“…The TE and TM parts of the magnetic field H are derived for region n from scalar functions 'I'n and 4>" which are expressed as double Fourier integrals. In the compressible plasma (region n = 2) the electric field E depends also on the pressure Pn, which is also given by a double integral [eq (1) to (16) of Galejs, 1966a]. The fields near the antenna are specified with the amplitudes A1 and B1 of 'l't and cl>t, which are computed after relating tliem to the amplitudes A2, B2, C2, Aa, and Ca, and to the reflection coefficients Rat, Rb1, Raz, and Rcz from a total of 10 boundary conditions (E:r, Ey, H:r, Hu continuous and Vz=O at z=zt and z2)-These equations can be solved for the reflection coefficients Rai and Rbi· A lenithly algebraic manipulation shows that the reflection coefficients of the TE modes Rat and Ra2 are the same as for cold plasma [eq (4), Galejs,196~b].…”