J.E. Blamont

TL;DR: In this article, the vertical structure of the Martian aerosols near the northern spring equinox was analyzed using the Phobos 2 spectrometer measurements of solar occultations close to the evening terminator, and it was assumed that the dust particles are levitated by eddy mixing.

TL;DR: In this paper, the vertical profile of the ozone density in the martian atmosphere above ≈35 km altitude in the equatorial region (0°20° N latitude) near the northern spring equinox (Ls = 0°-20°).

TL;DR: The European Venus Explorer (EVE) mission described in this paper was proposed in December 2010 to ESA as an 'M-class' mission under the Cosmic Vision programme as discussed by the authors, consisting of a single balloon platform floating in the middle of the main convective cloud layer of Venus at an altitude of 55 km, where temperatures and pressures are benign (∼25°C and ∼0.5 bar).

TL;DR: In this paper, the authors derived the production rate of OH radicals QOH = 4 xsx 1028 moleculesec −1sr−1 at 0.6 AU and the lifetime of the OH radical which is τ OH = 4.5 × 104 sec.