The evolution of climateBrooks, C. E. P. (Charles Ernest Pelham)
Science
The evolution of climate
Brooks, C. E. P. (Charles Ernest Pelham)
Climatology; Paleoclimatology
The great glaciation of the Permian period, referred to in the
next chapter, is a totally different matter. During this time the
ice-sheets appear to have reached their maximum area, and to have
extended to sea-level, in countries which are at present close to
the equator, while lands now in high latitudes remained unglaciated.
It is true that at the present day glaciers exist at high latitudes
under the equator itself, and given a ridge sufficiently steep and
a snowfall sufficiently heavy such glaciers would possibly extend
to sea-level; but even these conditions would not give rise to the
enormous deposits of true boulder-clay which have been discovered,
and there seems no way of avoiding the supposition of an enormous
difference in the position of the pole relatively to the continents
at this time.
Wegener’s theory alone, however, requires that glaciation should
always have been proceeding in some part of the globe (unless both
poles were surrounded by wide expanses of ocean), which is hard to
reconcile with the extremely definite and limited glaciations which
geological research has demonstrated. In these circumstances we may
tentatively explain the pre-Tertiary glacial periods by combining
Wegener’s theory of the movements of continents and oceans as a
whole with the theory of changes of elevation and of land and sea
distribution which is outlined below. That is to say, we may suppose
that the positions of the continents and oceans have changed,
relatively both to each other and to the poles, slowly but more
or less continuously throughout geological time; while at certain
periods the land and sea distribution became favourable for extensive
glaciation of the regions which at that time were in high latitudes.
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