From October 2012 to June 2013, Curiosity used its Tunable Laser Spectrometer (TLS) six times to search
for traces of methane in the Martian atmosphere.
Not exact matches
The main objectives
of this mission are to search
for evidence
of methane and other
trace atmospheric gases that could be signatures
of active biological or geological processes and to test key technologies in preparation
for ESA's contribution to subsequent missions to Mars.
In addition to the isotope concentration, the air bubbles trapped in the ice cores allow
for measurement
of the atmospheric concentrations
of trace gases, including greenhouse gases carbon dioxide,
methane, and nitrous oxide.
Spacecraft were not detecting all
of the spectroscopic signatures
of the gas,
for example, and ground - based observers had to contend with interference from
methane and other
trace gases in Earth's atmosphere.
The climate models as described here won't produce glacial / interglacial cycles if run
for a long time, and that is because they treat the atmospheric content
of trace IR - absorbing gases (CO2,
methane and N2O) as external forcings.
For the authors
of the paper to assess the spectral results against theory they needed to know the atmospheric profile
of temperature and humidity, as well as changes in the well - studied
trace gases like CO2 and
methane.