Search Results - "Durán, J. S. Castellanos"
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Detection of the Strongest Magnetic Field in a Sunspot Light Bridge
Published in The Astrophysical journal (01-06-2020)“…Traditionally, the strongest magnetic fields on the Sun have been measured in sunspot umbrae. More recently, however, much stronger fields have been measured…”
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2
Expulsion of Counter Evershed Flows from Sunspot Penumbrae
Published in The Astrophysical journal (01-08-2023)“…Abstract In addition to the Evershed flow directed from the umbra toward the outer boundary of a sunspot, under special circumstances a counter Evershed flow…”
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3
A Statistical Study of Photospheric Magnetic Field Changes During 75 Solar Flares
Published in The Astrophysical journal (01-01-2018)“…Abrupt and permanent changes of photospheric magnetic fields have been observed during solar flares. The changes seem to be linked to the reconfiguration of…”
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4
Expulsion of counter Evershed flows from sunspot penumbrae
Published 31-05-2023“…In addition to the Evershed flow directed from the umbra towards the outer boundary of the sunspot, under special circumstances, a counter Evershed flow (CEF)…”
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5
The MODEST catalog of depth-dependent spatially coupled inversions of sunspots observed by Hinode/SOT-SP
Published 11-03-2024“…A&A 687, A218 (2024) We present a catalog that we named MODEST containing depth-dependent information on the atmospheric conditions inside sunspot groups of…”
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The Statistical Relationship between White-light Emission and Photospheric Magnetic Field Changes in Flares
Published 06-07-2020“…Continuum emission, also called white-light emission (WLE), and permanent changes of the magnetic field ($\Delta{B}_{{\rm{LOS}}}$) are often observed during…”
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The non-LTE formation of the Fe I 6173 A line in the solar atmosphere
Published 18-11-2022“…A&A 669, A144 (2023) The current analysis is dedicated to a detailed investigation of the non-Local Thermodynamic Equilibrium (NLTE) effects influencing the…”
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Fast downflows in a chromospheric filament
Published 13-12-2019“…Proc. IAU 15 (2019) 454-457 An active region filament in the upper chromosphere is studied using spectropolarimetric data in He I 10830 A from the GREGOR…”
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Detection of the strongest magnetic field in a sunspot light bridge
Published 06-07-2020“…Traditionally, the strongest magnetic fields on the Sun have been measured in sunspot umbrae. More recently, however, much stronger fields have been measured…”
Get full text
Journal Article -
10
A Statistical Study of Photospheric Magnetic Field Changes During 75 Solar Flares
Published 16-01-2018“…Astrophysical Journal 2018 Abrupt and permanent changes of photospheric magnetic fields have been observed during solar flares. The changes seem to be linked…”
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11
texttt{globin}$: A spectropolarimetric inversion code for the coupled inference of atomic line parameters
Published 04-04-2024“…A&A 686, A262 (2024) For many transitions, atomic data, such as the oscillator strength (log(gf)) and the central wavelength of the line, are poorly…”
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Magnetized supersonic downflows in the chromosphere. A statistical study using the He I 10830 \r{A} lines
Published 23-02-2022“…A&A 661, A122 (2022) The chromosphere above active regions (ARs) on the Sun hosts magnetized supersonic downflows. Studies of these supersonic downflows help…”
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Ti I lines at 2.2 ${\mu}$m as probes of the cool parts of sunspots
Published 02-07-2021“…A&A 653, A91 (2021) The sunspot umbra harbors the coolest plasma on the solar surface due to the presence of strong magnetic fields. The routinely used atomic…”
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Metadata and their importance in SO/PHI's on-board data processing
Published 17-12-2019“…To cope with the telemetry limitations, the Polarimetric and Helioseismic Imager on Solar Orbiter does full on-board data processing. Metadata are central to…”
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Performance analysis of the SO/PHI software framework for on-board data reduction
Published 21-05-2019“…Astronomical Data Analysis Software and Systems XXVIII, Volume: 523, Year: 2019 The Polarimetric and Helioseismic Imager (PHI) is the first deep-space solar…”
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