Antony Hewish, PhD

1952- Cavendish Astrophysics Group University of Cambridge, Cambridge, England, United Kingdom 
Radio Astronomy, Pulsars
"Antony Hewish"

The Nobel Prize in Physics 1974 was awarded jointly to Sir Martin Ryle and Antony Hewish "for their pioneering research in radio astrophysics: Ryle for his observations and inventions, in particular of the aperture synthesis technique, and Hewish for his decisive role in the discovery of pulsars"

Mean distance: 13.98


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Martin Ryle grad student 1946-1952 Cambridge


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Derek Wills grad student 1966 Cambridge
Jocelyn Bell Burnell grad student 1965-1969 Cambridge
Anthony C. Readhead grad student 1972 Cambridge
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Hewish A. (2008) Background to discovery: Some recollections Aip Conference Proceedings. 983: 3-7
Hewish A. (2004) Passionate about pulsars [3] Astronomy and Geophysics. 45: 7
Hewish A. (2001) Drummed out New Scientist. 170: 54-55
Hewish A. (2000) Comment I on "Generation of focused, nonspherically decaying pulses of electromagnetic radiation" Physical Review. E, Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics. 62: 3007
Crooker NU, Gosling JT, Bothmer V, et al. (1999) CIR morphology, turbulence, discontinuities, and energetic particles: Report of Working Group 2 Space Science Reviews. 89: 179-220
Balogh A, Bothmer V, Crooker NU, et al. (1999) The solar origin of corotating interaction regions and their formation in the inner heliosphere: Report of Working Group 1 Space Science Reviews. 89: 141-178
Hewish A. (1996) Problems with the superluminal pulsar model Monthly Notices of the Royal Astronomical Society. 280: L27-L30
Hewish A. (1996) Low density drivers of strong interplanetary shocks Astrophysics and Space Science. 243: 5-13
Hewish A, Woan G. (1995) Interplanetary scintillation imaging of disturbances in the solar wind Lecture Notes in Physics. 444: 173-182
Willis DM, Hewish A, Rishbeth H, et al. (1994) Synoptic data for solar-terrestrial physics: the U.K. contribution to long-term monitoring Journal of Atmospheric and Terrestrial Physics. 56: 871-875,877-886
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