activity
20022022
most citedTeraelectronvolt emission from the -ray burst GRB 190114C

286 citations · 1.8k across the 45 of their papers we have counts for

collaborators

47 papers

astro-ph.SR2022

Proton Penetration Efficiency over a High Altitude Observatory in Mexico

S. Miyake, T. Koi, Y. Muraki +12

In association with a large solar flare on November 7, 2004, the solar neutron detectors located at Mt. Chacaltaya (5,250m) in Bolivia and Mt. Sierra Negra (4,600m) in Mexico recor…

astro-ph.SR2021★ 4 cited

Energy and spectral analysis of confined solar flares from radio and X-ray observations

Chengming Tan, Karl-Ludwig Klein, Yihua Yan +4

The energy and spectral shape of radio bursts may help us understand the generation mechanism of solar eruptions, including solar flares, CMEs, eruptive filaments, and various scal…

astro-ph.SR2021★ 37 cited

Non-equilibrium Flux Rope Formation by Confined Flares Preceding a Solar Coronal Mass Ejection

Bernhard Kliem, Jeongwoo Lee, Rui Liu +3

We present evidence that a magnetic flux rope was formed before a coronal mass ejection (CME) and its associated long-duration flare during a pair of preceding confined eruptions a…

astro-ph.SR2020★ 3 cited

Solar Neutron Decay Protons observed in November 7, 2004

Yasushi Muraki, Jose F. Valde-Galicia, Ernesto Ortiz +10

We have found an interesting event registered by the solar neutron telescopes installed at high mountains in Bolivia (5250 m a.s.l.) and Mexico (4600 m a.s.l.). The event was obser…

astro-ph.SR2020★ 7 cited

Multiwavelength Stereoscopic Observation of the May 1, 2013 Solar Flare and CME

Erica Lastufka, Säm Krucker, Ivan Zimovets +7

A M-class behind-the-limb solar flare on 1 May 2013 (SOL2013-05-01T02:32), accompanied by a ( 400 km/s) CME was observed by several space-based observatories with different v…

astro-ph.HE2020★ 11 cited

Study of the GeV to TeV morphology of the -Cygni SNR (G78.2+2.1) with MAGIC and Fermi-LAT

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +183

Context. Diffusive shock acceleration (DSA) is the most promising mechanism to accelerate Galactic cosmic rays (CRs) in the shocks of supernova remnants (SNRs). The turbulence upst…