activity
20012026
most citedDynamic Processes of the Moreton Wave on 2014 March 29

15 citations · 44 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

Short timescale variation in the submillimeter flux of Sagittarius A*

Makoto Miyoshi, Yoshiaki Kato, Yoshiharu Asaki +8

We study short-timescale 340 GHz flux-density variability of Sgr A* using ALMA Cycle 3 observations. Careful self-calibration enabled 10 s snapshot imaging with very high effective…

astro-ph.SR2021★ 3 cited

A Three-Dimensional Velocity of an Erupting Prominence Prior to a Coronal Mass Ejection

Maria V. Gutierrez, Kenichi Otsuji, Ayumi Asai +10

We present a detailed three-dimensional (3D) view of a prominence eruption, coronal loop expansion, and coronal mass ejections (CMEs) associated with an M4.4 flare that occurred on…

astro-ph.SR2019★ 15 cited

Dynamic Processes of the Moreton Wave on 2014 March 29

Denis P. Cabezas, Ayumi Asai, Kiyoshi Ichimoto +4

On 2014 March 29, an intense solar flare classified as X1.0 occurred in the active region 12017. Several associated phenomena accompanied this event, among them a fast-filament eru…

astro-ph.SR2017★ 7 cited

"Dandelion" Filament Eruption and Coronal Waves Associated with a Solar Flare on 2011 February 16

Denis P. Cabezas, Lurdes M. Martínez, Yovanny J. Buleje +11

Coronal disturbances associated with solar flares, such as H Moreton waves, X-ray waves, and extreme ultraviolet (EUV) coronal waves are discussed herein in relation to magnetoh…

astro-ph.HE2009★ 2 cited

Water Cherenkov Detectors response to a Gamma Ray Burst in the Large Aperture GRB Observatory

D. Allard, C. Alvarez, H. Asorey +38

In order to characterise the behaviour of Water Cherenkov Detectors (WCD) under a sudden increase of 1 GeV - 1 TeV background photons from a Gamma Ray Burst (GRB), simulations were…

astro-ph.HE2009★ 2 cited

The Large Aperture GRB Observatory

D. Allard, C. Alvarez, H. Asorey +38

The Large Aperture GRB Observatory (LAGO) is aiming at the detection of the high energy (around 100 GeV) component of Gamma Ray Bursts, using the single particle technique in array…