Method of locating the Pc 1 source and hot plasma parameters in the generation region

[1]  L. J. Cahill,et al.  THE RELATION OF Pc 1 MICROPULSATIONS MEASURED AT SIPLE, ANTARCTICA, , 1977 .

[2]  D. S. Fligel,et al.  The locating of hydromagnetic whistler sources and determination of their generating proton spectra , 1977 .

[3]  A. Sternlieb,et al.  Numerical‐experimental investigation of the enhancement of the electromagnetic ion cyclotron instability by cold plasma , 1977 .

[4]  J. C. Johnson,et al.  Comparison between Pc-1 pulsation propagation paths and the whistler determined plasmapause , 1976 .

[5]  Ja.L. Al'pert On an outer ionosphere hydrostatic model , 1975 .

[6]  D. Williams,et al.  Further aspects of the proton ring current interaction with the plasmapause: Main and recovery phases , 1974 .

[7]  D. Williams,et al.  The proton ring current and its interaction with the plasmapause: Storm recovery phase , 1974 .

[8]  T. Fritz,et al.  Initial Explorer 45 substorm observations and electric field considerations , 1974 .

[9]  T. Fritz,et al.  Observations of proton spectra (1.0 ≤ Ep ≤ 300 kev) and fluxes at the plasmapause , 1973 .

[10]  A. Roux,et al.  WAVE-PACKET PROPAGATION IN AN AMPLIFYING MEDIUM AND ITS APPLICATION TO THE DISPERSION CHARACTERISTICS AND TO THE GENERATION MECHANISMS OF Pc 1 EVENTS. , 1971 .

[11]  S.-I. Akasofu,et al.  Spherical harmonic analysis of worldwide cosmic ray variations during geomagnetic storms , 1971 .

[12]  R. R. Heacock The relation of the Pc 1 micropulsation source region to the plasmasphere , 1971 .

[13]  V. P. Hessler,et al.  POLARIZATION CHARACTERISTICS OF Pc 1 MICROPULSATIONS AT COLLEGE. , 1967 .

[14]  R. L. Smith,et al.  Properties of the outer ionosphere deduced from nose whistlers , 1961 .