Volume 86, Number 3, May 2009
|Number of page(s)||4|
|Section||Geophysics, Astronomy and Astrophysics|
|Published online||18 May 2009|
A new paradigm for solar coronal heating
K. U. Leuven, Center for Plasma Astrophysics - Celestijnenlaan 200B, 3001 Leuven, Belgium, EU and Leuven Mathematical Modeling and Computational Science Center (LMCC) - Leuven, Belgium, EU
Corresponding author: firstname.lastname@example.org
Accepted: 20 April 2009
The solar coronal heating problem refers to the question why the temperature of the Sun's corona is more than two orders of magnitude higher than that of its surface. Almost 70 years after the discovery, this puzzle is still one of the major challenges in astrophysics. The current basic paradigm of coronal heating is unable to explain all the observational features of heating. Here we argue that a new paradigm is required to solve the puzzle in a self-consistent manner. The alternative approach is based on the kinetic theory of drift waves. We show that, with qualitative and quantitative arguments, the drift waves have the potential to satisfy all coronal heating requirements.
PACS: 96.60.-j – Solar physics / 96.60.P- – Corona / 52.35.Kt – Drift waves
© EPLA, 2009
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.