117 citations · 294 across the 14 of their papers we have counts for
14 papers
Research Progress on Solar Small-Scale Dynamo
Wen-Jie Jiang, Lei Ni, Chun-Lan Jin +2
The small-scale solar dynamo theory, as the core mechanism explaining the origin of the persistent, disperse weak magnetic field in the quiet Sun regions, has made significant prog…
Statistical analysis of the Si I 6560.58 Å line observed by CHASE
Jie Hong, Ye Qiu, Qi Hao +4
The Si I 6560.58 Å line in the H blue wing is blended with a telluric absorption line from water vapor in ground-based observations. Recent observations with the space-based tel…
Calibration procedures for the CHASE/HIS science data
Ye Qiu, ShiHao Rao, Chuan Li +17
The Hα line is an important optical line in solar observations containing the information from the photosphere to the chromosphere. To study the mechanisms of solar eruptions and t…
High-Resolution Observations of Prominence Plume Formation with the New Vacuum Solar Telescope
Jian-Chao Xue, Jean-Claude Vial, Yang Su +5
Prominence plumes are evacuated upflows that emerge from bubbles below prominences, whose formation mechanism is still unclear. Here we present a detailed study of plumes in a quie…
Imaging and spectral study on the null point of a fan-spine structure during a solar flare
Shuhong Yang, Qingmin Zhang, Zhi Xu +3
Using the multi-instrument observations, we make the first simultaneous imaging and spectral study on the null point of a fan-spine magnetic topology during a solar flare. When mag…
Propagating Slow Sausage Waves in a Sunspot Observed by the New Vacuum Solar Telescope
Song Feng, Zheng Deng, Ding Yuan +2
A sunspot is an ideal waveguide for a variety of magnetohydrodynamic waves, which carry a significant amount of energy to the upper atmosphere and could be used as a tool to probe…
Spectro-polarimetric Observations at the NVST: I. Instrumental Polarization Calibration and Primary Measurements
Jun-Feng Hou, Zhi Xu, Shu Yuan +8
This paper is devoted to the primary spectro-polarimetric observation performed at the New Vacuum Solar Telescope of China since 2017, and our aim is to precisely evaluate the real…
Research progress based on observations of the New Vacuum Solar Telescope
Xiaoli Yan, Zhong Liu, Jun Zhang +1
The purpose of this paper is to introduce the main scientific results made by the one-meter New Vacuum Solar Telescope (NVST), which was put into commission on 2010. NVST is one of…
Composing Method for the Two-dimensional Scanning Spectra Observed by the New Vacuum Solar Telescope
Yun-Fang Cai, Zhi Xu, Yu-Chao Chen +4
In this paper we illustrate the technique used by the New Vacuum Solar Telescope to increase the spatial resolution of two-dimensional (2D) solar spectroscopy observation involving…
Precise Reduction of Solar Spectra Observed by the 1-meter New Vacuum Solar Telescope
Yunfang Cai, Zhi Xu, Zhenggang Li +4
We present a precise and complete procedure for processing spectral data observed by the 1-meter New Vacuum Solar Telescope (NVST). The procedure is suitable for both the sit-and-s…
Are IRIS bombs connected to Ellerman bombs?
Hui Tian, Zhi Xu, Jiansen He +1
Recent observations by the Interface Region Imaging Spectrograph (IRIS) have revealed pockets of hot gas (2--810 K) potentially resulting from magnetic reconnec…
Fine Magnetic Structure and Origin of Counter-Streaming Mass Flows in a Quiescent Solar Prominence
Yuandeng Shen, Yu Liu, Ying D. Liu +4
We present high-resolution observations of a quiescent solar prominence which was consisted of a vertical and a horizontal foot encircled by an overlying spine, and counter-streami…
Diagnostics of Ellerman Bombs with High-resolution Spectral Data
Z. Li, C. Fang, Y. Guo +3
Ellerman bombs (EBs) are tiny brightenings often observed near sunspots. The most impressive characteristic of the EB spectra is the two emission bumps in both wings of the H an…
New Vacuum Solar Telescope and Observations with High Resolution
Zhong Liu, Jun Xu, Bo-Zhong Gu +17
The New Vacuum Solar Telescope (NVST) is a 1 meter vacuum solar telescope that aims to observe the fine structures on the Sun. The main tasks of NVST are high resolution imaging an…