B
B. Ruiz Cobo
Researcher at Spanish National Research Council
Publications - 119
Citations - 3765
B. Ruiz Cobo is an academic researcher from Spanish National Research Council. The author has contributed to research in topics: Photosphere & Sunspot. The author has an hindex of 32, co-authored 113 publications receiving 3510 citations. Previous affiliations of B. Ruiz Cobo include IAC & University of Catania.
Papers
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Journal ArticleDOI
Inversion of Stokes profiles
TL;DR: In this paper, an inversion code of Stokes line profiles is presented, which allows the recovery of the stratification of the temperature, the magnetic field vector, and the line of sight velocity through the atmosphere.
Journal ArticleDOI
An open-source, massively parallel code for non-LTE synthesis and inversion of spectral lines and Zeeman-induced Stokes profiles
Hector Socas-Navarro,Hector Socas-Navarro,J. de la Cruz Rodríguez,A. Asensio Ramos,A. Asensio Ramos,J. Trujillo Bueno,J. Trujillo Bueno,B. Ruiz Cobo,B. Ruiz Cobo +8 more
TL;DR: NICOLE as mentioned in this paper is a non-LTE radiative transfer tool for the synthesis and inversion of spectral lines and Zeeman-induced polarization profiles from the photosphere to the chromosphere.
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Non-LTE Inversion of Stokes Profiles Induced by the Zeeman Effect
TL;DR: In this article, a non-LTE inversion code of Stokes profiles induced by the Zeeman effect in magnetized stellar atmospheres is presented for the inference of the thermal, dynamic, and magnetic properties of the solar chromosphere.
Journal ArticleDOI
Optical Tomography of a Sunspot. II. Vector Magnetic Field and Temperature Stratification
C. Westendorp Plaza,J. C. del Toro Iniesta,B. Ruiz Cobo,V. Martínez Pillet,Bruce W. Lites,Andrew Skumanich +5 more
TL;DR: In this article, the Stokes Inversion based on Response Functions (SIR inversion) was applied to a low-noise, full Stokes profile two-dimensional map of the sunspot as observed with the Advanced Stokes Polarimeter.
Journal ArticleDOI
Evidence for a downward mass flux in the penumbral region of a sunspot
C. Westendorp Plaza,J. C. del Toro Iniesta,B. Ruiz Cobo,V. Martínez Pillet,Bruce W. Lites,A. Skumanich +5 more
TL;DR: In this paper, the authors used a recently developed optical tomographic technique to obtain a three-dimensional model of the magnetic field and mass flow in the vicinity of a sunspot and found that some magnetic field lines, together with a significant part of the Evershed mass flux, flow back towards the Sun in the deepest atmospheric layers at the outer edge of the sunspot.