Borrero, J. M.; Martinez-Pillet, V.; Schlichenmaier, R.; Solanki, S. K.; Bonet, J. A.; del Toro Iniesta, J. C.; Schmidt, W.; Barthol, P.; Gandorfer, A.; Domingo, V.et al.; Knoelker, M.: Supersonic Magnetic Upflows in Granular Cells Observed with SUNRISE/IMaX. Astrophysical Journal 723 (2), pp. L144 - L148 (2010)
Borrero, J. M.; Rempel, M.; Solanki, S. K.: Spectropolarimetric analysis of 3D MHD sunspot simulations. Astron. Nachrichten 331 (6), pp. 567 - 569 (2010)
Borrero, J. M.: The structure of sunspot penumbrae - IV. MHS equilibrium for penumbral flux tubes and the origin of dark core penumbral filaments and penumbral grains. Astronomy and Astrophysics 471, pp. 967 - 975 (2007)
Borrero, J. M.; Solanki, S. K.; Lagg, A.; Socas-Navarro, H.; Lites, B.: On the fine structure of sunspot penumbrae: III. The vertical extension of penumbral filaments. Astronomy and Astrophysics 450, pp. 383 - 393 (2006)
Borrero, J. M.; Bellot Rubio, L. R.; Barklem, P. S.; Del Toro Iniesta, J. C.: Accurate atomic parameters for near-infrared spectral lines. Astronomy and Astrophysics 404, p. 749 (2003)
Bellot Rubio, L. R.; Borrero, J. M.: Iron abundance in the solar photosphere. Application of a two-component model atmosphere. Astronomy and Astrophysics 391 (3), pp. 331 - 337 (2002)
Borrero, J. M.; Rubio, L. R. B.: A two-component model of the solar photosphere from the inversion of spectral lines. Astronomy and Astrophysics 385 (3), pp. 1056 - 1072 (2002)
Borrero, J. M.; Lagg, A.; Solanki, S. K.; Frutiger, C.; Collados, M.; Bellot Rubio, L. R.: Modeling the Fine Structure of a Sunspot Penumbra through the Inversion of Stokes Profiles. Astronomical Society of the Pacific, pp. 235 - 242 (2003)
Borrero, J. M.; Lagg, A.; Solanki, S. K.; Frutiger, C.; Collados, M.; Bellot Rubio, L. R.: Modeling the Fine Structure of a Sunspot Penumbra through the Inversion of Stokes Profiles. In: Current Theoretical Models and Future High Resolution Solar Observations: Preparing for ATST, p. 235 (Eds. Pevtsov, A. A.; Uitenbroek, H.). (2003)
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