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Innovative and automated method for vortex identification: II. Application to numerical simulations of the solar atmosphere

Astronomy and astrophysics (Berlin), 2024-02, Vol.682, p.A181

2024

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Hα Surges Initiated by Newly-emerging Satellite Magnetic Fields

Chinese astronomy and astrophysics, 2014-01, Vol.38 (1), p.65-74

2014

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Numerical solutions to linear transfer problems of polarized radiation: II. Krylov methods and matrix-free implementation

Astronomy and astrophysics (Berlin), 2021-11, Vol.655, p.A88

2021

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A first look at the submillimeter Sun with ALMA

Astronomy and astrophysics (Berlin), 2022-05, Vol.661, p.L4

2022

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ELLERMAN BOMBS at HIGH RESOLUTION. IV. VISIBILITY in NaI and MgI

The Astrophysical journal, 2015-08

2015

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Dark halos around solar active regions: I. Emission properties of the dark halo around NOAA 12706

Astronomy and astrophysics (Berlin), 2023-12, Vol.680, p.A61

2023

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Anisotropic nonthermal motions in the transition region of solar active regions

Astronomy and astrophysics (Berlin), 2022-04, Vol.660, p.A3

2022

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Numerical solutions to linear transfer problems of polarized radiation: IV. Efficient preconditioning in a physics-based framework

Astronomy and astrophysics (Berlin), 2024-02, Vol.682, p.A68

2024

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Spectroscopic observation of a transition region network jet

Astronomy and astrophysics (Berlin), 2022-04, Vol.660, p.A116

2022

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High-resolution Observations of Dynamics of Superpenumbral H Fibrils

The Astrophysical journal, 2019-08, Vol.880 (2)

2019

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The Dark Side of Penumbral Microjets: Observations in H

The Astrophysical journal, 2019-05, Vol.876 (1)

2019

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Power distribution of oscillations in the atmosphere of a plage region: Joint observations with ALMA, IRIS, and SDO

Astronomy and astrophysics (Berlin), 2022-05, Vol.661, p.A95

2022

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Inelastic O+H collisions and the O I 777 nm solar centre-to-limb variation

Astronomy and astrophysics (Berlin), 2018-08, Vol.616, p.A89

2018

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THE DYNAMICS OF RAPID REDSHIFTED AND BLUESHIFTED EXCURSIONS IN THE SOLAR H LINE

The Astrophysical journal, 2015-03, Vol.802 (1)

2015

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The Spectral Content of SDO/AIA 1600 and 1700 Filters from Flare and Plage Observations

The Astrophysical journal, 2019-01, Vol.870 (2), p.114

2019

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A comparative study of resistivity models for simulations of magnetic reconnection in the solar atmosphere: II. Plasmoid formation

Astronomy and astrophysics (Berlin), 2024-03, Vol.683, p.A95

2024

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Convective blueshifts in the solar atmosphere: I. Absolute measurements with LARS of the spectral lines at 6302 Å

Astronomy and astrophysics (Berlin), 2018-03, Vol.611, p.A4

2018

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Millimeter radiation from a 3D model of the solar atmosphere: I. Diagnosing chromospheric thermal structure

Astronomy and astrophysics (Berlin), 2015-03, Vol.575, p.A15

2015

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Modeling the scattering polarization of the solar Ca I 4227 Å line with angle-dependent partial frequency redistribution

Astronomy and astrophysics (Berlin), 2021-11, Vol.655, p.A13

2021

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The influence of NLTE effects in Fe I lines on an inverted atmosphere: II. 6301 Å and 6302 Å lines formed in 3D NLTE

Astronomy and astrophysics (Berlin), 2021-03, Vol.647, p.A46

2021

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Evolution of dynamic fibrils from the cooler chromosphere to the hotter corona

Astronomy and astrophysics (Berlin), 2023-10, Vol.678, p.L5

2023

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Categorization model of moving small-scale intensity enhancements in solar active regions

Astronomy and astrophysics (Berlin), 2022-06, Vol.662, p.A30

2022

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Efficient Radiative Transfer for Dynamically Evolving Stratified Atmospheres ∗ The National Center for Atmospheric Research is sponsored by the National Science Foundation

The Astrophysical journal, 2017-12, Vol.851 (1)

Judge, Philip G.

2017

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ALFVÉNIC WAVE HEATING OF THE UPPER CHROMOSPHERE IN FLARES

Astrophysical journal. Letters, 2016-02, Vol.818 (1), p.L20

2016

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Solar Hα features with hot onsets

Astronomy and astrophysics (Berlin), 2017, Vol.597

2017

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Innovative and automated method for vortex identification: II. Application to numerical simulations of the solar atmosphere

Hα Surges Initiated by Newly-emerging Satellite Magnetic Fields

Numerical solutions to linear transfer problems of polarized radiation: II. Krylov methods and matrix-free implementation

A first look at the submillimeter Sun with ALMA

ELLERMAN BOMBS at HIGH RESOLUTION. IV. VISIBILITY in NaI and MgI

Dark halos around solar active regions: I. Emission properties of the dark halo around NOAA 12706

Anisotropic nonthermal motions in the transition region of solar active regions

Numerical solutions to linear transfer problems of polarized radiation: IV. Efficient preconditioning in a physics-based framework

Spectroscopic observation of a transition region network jet

High-resolution Observations of Dynamics of Superpenumbral H Fibrils

The Dark Side of Penumbral Microjets: Observations in H

Power distribution of oscillations in the atmosphere of a plage region: Joint observations with ALMA, IRIS, and SDO

Inelastic O+H collisions and the O I 777 nm solar centre-to-limb variation

THE DYNAMICS OF RAPID REDSHIFTED AND BLUESHIFTED EXCURSIONS IN THE SOLAR H LINE

The Spectral Content of SDO/AIA 1600 and 1700 Filters from Flare and Plage Observations

A comparative study of resistivity models for simulations of magnetic reconnection in the solar atmosphere: II. Plasmoid formation

Convective blueshifts in the solar atmosphere: I. Absolute measurements with LARS of the spectral lines at 6302 Å

Millimeter radiation from a 3D model of the solar atmosphere: I. Diagnosing chromospheric thermal structure

Modeling the scattering polarization of the solar Ca I 4227 Å line with angle-dependent partial frequency redistribution

The influence of NLTE effects in Fe I lines on an inverted atmosphere: II. 6301 Å and 6302 Å lines formed in 3D NLTE

Evolution of dynamic fibrils from the cooler chromosphere to the hotter corona

Categorization model of moving small-scale intensity enhancements in solar active regions

Efficient Radiative Transfer for Dynamically Evolving Stratified Atmospheres ∗ The National Center for Atmospheric Research is sponsored by the National Science Foundation

ALFVÉNIC WAVE HEATING OF THE UPPER CHROMOSPHERE IN FLARES

Solar Hα features with hot onsets

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