38 citations · 119 across the 6 of their papers we have counts for
6 papers
Extreme-ultraviolet Late Phase Caused by Magnetic Reconnection over Quadrupolar Magnetic Configuration in a Solar Flare
Zhenjun Zhou, Xin Cheng, Lijuan Liu +3
A second emission enhancement in warm coronal extreme-ultraviolet (EUV) lines (about 2-7 MK) during some solar flares is known as the EUV late phase. Imaging observations confirm t…
Extremely Large Extreme-ultraviolet Late Phase Powered by Intense Early Heating in a Non-eruptive Solar Flare
Yu Dai, Mingde Ding, Weiguo Zong +1
We analyzed and modeled an M1.2 non-eruptive solar flare on 2011 September 9. The flare exhibits a strong late-phase peak of the warm coronal emissions (3~MK) of extreme-ultr…
Probing the Production of Extreme-ultraviolet Late-Phase Solar Flares by Using the Model Enthalpy-Based Thermal Evolution of Loops
Yu Dai, Mingde Ding
Recent observations in extreme-ultraviolet (EUV) wavelengths reveal an EUV late phase in some solar flares that is characterized by a second peak in warm coronal emissions (…
Mode-Conversion of a Solar Extreme-Ultraviolet Wave over a Coronal Cavity
Weiguo Zong, Yu Dai
We report on observations of an extreme-ultraviolet (EUV) wave event in the Sun on 2011 January 13 by \emph{Solar Terrestrial Relations Observatory} (\emph{STEREO}) and \emph{Solar…
Coronal and Chromospheric Signatures of Large-Scale Disturbances Associated with a Major Solar Eruption
Weiguo Zong, Yu Dai
We present both coronal and chromospheric observations of large-scale disturbances associated with a major solar eruption on 2005 September 7. In GOES/SXI, arclike coronal brighten…
Millimeter Dust Emission in the GQ Lup System
Yu Dai, David J. Wilner, Sean M. Andrews +1
We present Submillimeter Array observations of the GQ Lup system at 1.3 millimeters wavelength with $0\farcs4$ (60 AU) resolution. Emission is detected from the position of t…