activity
20072022
most citedObservational Test of Coronal Magnetic Field Models I. Comparison with Potential Field Model

65 citations · 210 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.IM2022

Development of Integral Field Spectrographs to Revolutionize Spectroscopic Observations of Solar Flares and other Energetic Solar Eruptions

Haosheng Lin, Tetsu Anan, Gianna Cauzzi +9

The Sun's proximity offers us a unique opportunity to study in detail the physical processes on a star's surface; however, the highly dynamic nature of the stellar surface -- in pa…

astro-ph.SR2022

Justification of the use of Stokes-V Cryo-NIRSP/DKIST observations for the 3D Reconstruction of the Coronal Magnetic Field

Maxim Kramar, Haosheng Lin

This study presents a justification of the use of Stokes-V Cryo-NIRSP/DKIST observations for the 3D Reconstruction of the Coronal Magnetic Field. A magnetohydrodynamic (MHD) model…

astro-ph.SR2019★ 2 cited

Astro2020 Science White Paper: Synoptic Studies of the Sun as a Key to Understanding Stellar Astrospheres

Valentin Martinez Pillet, Frank Hill, Heidi Hammel +11

Ground-based solar observations provide key contextual data (i.e., the 'big picture') to produce a complete description of the only astrosphere we can study in situ: our Sun's heli…

astro-ph.IM2018★ 5 cited

Infrared Imaging Spectroscopy Using Massively Multiplexed Slit-Based Techniques and Sub-Field Motion Correction

Thomas A. Schad, Haosheng Lin

Targeting dynamic spatially-extended phenomena in the upper solar atmosphere, a new instrument concept has been developed and tested at the Dunn Solar Telescope in New Mexico, USA,…

astro-ph.SR2016★ 50 cited

Vector magnetic field measurements along a cooled stereo-imaged coronal loop

Thomas A. Schad, Matthew J. Penn, Haosheng Lin +1

The variation of the vector magnetic field along structures in the solar corona remains unmeasured. Using a unique combination of spectropolarimetry and stereoscopy, we infer and c…

astro-ph.SR2016★ 1 cited

3D Global Coronal Density Structure and Associated Magnetic Field near Solar Maximum

Maxim Kramar, Vladimir Airapetian, Haosheng Lin

Measurement of the coronal magnetic field is a crucial ingredient in understanding the nature of solar coronal dynamic phenomena at all scales. We employ STEREO/COR1 data obtained…