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David Ruffolo

Researcher at Mahidol University

Publications -  207
Citations -  4271

David Ruffolo is an academic researcher from Mahidol University. The author has contributed to research in topics: Cosmic ray & Solar wind. The author has an hindex of 32, co-authored 189 publications receiving 3321 citations. Previous affiliations of David Ruffolo include National Astronomical Research Institute of Thailand & Chulalongkorn University.

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Effect of adiabatic deceleration on the focused transport of solar cosmic rays

TL;DR: In this paper, an explicit formula is given for the deceleration of individual particles as a function of the pitch angle, and other first-order effects of the solar wind, including convection, are incorporated into a numerical code for simulating the transport of energetic particles along the interplanetary magnetic field.
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Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 γ-ray Galactic sources

Zhengguo Cao, +264 more
- 17 May 2021 - 
TL;DR: In this article, the authors reported the detection of more than 530 photons at energies above 100 teraelectronvolts and up to 1.4 PeV from 12 sources in the Galaxy.
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Energetic Particle Observations during the 2000 July 14 Solar Event

TL;DR: In this paper, high-latitude neutron monitors are used to deduce the intensity-time and anisotropy-time pro-les and pitch-angle distributions of energetic protons near Earth during the major solar event on 2000 July 14 (also known as the Bastille Day event).
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Spectral properties and length scales of two-dimensional magnetic field models

TL;DR: In this paper, the authors discuss the properties of 2D models of magnetic field fluctuations and turbulence and their observable power spectra and present a technique for determining an ultrascale from observations at a single spacecraft.
Posted Content

The Large High Altitude Air Shower Observatory (LHAASO) Science White Paper

X. Bai, +116 more
TL;DR: The Large High Altitude Air Shower Observatory (LHAASO) project is a new generation multi-component instrument, to be built at 4410 meters of altitude in the Sichuan province of China, with the aim to study with unprecedented sensitivity the spec trum, the composition and the anisotropy of cosmic rays in the energy range between 10$^{12}$ and 10$€18}$ eV, as well as to act simultaneously as a wide aperture (one stereoradiant), continuously operated gamma ray telescope in the EH range between