The equation proposed earlier has been derived from a new kinetic concept. I t is shown t o be a reasonable approximation of this new consideration. The equation is also shown to be mathematically consistent with the general fact that when the thermomolecular pressure difference is plotted against the normally measured pressure, a single maximum is obtained. T h e curves calculated from this equation are shown t o agree closely with those from the Weber equation using van Itterbeek and de Grande's data. T h e practical use of the equation is discussed.
INTRODUCTIONThe problem of the effect of thermal transpiration on pressure, or the thermomolecular pressure difference, was observed and investigated by a number of workers both experimentally and mathematically (1,4, 9). Although a practical solution was not obtained, the problem was neglected for many years. I t was not even mentioned in most publications where it was obviously important.Recently, Weber and his co-workers reinvestigated this problem and showed the extent to which a pressure measurement may be affected (11, 12). More recently, the problem was again brought to the general attention of this continent. Its practical importance was demonstrated by Liang (6) in the the case of vapor pressure measurement, and by Crowell and Young (2) in the case of physical adsorption.Until very recently, the only available equation by which the thermal transpiration effect may be calculated was a semiempirical one obtained by Weber and his co-workers. The equation was derived along the line given by Maxwell with modifications suggested by Weber, and took the general form in which y = R/X, R being the tube radius and X the mean free path of the gas; n was related to the viscosity q by the equation B , C, D, m, m', and m" were constants calculated from another three semiempirical constants, kl, k?, and p, which in turn were evaluated from the experimental data. Weber and Schmidt (13) calculated the constants for helium. van Itterbeek and de Grande (10) found that the values of kl, k?, and p were functions of the nature of the gas and that separate determinations for different gases must be made. They extended the equation accordingly to cover the cases of hydrogen, deuterium, and neon. l d~a~z z~s c r i p t