“…A number of recent dynamo calculations (RICHMOND et al, 1976;KIRCHHOFF and CARPENTER, 1976;LINDZEN, 1976a, b, 1977;SALAH and EVANS, 1977;HARPER, 1977a) MAEDA, 1955;KATO, 1956;HIRONO and KITAMURA, 1956;STENING, 1969a;MATSUSHITA, 1969;TARPLEY, 1970b;VOLLAND, 1971b;MURATA, 1974b;MOHLMANN, 1976b) whose dynamo effect is most important in the 120-200km height range during the day (VOLLAND, 1971a;MOHLMANN, 1973;RICHMOND et al, 1976;FORBES and LINDZEN, 1976a). This tide can be identified to a large extent with the S1, 2 mode, modified by ion drag, generated in situ by solar heating.…”