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Gas is generally characterized by the ratio of gas density to air density.
It can now be seen why η is independent of gas density or pressure.
The gas density effect is found to increase with the gas density and the gas velocity.
In dense regions, the SFR and total gas density are well-represented by a Schmidt power-law relation.
Stellar radiation can apparently enter the cloud through channels where the dust (and gas) density is lower than average.
The gas density effect increased with the gas velocity.
It was observed that ANFIS predicts natural gas density with AARD% of 1.704; and is able to estimate gas density as accurate as sophisticated EOS.
where is the Langevin collision rate, with ρn being the buffer gas density, αn the cold-atom polarizability and μ the atom ion reduced mass.
One of his first assignments was to develop a device to determine how changes in pressure and temperature affect gas density.
This is accomplished by leaving a gas density depression on the channel's axis after hydrodynamic expansion.
In the case of reduced gas density, the opposite effect will occur.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com