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    Article

    Solar Coronal Jets: Observations, Theory, and Modeling

    Coronal jets represent important manifestations of ubiquitous solar transients, which may be the source of significant mass and energy input to the upper solar atmosphere and the solar wind. While the energy i...

    N. E. Raouafi, S. Patsourakos, E. Pariat, P. R. Young in Space Science Reviews (2016)

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    Article

    The Emergence of Magnetic Field into Stellar Atmospheres

    The magnetic activity in the atmosphere of the Sun, possibly of most other magnetically active late-type stars, is a consequence of the emergence of magnetic flux from the stellar interior. Research in this fi...

    F. Moreno-Insertis in Astrophysics and Space Science (2004)

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    Chapter

    The Emergence of Magnetic Field into Stellar Atmospheres

    The magnetic activity in the atmosphere of the Sun, possibly of most other magnetically active late-type stars, is a consequence of the emergence of magnetic flux from the stellar interior. Research in this fi...

    F. Moreno-Insertis in Magnetic Fields and Star Formation (2004)

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    Article

    Active region asymmetry as a result of the rise of magnetic flux tubes

    The magnetic flux tubes that rise across the convection zone to produce active regions are shown to develop a difference in inclination between their preceding and follower sides. This asymmetry is such that t...

    F. Moreno-insertis, P. Caligari, M. Schüssler in Solar Physics (1994)

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    Chapter

    Dynamics of Erupting Magnetic Flux Tubes

    The eruption of magnetic flux tubes from the overshoot layer due to instability and the dynamics of their subsequent rise through the solar convection zone are followed by numerical simulation. Special emphasi...

    F. Moreno-Insertis, M. Schüssler, P. Caligari in Solar Surface Magnetism (1994)

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    Chapter and Conference Paper

    Storage of Magnetic Flux in the Overshoot Region

    The combined action of the subadiabatic ambient stratification in the overshoot region below the convection zone and the inertial forces associated with the solar rotation is shown to lead to the suppression o...

    F. Moreno-Insertis, M. Schüssler, A. Ferriz-Mas in The Cosmic Dynamo (1993)

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    Chapter

    The Motion of Magnetic Flux Tubes in the Convection Zone and the Subsurface Origin of Active Regions

    The rise of kink-unstable magnetic flux tubes through the solar convection zone is discussed with a view to explaining the subsurface origin of active regions. In spite of the advances and insights obtained by...

    F. Moreno-Insertis in Sunspots: Theory and Observations (1992)

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    Article

    Decay rates of sunspot groups from 1874 to 1976

    The global behaviour and fine structure of the distribution of sunspot decay rates from activity cycle 13 to 20 are presented. It is shown that the distribution of this parameter is lognormal. Statistically si...

    V. Martinez Pillet, F. Moreno-Insertis, M. Vázquez in Astrophysics and Space Science (1990)

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    Chapter and Conference Paper

    Observations of the birth and fine structure of sunspot penumbrae

    High resolution white-light pictures of sunspot penumbrae are presented. These include pictures showing details of their filamentary structure and some instances of birth of a penumbra. The observations are di...

    M. Collados, J. I. García de la Rosa in High Resolution in Solar Physics (1985)

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    Article

    Geometrical foundations and results on a problem suggested in a paper by Andersonet al.

    F. González-Gascón, F. Moreno-Insertis in Lettere al Nuovo Cimento (1971-1985) (1978)

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    Article

    Symmetries, first integrals and splittability of dynamical systems

    F. González-Gascón, F. Moreno-Insertis in Lettere al Nuovo Cimento (1971-1985) (1978)