We measured maps of atmospheric water (H2O) and its deuterated form (HDO) across the
martian globe, showing strong isotopic anomalies and a significant high …

Over the past two decades there has been a vast increase in the amount and variety of
observations characterizing the thermal structure and composition of the Mars atmosphere …

We present the results of the first three‐dimensional (3‐D) simulation of the water isotope
HDO in the Martian atmosphere. This deuterated isotope of water has long been used on …

Ever since the Viking mass spectrometer failed to detect organics on the surface of Mars in
1976 (Biemann et al., 1976), hydrogen peroxide (H2O2) has been suggested as a possible …

The recent discovery of methane on Mars has led to much discussion concerning its origin.
On Earth, the isotopic signatures of methane vary with the nature of its production …

New maps of martian water vapor and hydrogen peroxide have been obtained in November–
December 2005, using the Texas Echelon Cross Echelle Spectrograph (TEXES) at the …

We propose a submillimetre-wave atmospheric emission sounding instrument, called Far-
InfraRed Experiment (FIRE), for the Japanese Martian exploration programme “Mars …

Mapping the D/H isotopic ratio across Mars provides unique insights into the evolution and
climatology of its atmosphere, and may help to identify the sources and sinks of atmospheric …

Lorentz half-width coefficients and their temperature dependence exponents for CO 2
broadening in the fundamental bands of HDO are important for reliable and accurate …

The investigation of the Martian atmosphere is of key importance for an understanding of the
planets present and past. Passive limb observations of thermal radiation at submillimeter …