The Energy System of Matter: A Deduction from Terrestrial Energy PhenomenaWeir, James, active 1883-1912
Science
The Energy System of Matter: A Deduction from Terrestrial Energy Phenomena
Weir, James, active 1883-1912
Force and energy
It might naturally be expected that such movements of the atmospheric
air masses as have been described above would give rise to great
atmospheric disturbance over the earth's surface, and that the transfer
of gaseous material from pole to equator and vice versa would be
productive of violent storms of wind. Such storms, however, are
phenomena of somewhat rare occurrence; the atmosphere, on the whole,
appears to be in a state of comparative tranquillity. This serenity of
the atmosphere is, however, confined to the lower strata, and may be
ascribed to an inherent stability possessed by the air mass as a whole
in virtue of the accession of energy to it at high levels. As already
explained, the transfer of energy from the vapour to the air masses is
accomplished at comparatively low altitudes, and when this reaction is
taking place the whole tendency of the energised material is to move
upwards. In so moving it tends to leave behind it the condensed aqueous
vapour, and would, therefore, rise to the higher altitudes in a
comparatively dry condition. This dryness is accentuated by the further
loss of aqueous vapour by condensation as the air moves toward regions
of low velocity. That air which actually attains to the poles will be
practically dry, and having also returned, in its entirety, the surplus
energy obtained from the aqueous vapour, it will be in this region
practically in the condition of statical equilibrium of a gas against
gravity (§ 34). But the general state of the atmosphere in other regions
where a transference of energy from the aqueous vapour has taken or is
taking place is very different from this condition of natural statical
equilibrium which is approached at the poles. In the lower strata of the
atmosphere the condition in some cases may approximate to the latter,
but in the upper strata it is possessed of energy qualities quite
abnormal to statical equilibrium. Its condition is rather one of the
nature of stable equilibrium. It is in a condition similar to that of a
liquid heated in its upper layers; there is absolutely no tendency to a
direct or vertical downward circulation. In statical equilibrium, any
downward movement of an air mass would simply be accompanied by the
natural rise in temperature corresponding to the transformation of its
energy of position, but in this condition of stable equilibrium any
motion downwards must involve, not only this natural temperature rise,
but also a return, either in whole or in part, of the energy absorbed
from the aqueous vapour. The natural conditions are therefore against
any direct vertical return. These conditions, however, favour in every
respect the circulatory motion of the highly energised upper air masses
towards regions of low velocity. All circumstances combine, in fact, to
confine the more powerfully energised and highly mobile air masses to
high altitudes. In the lower atmosphere, owing to the continuous action
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