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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…
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…
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…
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…
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…
Microwave Study of a Solar Circular Ribbon Flare
Jeongwoo Lee, Stephen M. White, Xingyao Chen +4
A circular ribbon flare SOL2014-12-17T04:51 is studied using the 17/34 GHz maps from the Nobeyama Radioheliograph (NoRH) along with (E)UV and magnetic data from the Solar Dynamics…