p-modes and temperature waves in photosphere
DESCRIPTION
P-modes and temperature waves in photosphere. Yuzef D. Zhugzhda Puskov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation of Russian Academy of Sciences. Darkening and visibility functions of p-modes Local approximation Inverse problem - PowerPoint PPT PresentationTRANSCRIPT
P-modes and P-modes and temperature waves temperature waves
in photospherein photosphereYuzef D. ZhugzhdaYuzef D. Zhugzhda
Puskov Institute of Terrestrial Puskov Institute of Terrestrial Magnetism, Ionosphere and Magnetism, Ionosphere and Radiowave Propagation of Radiowave Propagation of
Russian Academy of SciencesRussian Academy of Sciences
•Darkening and visibility functions of p-modes
•Local approximation
•Inverse problem
•True visibility and darkening function
•Explorations of Stodilka and Hidalgo et al
•Temperature waves in stratified atmosphere
•Brightness fluctuations of the Sun and stars and temperature waves
Expansion of intensity
P-modes produce small disturbances of the solar photosphere that makes possible to use expansion of intensity only up to the first order.
Opacity disturbances due to temperature and density
fluctuations
Adiabatic approximation
polar angle
darkening function
Local approximation makes possible to take out of the integral temperature disturbance
After integration over the whole disk of the star we arrive to relative visibility function normalized on relative temperature disturbances
The advantage of the local approximation is that relative visibility function depends only on parameters
of undisturbed atmosphere
Derivative of opacity with respect to temperature
Derivative of opacity with respect to density
Solid line – absolute visibility, long-dashed line –Plank function contribution, medium-dashed and short-dashed lines – contributions of opacity fluctuations due to temperature and density fluctuation
Inverse problem
Multi-channel photometer DIFOS
Circles –DIFOS, squares –SPM(SOHO)
Darkening functions
Temperature waves
Quasi-adiabatic approximation
Quasi-isothermal approximation
|||| aT kk
|||| aT kk
Coupling of p-modes and temperature waves
Optically thick
atmosphere
Optically thin
atmosphere
Isothermal atmosphere H-pressure
scale
It was found out analytical exact solution of the problem in terms of Generalized
Hypergeometrical functions
Wave coupling
P-
mod
es
Temperature waves