activity
20122022
most citedThe DArk Matter Particle Explorer mission

322 citations · 1.3k across the 31 of their papers we have counts for

collaborators

31 papers

astro-ph.SR2022★ 3 cited

Is there a Dynamic Difference between Stealthy and Standard CMEs?

Beili Ying, Alessandro Bemporad, Li Feng +2

Stealthy Coronal Mass Ejections (CMEs), lacking low coronal signatures, may result in significant geomagnetic storms. However, the mechanism of stealthy CMEs is still highly debate…

astro-ph.SR2022★ 10 cited

Plasma heating and nanoflare caused by slow-mode wave in a coronal loop

Fanxiaoyu Xia, Tongjiang Wang, Yang Su +4

We present a detailed analysis of a reflecting intensity perturbation in a large coronal loop that appeared as sloshing oscillation and lasted for at least one and a half periods.…

astro-ph.SR2022★ 5 cited

The Lyman- Emission in a C1.4 Solar Flare Observed by the Extreme Ultraviolet Imager aboard Solar Orbiter

Ying Li, Qiao Li, De-Chao Song +7

The hydrogen Lyman- (H {\sc i} Ly) emission during solar flares has rarely been studied in spatially resolved images and its physical origin has not been fully understood. In…

astro-ph.SR2022★ 5 cited

Spatially Resolved Moving Radio Burst in Association with an EUV Wave

Lei Lu, Li Feng, Weiqun Gan

Coronal mass ejections (CMEs) are large clouds of magnetized plasma ejected from the Sun, and are often associated with acceleration of electrons that can result in radio emission…

astro-ph.SR2022★ 8 cited

Three-dimensional analyses of an aspherical coronal mass ejection and its driven shock

Beili Ying, Li Feng, Bernd Inhester +4

Context. Observations reveal that shocks can be driven by fast coronal mass ejections (CMEs) and play essential roles in particle accelerations. A critical ratio, , derived from…

astro-ph.SR2022★ 19 cited

Observational Signatures of Tearing Instability in the Current Sheet of a Solar Flare

Lei Lu, Li Feng, Alexander Warmuth +7

Magnetic reconnection is a fundamental physical process converting magnetic energy into not only plasma energy but also particle energy in various astrophysical phenomena. In this…

astro-ph.SR2021

Quasi-Periodic Pulsations Detected in Ly and Nonthermal Emissions During Solar Flares

Lei Lu, Dong Li, Zongjun Ning +2

We report quasi-periodic pulsations (QPPs) with double periods during three solar flares (viz. SOL2011-Feb-15T01:44, SOL2011-Sep-25T04:31, SOL2012-May-17T01:25). The flare QPPs wer…

astro-ph.SR2021★ 37 cited

Detection of flare multi-periodic pulsations in mid-ultraviolet Balmer continuum, Ly-alpha, hard X-ray, and radio emissions simultaneously

Dong Li, Mingyu Ge, Marie Dominique +7

Quasi-periodic pulsations (QPPs), which usually appear as temporal pulsations of the total flux, are frequently detected in the light curves of solar/stellar flares. In this study,…

astro-ph.SR2020★ 10 cited

Three-Dimensional Reconstructions of Coronal Wave Surfaces Using a New Mask-Fitting Method

Li Feng, Lei Lu, Bernd Inhester +5

Coronal waves are large-scale disturbances often driven by coronal mass ejections (CMEs). We investigate a spectacular wave event on 7 March 2012, which is associated with an X5.4…

astro-ph.SR2020★ 11 cited

Extensive Study of a Coronal Mass Ejection with UV and WL coronagraphs: the need for multi-wavelength observations

Beili Ying, Alessandro Bemporad, Li Feng +3

Coronal Mass Ejections (CMEs) often show different features in different band-passes. By combining data in white-light (WL) and ultraviolet (UV) bands, we have applied different te…

astro-ph.SR2020★ 29 cited

Quasi-periodic pulsation detected in Lyman-alpha emission during solar flares

Dong Li, Lei Lu, Zongjun Ning +3

We investigated the quasi-periodic pulsation (QPP) in Lyman-alpha, X-ray and extreme-ultraviolet (EUV) emissions during two solar flares, i.e., an X-class (SOL2012-01-27T) and a C-…

astro-ph.SR2020★ 19 cited

Relationships between Photospheric Vertical Electric Currents and Hard X-Ray Sources in Solar Flares: Statistical Study

