Fine Structure and Dynamics of the Solar Photosphere (IAU S327)

Erscheinungsjahr 2017
ISBN: 978-1-107-17004-9
Verlag: Cambridge University Press

Buch, Englisch, 500 Seiten, Format (B × H): 254 mm x 179 mm, Gewicht: 414 g

Reihe: Proceedings of the International Astronomical Union Symposia and Colloquia

Solar activity has become of increasing importance in our modern society, as many aspects of today's technology could be affected by eruptive phenomena associated with solar magnetic variability. State of the art solar instrumentation is revealing the dynamics of the Sun with unprecedented temporal and spatial resolutions. This volume includes recent results in solar physics research presented at the IAU Symposium 327, the first IAU symposium held in Colombia, in the historical city of Cartagena de Indias, one of the oldest in the Americas. Its main scientific goal was to discuss recent results on the processes shaping the structure of the solar atmosphere and driving plasma eruptions and explosive events in our star. Researchers in both theory and observation, who study structure and activity in the solar atmosphere, discuss a wide range of topics in the field.

Autoren/Hrsg.

Vargas Domínguez, Santiago

Kosovichev, Alexander G.

Antolin, Patrick

Harra, Louise

Fachgebiete

• Naturwissenschaften Astronomie Astronomie: Allgemeines
• Naturwissenschaften Physik Angewandte Physik Astrophysik
• Technische Wissenschaften Sonstige Technologien | Angewandte Technik Weltraumforschung
• Naturwissenschaften Physik Thermodynamik Plasmaphysik
• Naturwissenschaften Physik Angewandte Physik Umweltphysik
• Naturwissenschaften Astronomie Astrophysik

Inhaltsverzeichnis

Solar ALMA predictions: tutorial R. J. Rutten; First Colombian Solar Radio Interferometer: current stage J. C. G. G´omez, J. C. M. Oliveros and B. Calvo-Mozo; sTools - a data reduction pipeline for the GREGOR Fabry-Pérot Interferometer and the High-resolution Fast Imager at the GREGOR solar telescope C. Kuckein et al.; A Python-based interface to examine motions in time series of solar images J. I. Campos-Rozo and S. V. Domínguez; Flows along arch filaments observed in the GRIS 'very fast spectroscopic mode' S. J. G. Manrique et al.; Granular cells in the presence of magnetic field J. Jurcák, B. Lemmerer and M. van Noort; Small magnetic structures near the polar regions of the Sun I. Cabello et al.; A new look at sunspot formation using theory and observations I. R. Losada et al.; A long-duration active region: Evolution and quadrature observations of ejective events H. Cremades et al.; Photospheric magnetic field of an eroded-by-solar-wind coronal mass ejection J. Palacios, C. Cid, E. Saiz and A. Guerrero; Magnetic instability of filaments in different solar regions J. Palacios et al.; Magnetic field line braiding in the solar atmosphere S. Candelaresi, D. I. Pontin and G. Hornig; Modelling short-term Solar Spectral Irradiance (SSI) using coronal electron density and temperature profiles based on solar magnetic field observations J. M. R. Gómez et al.; P-mode induced convective collapse in vertical expanding magnetic flux tubes? D. Utz et al.; Understanding the connection between the energy released during solar flares and their emission in the lower atmosphere F. R. da Costa; Initiation and chromospheric effects of a M1.0 class solar flare from high-resolution multi-wavelength observations V. M. Sadykov et al.; An Eruptive Complex Solar Flare and Events in its Aftermath M. L. Luoni et al.; What can He II 304 Å tell us about transient seismic emission from solar flares? C. Lindsey and A.-C. Donea; Relationships Between Sequential Chromospheric Brightening and the Corona M. S. Kirk et al.; MHD simulations of coronal dark downflows considering thermal conduction E. Zurbriggen et al.; Evidence of in-situ Type II radio bursts in interplanetary shocks S. M. D´iaz-Castillo, J. C. M. Oliveros and B. Calvo-Mozo; Author index.