activity
20062026
most cited3D Coronal Density Reconstruction and Retrieving the Magnetic Field Structure during Solar Minimum

25 citations · 53 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026★ 1 cited

A Probabilistic Calibration Procedure for the CORSAIR Polarimeter

Alan Hsu, Jenna Samra, Steven Tomczyk +1

We present a novel Bayesian model and a corresponding robust, probabilistic calibration procedure for the CORSAIR polarimeter that can be applied to other polarimeters. Our calibra…

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.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…

astro-ph.SR2015★ 19 cited

Direct Observation of Coronal Magnetic Fields by Vector Tomography of the Coronal Emission Line Polarizations

M. Kramar, H. Lin, S. Tomczyk

This article presents the first direct "observation" of the global-scale, 3D coronal magnetic fields of Carrington Rotation (CR) Cycle 2112 using vector tomographic inversion techn…

astro-ph.SR2014★ 25 cited

3D Coronal Density Reconstruction and Retrieving the Magnetic Field Structure during Solar Minimum

M. Kramar, V. Airapetian, Z. Mikić +1

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