The continuum intensity as a function of magnetic field II. Local magnetic flux and convective flows
2012
Abstract
Context. To deepen our understanding of the role of small-scale magnetic fields in active regions (ARs) and in the quiet Sun (QS) on the solar irradiance, it is fundamental to investigate the physical processes underlying their continuum brightness. Previous results showed that magnetic elements in the QS reach larger continuum intensities than in ARs at disk center, but left this difference unexplained.
Details
Title
The continuum intensity as a function of magnetic field II. Local magnetic flux and convective flows
Author(s)
Kobel, P. ; Solanki, S. K. ; Borrero, J. M.
Published in
Astronomy & Astrophysics
Volume
542
Pages
A96
Date
2012
Keywords
Other identifier(s)
View record in Web of Science
Laboratories
LMH
Record Appears in
Scientific production and competences > STI - School of Engineering > STI Archives > LMH - Laboratory for Hydraulic Machines
Peer-reviewed publications
Work produced at EPFL
Journal Articles
Published
Peer-reviewed publications
Work produced at EPFL
Journal Articles
Published
Record creation date
2012-07-27