Search Results - "Thalmann, J. K."
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Magnetic Helicity Estimations in Models and Observations of the Solar Magnetic Field. IV. Application to Solar Observations
Published in The Astrophysical journal (01-11-2021)“…Abstract In this ISSI-supported series of studies on magnetic helicity in the Sun, we systematically implement different magnetic helicity calculation methods…”
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How Should One Optimize Nonlinear Force-Free Coronal Magnetic Field Extrapolations from SDO/HMI Vector Magnetograms?
Published in Solar physics (01-11-2012)“…The Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Observatory (SDO) provides photospheric vector magnetograms with a high spatial and…”
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Statistical Properties of Ribbon Evolution and Reconnection Electric Fields in Eruptive and Confined Flares
Published in Solar physics (01-03-2018)“…A statistical study of the chromospheric ribbon evolution in H α two-ribbon flares was performed. The data set consists of 50 confined (62%) and eruptive (38%)…”
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FORCE-FREE FIELD MODELING OF TWIST AND BRAIDING-INDUCED MAGNETIC ENERGY IN AN ACTIVE-REGION CORONA
Published in The Astrophysical journal (01-01-2014)“…The theoretical concept that braided magnetic field lines in the solar corona may dissipate a sufficient amount of energy to account for the brightening…”
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Nonlinear Force-free Field Modeling of a Solar Active Region around the Time of a Major Flare and Coronal Mass Ejection
Published in The Astrophysical journal (10-03-2008)“…Solar flares and coronal mass ejections are associated with rapid changes in field connectivity and are powered by the partial dissipation of electrical…”
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TEMPORAL AND SPATIAL RELATIONSHIP OF FLARE SIGNATURES AND THE FORCE-FREE CORONAL MAGNETIC FIELD
Published in The Astrophysical journal (01-08-2016)“…ABSTRACT We investigate the plasma and magnetic environment of active region NOAA 11261 on 2011 August 2 around a GOES M1.4 flare/CME (SOL2011-08-02T06:19). We…”
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Estimating the Relative Helicity of Coronal Magnetic Fields
Published in Solar physics (01-09-2011)“…To quantify changes of the solar coronal field connectivity during eruptive events, one can use magnetic helicity, which is a measure of the shear or twist of…”
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Can We Improve the Preprocessing of Photospheric Vector Magnetograms by the Inclusion of Chromospheric Observations?
Published in Solar physics (01-02-2008)“…The solar magnetic field is key to understanding the physical processes in the solar atmosphere. Nonlinear force-free codes have been shown to be useful in…”
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Probing the solar coronal magnetic field with physics-informed neural networks
Published in Nature astronomy (01-10-2023)“…While the photospheric magnetic field of our Sun is routinely measured, its extent into the upper atmosphere is typically not accessible by direct…”
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Magnetic Helicity Evolution and Eruptive Activity in NOAA Active Region 11158
Published in The Astrophysical journal (01-10-2022)“…Abstract Coronal mass ejections are among the Sun’s most energetic activity events yet the physical mechanisms that lead to their occurrence are not yet fully…”
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Magnetic Helicity Estimations in Models and Observations of the Solar Magnetic Field. III. Twist Number Method
Published in The Astrophysical journal (01-05-2017)“…We study the writhe, twist, and magnetic helicity of different magnetic flux ropes, based on models of the solar coronal magnetic field structure. These…”
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THE INFLUENCE OF SPATIAL RESOLUTION ON NONLINEAR FORCE-FREE MODELING
Published in The Astrophysical journal (01-10-2015)“…ABSTRACT The nonlinear force-free field (NLFFF) model is often used to describe the solar coronal magnetic field, however a series of earlier studies revealed…”
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The Causes of Quasi-homologous CMEs
Published in The Astrophysical journal (01-08-2017)“…In this paper, we identified the magnetic source locations of 142 quasi-homologous (QH) coronal mass ejections (CMEs), of which 121 are from solar cycle (SC)…”
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ARCADE IMPLOSION CAUSED BY A FILAMENT ERUPTION IN A FLARE
Published in The Astrophysical journal (20-12-2016)“…ABSTRACT Coronal implosions-the convergence motion of plasmas and entrained magnetic field in the corona due to a reduction in magnetic pressure-can help to…”
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COMPARISON OF FORCE-FREE CORONAL MAGNETIC FIELD MODELING USING VECTOR FIELDS FROM HINODE AND SOLAR DYNAMICS OBSERVATORY
Published in The Astrophysical journal (20-05-2013)“…Photospheric magnetic vector maps from two different instruments are used to model the nonlinear force-free coronal magnetic field above an active region. We…”
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Stability of the coronal magnetic field around large confined and eruptive solar flares
Published 19-02-2024“…A&A 686, A115 (2024) In order to improve our understanding on the pre-requisites of eruptive solar flares, we study and compare different measures that…”
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The effect of spatial sampling on magnetic field modeling and helicity computation
Published 04-05-2022“…A&A 662, A3 (2022) Nonlinear force-free (NLFF) modeling is regularly used in order to indirectly infer the 3D geometry of the coronal magnetic field, not…”
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Magnetic helicity and energy budget around large confined and eruptive solar flares
Published 16-06-2021“…A&A 653, A69 (2021) We investigate the coronal magnetic energy and helicity budgets of ten solar ARs, around the times of large flares. In particular, we are…”
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Tracking magnetic flux and helicity from Sun to Earth -- Multi-spacecraft analysis of a magnetic cloud and its solar source
Published 05-10-2022“…A&A 669, A72 (2023) We analyze the complete chain of effects caused by a solar eruptive event in order to better understand the dynamic evolution of…”
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Magnetic helicity budget of solar active regions prolific of eruptive and confined flares
Published 15-10-2019“…We compare the coronal magnetic energy and helicity of two solar active regions (ARs), prolific in major eruptive (AR~11158) and confined (AR~12192) flaring,…”
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