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- A. Pouquet2 profiles68 · h 62
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- NSF NCAR High Altitude ObservatoryUS515 papers
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- Instituto de Astrofísica de CanariasES105 papers
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23 papers · 1 filter
A Synthetic Stellar Polarization Atlas from 400 to 1000 nm
H. Socas-Navarro, A. Asensio Ramos, R. Manso Sainz
% context heading (optional) {With the development of new polarimeters for large telescopes, the spectro-polarimetric study of astrophysical bodies is becoming feasible and, indeed…
Magnetic field vector retrieval with the Helioseismic and Magnetic Imager
J. M. Borrero, S. Tomczyk, A. Norton +5
We investigate the accuracy to which we can retrieve the solar photospheric magnetic field vector using the Helioseismic and Magnetic Imager (HMI) that will fly onboard of the Sola…
The Future of Computational Asteroseismology
Travis S. Metcalfe
The history of stellar seismology suggests that observation and theory often take turns advancing our understanding. The recent tripling of the sample of pulsating white dwarfs gen…
Marginally unstable Holmboe modes
Alexandros Alexakis
Marginally unstable Holmboe modes for smooth density and velocity profiles are studied. For a large family of flows and stratification that exhibit Holmboe instability, we show tha…
Origin of solar torsional oscillations
Matthias Rempel
Helioseismology has revealed many details of solar differential rotation and also its time variation, known as torsional oscillations. So far there is no generally accepted theoret…
Transport of toroidal magnetic field by the meridional flow at the base of the solar convection zone
Matthias Rempel
In this paper we discuss the transport of toroidal magnetic field by a weak meridional flow at the base of the convection zone. We utilize the differential rotation and meridional…