ii) In the case of the Ideal Gas Law it is the height of an atmosphere of a given mass that determines
the number of molecules per unit of volume at the surface and the more molecules per unit of volume the hotter the surface will become at a given level of solar input.
The molar density of a gas tells you the average
number of molecules per cubic metre of the gas.
The number of moles, the mass and
the number of molecules per gram are the properties that have a major influence on the mean free path length of photons through the gases comprising the atmosphere.
In the earths atmosphere, pressure, which is related to
the number of molecules per unit volume, decreases exponentially with altitude.
Not exact matches
If we now consider the
number of the stars (15,000 x 106 visible to the optical telescope alone) you will understand how it is possible to say, cosmically speaking, that we are enveloped in a sort
of monstrous gas formed
of molecules as heavy as the Sun moving at distances from each other so great that they have to be reckoned in light - years (bearing in mind that light travels at a speed
of 186,000 miles
per second, and that we are only 8 light - minutes distant from the sun)-- a gas made
of stars!
Carbon dioxide concentrations in the atmosphere are measured in parts
per million, the
number of molecules of carbon dioxide there are in every million
molecules of air.
As each sequencing glass slide can sequence only a finite
number of DNA
molecules, higher levels
of multiplexing would lead to fewer DNA
molecules to be sequenced
per sample.
Concentration units are parts
per million (ppm) or parts
per billion (ppb), indicating the
number of molecules of the greenhouse gas
per million or billion
molecules of air.
Whether being lesser than CO2 in
number of molecules in the atmosphere, methane is a potent greenhouse gas absorbing more infra - red radiation
per molecule than CO2.
An antibody therapy against a key inflammatory
molecule involved in migraines reduces the
number of headaches that chronic migraine patients experience
per month in a phase III trial A new s...
Amino acids have approximately the same
number of calories as any other peptide
molecule or protein, which is 4 calories
per gram.
The thyroid requires iodine to manufacture thyroid hormones, T3 and T4, the «3» and «4» referring to the
number of iodine atoms
per thyroid hormone
molecule.
So, by Avogadro's
number you've got about 6 x 10e23
molecules per mole
of air, and that's about 22 liters (according, at least, to some random website I once consulted — corrections welcomed.)
You have to look at the absorption crosssection
per molecule of CO2 and count up the
number of CO2
molecules per unit area that would be in the path
of a photon travelling a certain distance in the atmosphere you can understand how such a low concentration
of CO2 can have such a large effect.
The
number means there would be 950
molecules of carbon dioxide in the air
per every million air
molecules.
The
number means there were 313
molecules of carbon dioxide in the air
per every million air
molecules.
The
number of molecules passing through unit area
per unit time multiplied by the average energy carried
per molecule.
Ok, don't see where you gave where any
of the
numbers are coming from but it suffices you seem sure the radiation pressure from added GHG
molecules (H2O or CO2), let's say 10
per million is so infinitesimally small that the lift
of the atmosphere in every cubic meter
per one meter layer up to say 80 km is so insignificant it can be totally ignored.