An experimental investigation of the scintillation of radio stars observed at frequencies of 223 and 456 megacycles per second from a location close to the auroral zone
- 1 May 1962
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 67 (5) , 1763-1784
- https://doi.org/10.1029/jz067i005p01763
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Observed variations in the amplitude scintillations of the Cassiopeia (23N5A) radio sourceJournal of Atmospheric and Terrestrial Physics, 1960
- Effect of line-of-sight aurora on radio star scintillationsJournal of Geophysical Research, 1960
- The Use of Radio Stars to Study Irregular Refraction of Radio Waves in the IonosphereProceedings of the IRE, 1958
- The origin of the ionospheric irregularities responsible for radio-star scintillations and spread-F—I. Review of existing theoriesJournal of Atmospheric and Terrestrial Physics, 1957
- XCVII. A rotating-lobe interferometer and its application to radio astronomyJournal of Computers in Education, 1955
- Identification of the Radio Sources in Cassiopeia, Cygnus a, and Puppis a.The Astrophysical Journal, 1954
- Fine Structure of the Extra-terrestrial Radio Source Cygnus INature, 1953
- Apparent Angular Sizes of Discrete Radio Sources: Observations at Jodrell Bank, ManchesterNature, 1952
- The diffraction of galactic radio waves as a method of investigating the irregular structure of the ionosphereProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1952
- Diffraction from an irregular screen with applications to ionospheric problemsPhilosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1950