Open Access
Observations of high-energy gamma rays
Giovanni G. Fazio
- Vol. 339, pp 153
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TLDR
In this paper, the application of the Cerenkov light technique to detect the intensity and direction of incident gamma ray photons above 10 to the 11th power eV was studied, and the results showed that the technique can be used to detect gamma ray gamma rays.Abstract:
The application of the Cerenkov light technique to detect the intensity and direction of incident gamma ray photons above 10 to the 11th power eV is studied.read more
Citations
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Solar-terrestrial response to large extension or long-duration solar gamma ray events
TL;DR: In this article, the authors discuss the plasma and particle data at Earth´s orbit for these two types of events and propose that some perturbations in interplanetary space may originate in the solar chromosphere outside active regions.
Small scale turbulence in the Crab Nebula: Evidence of lower hybrid parametric instabilities driven by the pulsar wave
TL;DR: In this paper, it was shown that the strong 30 Hz pulsar wave can parametrically excite instabilities near the lower hybrid frequency in the thermal plasma of the Crab Nebula with a characteristic wavelength of the order of the scale size a of the turbulence observed.
References
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Journal ArticleDOI
Solar-terrestrial response to large extension or long-duration solar gamma ray events
TL;DR: In this article, the authors discuss the plasma and particle data at Earth´s orbit for these two types of events and propose that some perturbations in interplanetary space may originate in the solar chromosphere outside active regions.
Small scale turbulence in the Crab Nebula: Evidence of lower hybrid parametric instabilities driven by the pulsar wave
TL;DR: In this paper, it was shown that the strong 30 Hz pulsar wave can parametrically excite instabilities near the lower hybrid frequency in the thermal plasma of the Crab Nebula with a characteristic wavelength of the order of the scale size a of the turbulence observed.