I. V. Zimovets, I. N. Sharykin, W. Q. Gan

There are still debates whether particle acceleration in solar flares may occur due to interruption of electric currents flowing along magnetic loops. To contribute to this problem…

astro-ph.SR2019★ 25 cited

Spectroscopic and Stereoscopic Observations of the Solar Jets

Lei Lu, Li Feng, Ying Li +3

We present a comprehensive study of a series of recurrent jets that occurred at the periphery of the NOAA active region 12114 on 2014 July 7. These jets were found to share the sam…

astro-ph.SR2019★ 22 cited

A New Automatic Tool for CME Detection and Tracking with Machine Learning Techniques

Pengyu Wang, Yan Zhang, Li Feng +7

With the accumulation of big data of CME observations by coronagraphs, automatic detection and tracking of CMEs has proven to be crucial. The excellent performance of convolutional…

astro-ph.SR2019★ 19 cited

First Determination of 2D Speed Distribution within the Bodies of Coronal Mass Ejections with Cross-Correlation Analysis

Beili Ying, Alessandro Bemporad, Silvio Giordano +5

The determination of the speed of Coronal Mass Ejections (CMEs) is usually done by tracking brighter features (such as the CME front and core) in visible light coronagraphic images…

astro-ph.SR2019★ 35 cited

Different Signatures of Chromospheric Evaporation in Two Solar Flares Observed with IRIS

Y. Li, M. D. Ding, J. Hong +2

We present different signatures of chromospheric evaporation in two solar flares observed by the Interface Region Imaging Spectrograph (IRIS). In the B1.6 flare on 2016 December 6…

astro-ph.SR2019★ 24 cited

Forward Modeling of SDO/AIA and X-Ray Emission from a Simulated Flux Rope Ejection

Xiaozhou Zhao, Chun Xia, Tom Van Doorsselaere +2

We conduct forward-modeling analysis based on our 2.5 dimensional magnetohydrodynamics (MHD) simulation of magnetic flux rope (MFR) formation and eruption driven by photospheric co…

astro-ph.IM2018★ 5 cited

On the error analyses of polarization measurements of the white-light coronagraph aboard ASO-S

Li Feng, Hui Li, Bernd Inhester +4

The Advanced Space-based Solar Observatory (ASO-S) mission aims to explore two most spectacular eruptions in the Sun: solar flares and coronal mass ejections (CMEs), and their magn…

astro-ph.SR2018★ 15 cited

Properties of a Small-scale Short-duration Solar Eruption with a Driven Shock

Beili Ying, Li Feng, Lei Lu +5

Large-scale solar eruptions have been extensively explored over many years. However, the properties of small-scale events with associated shocks have been rarely investigated. We p…

astro-ph.SR2017★ 29 cited

Spectroscopic Observations of Magnetic Reconnection and Chromospheric Evaporation in an X-shaped Solar Flare

Y. Li, M. Kelly, M. D. Ding +3

We present observations of distinct UV spectral properties at different locations during an atypical X-shaped flare (SOL2014-11-09T15:32) observed by the Interface Region Imaging S…

astro-ph.IM2017★ 322 cited

The DArk Matter Particle Explorer mission

J. Chang, G. Ambrosi, Q. An +160

The DArk Matter Particle Explorer (DAMPE), one of the four scientific space science missions within the framework of the Strategic Pioneer Program on Space Science of the Chinese A…

astro-ph.SR2017★ 12 cited

Characteristics of events with metric-to-decahectometric type II radio bursts associated with CMEs and flares in relation to SEP events

O. Prakash, Li Feng, G. Michalek +4

A gradual solar energetic particle (SEP) event is thought to happen when particles are accelerated at a shock due to a fast coronal mass ejection (CME). To quantify what kind of so…

astro-ph.SR2016★ 7 cited

On the Power-Law Distributions of X-ray Fluxes from Solar Flares Observed with GOES

You-ping Li, Li Feng, Ping Zhang +2

Power-law frequency distributions of the peak flux of solar flare X-ray emission have been studied extensively and attributed to a system of self-organized criticality (SOC). In th…

astro-ph.SR2015★ 32 cited

Why does the apparent mass of a coronal mass ejection increase?

Li Feng, Yuming Wang, Fang Shen +4

Mass is one of the most fundamental parameters characterizing the dynamics of a coronal mass ejection (CME). It has been found that CME apparent mass measured from the brightness e…