere Mesosphere Energetics and Dynamics)) and HALOE (Halogen Occultation Experiment; onboard UARS (Upper Atmosphere Research Satellite)).
Even if the temperatures observed by the STScI team are the lowest seen for microbe activity, he says, the critical factor for martian life would still be liquid water--something not yet confirmed by NASA spacecraft.
Since the contraction (Tc) and re-solidification (Tr) temperatures observed by Khan (1985) did not change, while the reported softening temperature (Ts) plummeted with the increase of CO2 pressure; we may conclude that the "softening effect" was subtle and had to be determined by either elimination of the baseline drift or its stabilization and baseline subtraction.
With pressure balance between the tail lobe and plasma sheet, magnetic field intensity in the tail lobe is derived as B lobe= B 2+2μ 0 n k B (T i +T e ))1/2, where B,n,T i, and T e are local magnetic field intensity, plasma density, ion, and electron temperatures observed by Geotail in the current sheet, respectively.
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