Excerpt from Report on the Present State of Our Knowledge, Respecting the General Circulation of the Atmosphere: Presented to the Meteorological Congress at Chicago, August, 1893
But if, as Ferrel wished, we apply the law of conservation of areas to these currents, their existence becomes extremely difficult of comprehension. At great heights friction is very small, so that the velocities ought to approach the theoretical ones; from which it results that there must be a very considerable s10pe in order to overcome centrifugal effects.
Now, one finds oneself in this dilemma - Either the elevation of the air necessary at the equator in order to produce this slope is due to a dynamic effect, and then the pressure at the equator ought to be very great in the lower regions, in consequence of the considerable mass of air which rises there; or the elevation is due to a difference of density, and then it is necessary that there should exist a difference of temperature between the equator and the pole which is not observed on the globe, or indeed that the currents should be produced at an enormous height.
M. Moller has, in fact, shown that it is necessary, in addition to the flattening of the globe, that the air should fall more than 21 kilometres in order to permit it to reach Now, the difference of temperature between the equator and the poles scarcely gives a fall of 900 metres at the height of metres. It would therefore be necessary that the current directed towards the pole should be at an enormous height, in order that the effect of the equatorial heating should produce the necessary difference of elevation, which is that of at least 21 kilometres.
I leave these reflections for the consideration of meteorologists, and I think that my reservation as to these currents will be approved.
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Paperback. Condición: New. Print on Demand. This book analyzes Earth's weather systems, looking at how pressure, temperature, wind, and other elements interact to drive the global circulation patterns that affect our everyday lives. The author, who has been studying the movement of the atmosphere for over fifteen years, describes how the sun's energy creates temperature differences that result in pressure variations. These variations cause air to move from high pressure areas to low pressure areas, generating winds and changing weather patterns. The book draws on the laws of physics to explain how the Earthâs rotation and the Earthâs uneven heating combine to create the complex dynamics of the atmosphere. It examines the effects of these systems on temperature, humidity, and precipitation and shows how they interact to create the unique climates we find around the world. The author also explores how the atmosphere interacts with the oceans, the land, and even the sun, providing a comprehensive overview of how the Earth's systems connect and influence each other. This book is a reproduction of an important historical work, digitally reconstructed using state-of-the-art technology to preserve the original format. In rare cases, an imperfection in the original, such as a blemish or missing page, may be replicated in the book. print-on-demand item. Nº de ref. del artículo: 9781332289318_0
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PAP. Condición: New. New Book. Shipped from UK. Established seller since 2000. Nº de ref. del artículo: LW-9781332289318
Cantidad disponible: 15 disponibles