Physics
Scientific paper
Jun 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...42..497h&link_type=abstract
Solar Physics, vol. 42, June 1975, p. 497-527. Research supported by the Science Research Council of England.
Physics
36
Cosmic Rays, Interplanetary Magnetic Fields, Particle Diffusion, Power Spectra, Radiation Measurement, Spectrum Analysis, Data Acquisition, Diffusion Coefficient, Error Analysis, Heos A Satellite, Heos B Satellite, Low Frequencies, Magnetic Field Configurations, Solar Wind Velocity
Scientific paper
The analysis reported uses data from the HEOS-1 and HEOS-2 earth satellites, which have provided data on the interplanetary field from December 1968 to the present. A power spectral analysis in which the fast Fourier transform technique was used is discussed, taking into account the method, the limitations of the analysis, the coordinate system, the treatment of data breaks, and tests of the method. The spectra deduced from 5-day data sets are considered along with the spectra deduced from 85-day data sets. Attention is given to the mean field strength and solar wind velocity, the power spectra, a comparison with Explorer data, the spectral indices, the time variability of the spectra, and cosmic ray considerations.
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