In 2005, astrobiologist Chris McKay argued that if methanogenic life did exist on the surface of Titan, it would likely have a measurable effect on the mixing ratio in the Titan troposphere : levels of hydrogen and acetylene would be measurably lower than otherwise expected.
32.
:" [ calculate ] the time-dependent change in CO2 mixing ratio from a given anthropogenic emission rate, [ and with that ] the time-dependent difference in mixing ratio resulting from two different emission levels by subtracting results from the equation solved twice.
33.
:" [ calculate ] the time-dependent change in CO2 mixing ratio from a given anthropogenic emission rate, [ and with that ] the time-dependent difference in mixing ratio resulting from two different emission levels by subtracting results from the equation solved twice.
34.
The " Mollier " i "-" x " " ( Enthalpy-Humidity Mixing Ratio ) diagram, developed by Richard Mollier in 1923, is an alternative psychrometric chart, preferred by many users in Scandinavia, Eastern Europe, and Russia.
35.
The fluid ( s ) will evaporate or condense until the actual concentrations of each gas is equal to the fluid's vapor pressure for that gas ( which may itself change during the process because evaporation / condensation can affect the temperature and fluid mixing ratio ).
36.
As a result, absolute humidity in chemical engineering may refer to mass of water vapor per unit mass of dry air, also known as the " mass mixing ratio " ( see " specific humidity " below ), which is better suited for heat and mass balance calculations.
37.
Lattice constants of the compounds also tend to be different, and the lattice mismatch against the substrate, dependent on the mixing ratio, causes defects in amounts dependent on the mismatch magnitude; this influences the ratio of achievable radiative / nonradiative recombinations and determines the luminous efficiency of the device.
38.
Hydrocarbons heavier than methane are present in a relatively narrow layer between 160 and 320 km in altitude, corresponding to the pressure range from 10 to 0.1 mbar and temperatures from 100 to 130 K . The most abundant stratospheric hydrocarbons after methane are acetylene and ethane, with mixing ratios of around 10 " 7.
39.
DISR was developed at the Lunar and Planetary Laboratory at the University of Arizona under the direction of Martin Tomasko, with several European institutes contributing to the hardware . " The scientific objectives of the experiment fall into four areas including ( 1 ) measurement of the solar heating profile for studies of the thermal balance of Titan; ( 2 ) imaging and spectral reflection measurements of the surface for studies of the composition, topography, and physical processes which form the surface as well as for direct measurements of the wind profile during the descent; ( 3 ) measurements of the brightness and degree of linear polarization of scattered sunlight including the solar aureole together with measurements of the extinction optical depth of the aerosols as a function of wavelength and altitude to study the size, shape, vertical distribution, optical properties, sources and sinks of aerosols in Titan s atmosphere; and ( 4 ) measurements of the spectrum of downward solar flux to study the composition of the atmosphere, especially the mixing ratio profile of methane throughout the descent ."
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