On the possibility to study the thin structure of external solar wind in decameter radio waves

Details On the possibility to study the thin structure of external solar wind in decameter radio waves On the possibility to study the thin structure of external solar wind in decameter radio waves

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006kfnt...22..340o&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 22, no. 5, p.340-345

Physics

1

Scientific paper

The Feynman path-integral technique is applied to calculate the cross-spectra and phase speed of weak interplanetary scintillations. The possibility to investigate the thin structure of the outer solar wind by simultaneous measurements of temporary scintillation spectra and the phase speed dispersion dependencies is considered for decameter radio waves.

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