Search Results - "Schrijver, Carolus J."
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Testing the Solar Activity Paradigm in the Context of Exoplanet Transits
Published in The Astrophysical journal (20-02-2020)“…Transits of exoplanets across cool stars contain blended information about structures on the stellar surface and about the planetary body and atmosphere. To…”
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THE NONPOTENTIALITY OF CORONAE OF SOLAR ACTIVE REGIONS, THE DYNAMICS OF THE SURFACE MAGNETIC FIELD, AND THE POTENTIAL FOR LARGE FLARES
Published in The Astrophysical journal (01-04-2016)“…ABSTRACT Flares and eruptions from solar active regions (ARs) are associated with atmospheric electrical currents accompanying distortions of the coronal field…”
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Extreme solar events
Published in Living reviews in solar physics (01-12-2022)“…We trace the evolution of research on extreme solar and solar-terrestrial events from the 1859 Carrington event to the rapid development of the last twenty…”
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The Characteristics of Solar X-Class Flares and CMEs: A Paradigm for Stellar Superflares and Eruptions?
Published in Solar physics (01-08-2016)“…This paper explores the characteristics of 42 solar X-class flares that were observed between February 2011 and November 2014, with data from the Solar…”
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Sun-as-a-star Spectral Irradiance Observations of Transiting Active Regions
Published in The Astrophysical journal (01-10-2020)“…Major solar flares are prone to occur in active-region (AR) atmospheres associated with large, complex, dynamically evolving sunspots. This points to the…”
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A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953
Published in The Astrophysical journal (10-05-2009)“…Nonlinear force-free field (NLFFF) models are thought to be viable tools for investigating the structure, dynamics, and evolution of the coronae of solar…”
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Bright Hot Impacts by Erupted Fragments Falling Back on the Sun: A Template for Stellar Accretion
Published in Science (American Association for the Advancement of Science) (19-07-2013)“…Impacts of falling fragments observed after the eruption of a filament in a solar flare on 7 June 2011 are similar to those inferred for accretion flows on…”
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Observations and Modeling of the Early Acceleration Phase of Erupting Filaments Involved in Coronal Mass Ejections
Published in The Astrophysical journal (10-02-2008)“…We examine the early phases of two near-limb filament destabilizatlons involved in coronal mass ejections (CMEs) on 2005 June 16 and July 27, using…”
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Nonlinear Force-Free Modeling of Coronal Magnetic Fields Part I: A Quantitative Comparison of Methods
Published in Solar physics (01-05-2006)“…We compare six algorithms for the computation of nonlinear force-free (NLFF) magnetic fields (including optimization, magnetofrictional, Grad-Rubin based, and…”
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Nonlinear Force-Free Modeling of Coronal Magnetic Fields. II. Modeling a Filament Arcade and Simulated Chromospheric and Photospheric Vector Fields
Published in Solar physics (01-02-2008)“…We compare a variety of nonlinear force-free field (NLFFF) extrapolation algorithms, including optimization, magneto-frictional, and Grad – Rubin-like codes,…”
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The Global Solar Magnetic Field Through a Full Sunspot Cycle: Observations and Model Results
Published in Solar physics (01-10-2008)“…Based on 11 years of SOHO/MDI observations from the cycle minimum in 1997 to the next minimum around 2008, we compare observed and modeled axial dipole moments…”
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Blind Stereoscopy of the Coronal Magnetic Field
Published in Solar physics (01-10-2015)“…We test the feasibility of 3D coronal-loop tracing in stereoscopic EUV image pairs, with the ultimate goal of enabling efficient 3D reconstruction of the…”
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Braiding-induced Interchange Reconnection of the Magnetic Field and the Width of Solar Coronal Loops
Published in The Astrophysical journal (20-06-2007)“…The random walk of the footpoints of coronal loops in the rapidly evolving solar granulation is expected to cause braiding of the field, which in turn should…”
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MAGNETIC PROPERTIES OF SOLAR ACTIVE REGIONS THAT GOVERN LARGE SOLAR FLARES AND ERUPTIONS
Published in The Astrophysical journal (01-01-2017)“…ABSTRACT Solar flares and coronal mass ejections (CMEs), especially the larger ones, emanate from active regions (ARs). With the aim of understanding the…”
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Magnetic Field Topology and the Thermal Structure of the Corona over Solar Active Regions
Published in The Astrophysical journal (20-08-2010)“…Solar extreme ultraviolet (EUV) images of quiescent active-region coronae are characterized by ensembles of bright 1-2 MK loops that fan out from select…”
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The Magnetic Connection between the Solar Photosphere and the Corona
Published in The Astrophysical journal (10-11-2003)Get full text
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The Properties of Small Magnetic Regions on the Solar Surface and the Implications for the Solar Dynamo(s)
Published in The Astrophysical journal (20-02-2003)Get full text
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The Nonpotentiality of Active-Region Coronae and the Dynamics of the Photospheric Magnetic Field
Published in The Astrophysical journal (20-07-2005)“…The magnetic field in the solar photosphere frequently carries strong electric currents, even though the global coronal configuration often resembles a…”
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The Coronal Heating Mechanism as Identified by Full-Sun Visualizations
Published in The Astrophysical journal (01-11-2004)“…We constrain the properties of the mechanism(s) responsible for the bulk of the heating of the corona of the Sun by simulating, for the first time, the…”
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On the Formation of Polar Spots in Sun-like Stars
Published in The Astrophysical journal (20-04-2001)Get full text
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