Search Results - "Durán, J. S. Castellanos"

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  1. 1

    Detection of the Strongest Magnetic Field in a Sunspot Light Bridge by Durán, J. S. Castellanos, Lagg, Andreas, Solanki, Sami K., Noort, Michiel van

    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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    Journal Article
  2. 2

    Expulsion of Counter Evershed Flows from Sunspot Penumbrae by Castellanos Durán, J. S., Korpi-Lagg, A., Solanki, S. K.

    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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    Journal Article
  3. 3

    A Statistical Study of Photospheric Magnetic Field Changes During 75 Solar Flares by Castellanos Durán, J. S., Kleint, L., Calvo-Mozo, B.

    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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    Journal Article
  4. 4

    Expulsion of counter Evershed flows from sunspot penumbrae by Durán, J. S. Castellanos, Korpi-Lagg, A, Solanki, S. K

    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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    Journal Article
  5. 5

    The MODEST catalog of depth-dependent spatially coupled inversions of sunspots observed by Hinode/SOT-SP by Durán, J. S. Castellanos, Milanovic, N, Korpi-Lagg, A, Löptien, B, van Noort, M, Solanki, S. K

    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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    Journal Article
  6. 6

    The Statistical Relationship between White-light Emission and Photospheric Magnetic Field Changes in Flares by Durán, J. S. Castellanos, Kleint, L

    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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    Journal Article
  7. 7

    The non-LTE formation of the Fe I 6173 A line in the solar atmosphere by Smitha, H. N, van Noort, M, Solanki, S. K, Durán, J. S. Castellanos

    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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  8. 8

    Fast downflows in a chromospheric filament by Sowmya, K, Lagg, A, Solanki, S. K, Durán, J. S. Castellanos

    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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  9. 9

    Detection of the strongest magnetic field in a sunspot light bridge by Durán, J. S. Castellanos, Lagg, A, Solanki, S. K, van Noort, M

    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. 10

    A Statistical Study of Photospheric Magnetic Field Changes During 75 Solar Flares by Durán, J. S. Castellanos, Kleint, L, Calvo-Mozo, B

    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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    Journal Article
  11. 11

    texttt{globin}$: A spectropolarimetric inversion code for the coupled inference of atomic line parameters by Vukadinović, D, Smitha, H. N, Korpi-Lagg, A, van Noort, M, Durán, J. S. Castellanos, Solanki, S. K

    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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  12. 12

    Magnetized supersonic downflows in the chromosphere. A statistical study using the He I 10830 \r{A} lines by Sowmya, K, Lagg, A, Solanki, S. K, Durán, J. S. Castellanos

    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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  13. 13

    Ti I lines at 2.2 ${\mu}$m as probes of the cool parts of sunspots by Smitha, H. N, Durán, J. S. Castellanos, Solanki, S. K, Tiwari, S. K

    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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  14. 14

    Metadata and their importance in SO/PHI's on-board data processing by Albert, K, Hirzberger, J, Busse, D, Durán, J. S. Castellanos, Gutierrez-Marques, P, Kolleck, M

    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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  15. 15

    Performance analysis of the SO/PHI software framework for on-board data reduction by Albert, K, Hirzberger, J, Busse, D, Rodríguez, J. Blanco, Durán, J. S. Castellanos, Carrascosa, J. P. Cobos, Fiethe, B, Gandorfer, A, Guan, Y, Kolleck, M, Lagg, A, Lange, T, Michalik, H, Solanki, S. K, Iniesta, J. C. del Toro, Woch, J

    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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