activity
20172019
most citedSuccessive Two-sided loop Jets Caused by Magnetic Reconnection between Two adjacent Filamentary Threads

41 citations · 171 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2019

Two Quasi-periodic Fast-propagating Magnetosonic Wave Events Observed In Active Region NOAA 11167

Yuhu Miao, Yu Liu, A. Elmhamdi +6

We report a detailed observational study of two quasi-periodic fast-propagating (QFP) magnetosonic wave events occurred on 2011 March 09 and 10, respectively. Interestingly, both t…

astro-ph.SR201916 cited

A new small satellite sunspot triggering recurrent standard- and blowout-coronal jets

Yuhu Miao, Y. Liu, Y. D. Shen +5

In this paper,we report a detailed analysis of recurrent jets originated from a location with emerging, canceling and converging negative magnetic field at the east edge of NOAA ac…

astro-ph.SR201833 cited

A Quasi-periodic propagating wave and EUV waves excited simultaneously in a solar eruption event

Y. H. Miao, Y. Liu, Y. D. Shen +4

Quasi-periodic fast-propagating (QFP) magnetosonic waves and extreme ultraviolet (EUV) waves were proposed to be driven by solar flares and coronal mass ejections (CMEs), respectiv…

astro-ph.SR201830 cited

Two strong white-light solar flares in AR NOAA 12673 as potential clues for stellar superflares

Paolo Romano, Abouazza Elmhamdi, Ayman Kordi

Recently, two strong homologous white light flares of X-GOES class occurred on the Sun on Sept. 06, 2017, providing a rare exceptional opportunity to study the mechanisms responsib…

astro-ph.SR201831 cited

Homologous white light solar flares driven by photosperic shear motions

P. Romano, A. Elmhamdi, M. Falco +4

We describe the peculiarity of two recurrent white light flares occurred on Sept. 06, 2017, in the super Active Region (SAR) NOAA 12673, with a time interval, between their peaks,…

astro-ph.IM201720 cited

Conditions for Coronal Observation at the Lijiang Observatory in 2011

M. Y. Zhao, Y. Liu, A. Elmhamdi +4

The sky brightness is a critical parameter for estimating the coronal observation conditions for solar observatory. As part of a site-survey project in Western China, we measured t…