R
Reza Rezaei
Researcher at Spanish National Research Council
Publications - 112
Citations - 2773
Reza Rezaei is an academic researcher from Spanish National Research Council. The author has contributed to research in topics: Sunspot & Photosphere. The author has an hindex of 32, co-authored 112 publications receiving 2531 citations. Previous affiliations of Reza Rezaei include University of Shahrood & University of La Laguna.
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The formation of a sunspot penumbra
TL;DR: In this article, the formation of a penumbra in the leading spot was observed at a cadence of 5 images per second for the next 4:40 h, interrupted by one large gap of 35 min and a few more small gaps of about 10 min.
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Detection of vortex tubes in solar granulation from observations with sunrise
Oskar Steiner,M. Franz,N. Bello González,Ch. Nutto,Reza Rezaei,V. Martínez Pillet,J. A. Bonet Navarro,J. C. del Toro Iniesta,V. Domingo,Sami K. Solanki,Sami K. Solanki,M. Knölker,W. Schmidt,Peter Barthol,Achim Gandorfer +14 more
TL;DR: In this paper, the authors investigated a time series of continuum intensity maps and corresponding Dopplergrams of granulation in a very quiet solar region at the disk center, recorded with the Imaging Magnetograph eXperiment (IMaX) on board the balloon-borne solar observatory SUNRISE.
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The horizontal internetwork magnetic field : numerical simulations in comparison to observations with hinode
TL;DR: In this article, the authors investigate realistic numerical simulations of the surface layers of the Sun with respect to horizontal magnetic fields and compute the corresponding polarimetric response in the Fe i 630 nm line pair.
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Relation between photospheric magnetic field and chromospheric emission
TL;DR: In this paper, the authors investigated the relationship between the photospheric magnetic field and the emission of the mid chromosphere of the Sun and found that a dominant fraction of the calcium emission caused by the heated atmosphere in the magnetic network has non-magnetic origin.
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The signature of chromospheric heating in Ca II H spectra
TL;DR: In this paper, the authors analyzed a 1-h time series of cospatial Call H intensity spectra and photospheric polarimetric spectra around 630 nm to derive the signature of the chromospheric heating process in the spectra.