VI. On the heat dissipated by a platinum surface at high temperatures. Part IV. Thermal emissivity in high-pressure gases
The question of the heat dissipated by a hot body in gases at ordinary pressures has received considerable attention during recent years. The subject has been experimentally treated in many different ways. The rate of cooling of a body of known specific heat has been directly measured by Dulong and Petit, Narr, Macfarlane, Nichol, Stefan, Brush, Bottomley, Winkelmann, Kundt, and Warburg, Eckerlein, Graetz, &c. By Christiansen’s method, the value of the conductivity has been derived from the fall of temperature per unit length along the axis of a cylinder carrying a constant flow of heat. Schleierm acher, Sala, Ayrton, and others have preferred to measure the quantity of electrical energy dissipated per unit time. These experiments have, however, been carried out at or below the atmospheric pressure, and the question of the heat dissipated in gases at high pressures has rarely been touched upon. From the ordinarily accepted principles of the Kinetic theory of gases, it may be shown that the conductivity of any perfect gas is independent of pressure. The experimental work of Stefan and of Kundt and Warburg has gone far to confirm this law as far as ordinary pressures are concerned. It will be seen, however, that at higher pressures, only a small proportion of the loss of heat is due to conductivity, and the question as to whether the theoretical law is strictly correct, though well worth investigation, is not of primary importance. For the above reasons the present work has been restricted to a study of the total heat dissipated at exceptionally high pressures and temperatures.