F
Fernando Moreno-Insertis
Researcher at University of La Laguna
Publications - 98
Citations - 5546
Fernando Moreno-Insertis is an academic researcher from University of La Laguna. The author has contributed to research in topics: Magnetic flux & Magnetohydrodynamics. The author has an hindex of 37, co-authored 95 publications receiving 5156 citations. Previous affiliations of Fernando Moreno-Insertis include Spanish National Research Council.
Papers
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Journal ArticleDOI
Emerging flux tubes in the solar convection zone. 1: Asymmetry, tilt, and emergence latitude
Journal ArticleDOI
Solar coronal jets: Observations, theory, and modeling
N.-E. Raouafi,Spiros Patsourakos,Etienne Pariat,Peter R. Young,Peter R. Young,Alphonse C. Sterling,Antonia Savcheva,Masumi Shimojo,Fernando Moreno-Insertis,C. R. DeVore,Vasilis Archontis,Tibor Torok,Helen E. Mason,Werner Curdt,Karen A. Meyer,Kévin Dalmasse,Y. Matsui +16 more
TL;DR: In this paper, the authors studied the behavior of coronal jets, which are the source of significant mass and energy input to the upper solar atmosphere and the solar wind, and provided critical insight for understanding the larger, more complex drivers of the solar activity.
Journal ArticleDOI
Emergence of magnetic flux from the convection zone into the corona
Vasilis Archontis,Fernando Moreno-Insertis,Fernando Moreno-Insertis,K. Galsgaard,K. Galsgaard,A. W. Hood,E. O'Shea +6 more
TL;DR: In this paper, the authors used idealized models for the initial stratification and magnetic field distribution below the photosphere similar to those used for multidimensional flux emergence experiments in the literature.
Journal ArticleDOI
Jets in Coronal Holes: Hinode Observations and Three-dimensional Computer Modeling
TL;DR: In this paper, a three-dimensional numerical experiment of flux emergence from the solar interior into a coronal hole and compare them with simultaneous XRT and EIS observations of a jet-launching event that accompanied the appearance of a bipolar region in MDI magnetograms.
Journal ArticleDOI
Jets in coronal holes: Hinode observations and 3D computer modelling
TL;DR: In this paper, a 3D numerical experiment of flux emergence from the solar interior into a coronal hole and compare them with simultaneous XRT and EIS observations of a jet-launching event that accompanied the appearance of a bipolar region in MDI magnetograms is presented.