Exact(7)
The atmosphere parameters (density, pressure, temperature) can be represented by an exponential model or tabulated with respect to the altitude.
These results are also compared with Reilly's analytical single scattering model [1] as well as the Monte Carlo simulated multiple scattering model [2], respectively, under the same geometries and atmosphere parameters.
The path by which decaying slow C exits the terrestrial system is determined by the "fraction to atmosphere" parameters which have a default value of 1, (i.e., 100% of respired C goes to the atmosphere).
It is currently envisioned as a 4-spacecraft (identically instrumented) mission, which will measure all relevant in situ plasma and neutral atmosphere parameters with the option of including remote observations for a wider perspective.
The model was developed in WD of IZMIRAN and describes the three-dimensional time-dependent distribution of the upper atmosphere parameters between 80km to 15 Earth's radii including electron concentration.
The Haute Provence Observatory has for primary mission the operation of telescopes, up to two meters in diameter, for the astrophysics community, and the measurements of various upper atmosphere parameters for the geophysics community.
Similar(53)
The DOC fraction/fraction to atmosphere parameter values for the gauged catchments were applied to the ungauged catchments based on physiographic and hydrologic similarities [29] and model runs conducted for the entire SLW.
After model calibration, the three unique fraction-to-atmosphere parameters derived for Rithet, Council and Judge catchments were 0.945, 0.975, and 0.935, respectively (Table 4).
The fraction-to-atmosphere parameter from the slow belowground pool remained constant at 0.99 for all three catchments.
First, a two-dimensional soil-atmosphere model required two input categories, namely: soil properties and atmospheric parameters.
For the Baikal seismic zone (East Siberia region, 52°N, 103°E) the Earth's upper atmosphere radiation parameters were analysed for 557.7 nm emission line of atomic oxygen [OI] (de-excitation heights 85 115 km) during earthquakes.
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