Change search
ReferencesLink to record
Permanent link

Direct link
Effects of rotation and stratification on magnetic flux concentrations
Stockholm University, Faculty of Science, Department of Astronomy. Stockholm University, Nordic Institute for Theoretical Physics (Nordita).
2014 (English)Licentiate thesis, comprehensive summary (Other academic)
Abstract [en]

The formation of magnetic flux concentrations in the Sun is still a matter of debate. One observable manifestations of such concentrations is sunspots. A mechanism able to spontaneously form magnetic flux concentrations in strongly stratified hydromagnetic turbulence and in the presence of a weak magnetic field is the negative effective magnetic pressure instability (NEMPI). This instability is caused by the local suppression of the turbulence by the magnetic field. Due to the complexity of the system, and in order to understand the fundamental physics behind the instability, the study started by considering simplified conditions. In this thesis we aim to move towards the complexity of the Sun. Here we want to know whether the instability can develop under rotation and in the case of a polytropic stratification instead of the simpler isothermal stratification. We perform different kinds of simulations, namely direct numerical simulations (DNS)and mean field simulations (MFS) of strongly stratified turbulence in the presence of weak magnetic fields. We then study separately the effects of rotation and the change in stratification.

It is found that slow rotation can suppress the instability. For Coriolis numbers larger than $0.1$ the MFS no longer result in growth, whereas the DNS start first with adecreaseof the growth rate of the instability % with the speed-up of rotation is alleviated and then, for $\Co > 0.06$, an increase owing to the fact that rotation leads to  the onset of the dynamo instability, which couples with NEMPI in a combined system. In fact, the suppression implies a constraint on the depth where the instability can operate in the Sun. Since rotation is very weak in the uppermost layers of the Sun, the formation of the flux concentration through this instability might be a shallow phenomenon. The same constraint is found when we study the effects of polytropic stratificationon NEMPI. In this case, the instability also develops, but it is much more concentrated in the upper parts of the simulation domain than in the isothermal case. In contrast to the isothermal case, where the density scale height is constant inthe computational domain, polytropic layers decrease their stratification deeper down, so it becomes harder for NEMPI to operate.

With these studies we confirm that NEMPI can form magnetic flux concentrations even in the presence of weak rotation and for polytropic stratification. When applied to the Sun, the effects of rotation and the change of stratification constrain the depth where NEMPI can develop to the uppermost layers, where the rotational influence is weak and the stratification is strong enough.

Place, publisher, year, edition, pages
Stockholm: Department of Astronomy, Stockholm University , 2014. , 56 p.
National Category
Astronomy, Astrophysics and Cosmology
Research subject
URN: urn:nbn:se:su:diva-112879OAI: diva2:781742
2014-12-05, FB42, AlbaNova University Centre, Roslagstullsbacken 21, Stockholm, 10:00 (English)
Available from: 2015-01-19 Created: 2015-01-19 Last updated: 2016-05-16Bibliographically approved

Open Access in DiVA

fulltext(11058 kB)148 downloads
File information
File name FULLTEXT01.pdfFile size 11058 kBChecksum SHA-512
Type fulltextMimetype application/pdf

Search in DiVA

By author/editor
Illa, R. Losada
By organisation
Department of AstronomyNordic Institute for Theoretical Physics (Nordita)
Astronomy, Astrophysics and Cosmology

Search outside of DiVA

GoogleGoogle Scholar
Total: 148 downloads
The number of downloads is the sum of all downloads of full texts. It may include eg previous versions that are now no longer available

Total: 80 hits
ReferencesLink to record
Permanent link

Direct link