Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Seismic diagnostics on stellar convection treatment from oscillation
  amplitudes of p-modes   The excitation rate P of solar p-modes is computed with a model of stochatic
excitation which involves constraints on the averaged properties of the solar
turbulence. These constraints are obtained from a 3D simulation. Resulting
values for P are found ~9 times larger than when the calculation assumes
properties of turbulent convection which are derived from an 1D solar model
based on Gough (1977)'s formulation of the mixing-length theory (GMLT). This
difference is mainly due to the assumed values for the mean anisotropy of the
velocity field in each case.Calculations based on 3D constraints bring the P
maximum closer to the observational one.We also compute P for several models of
intermediate mass stars (1Mo < M < 2Mo). Differences in the values of P_max
between models computed with the classical mixing-length theory and GMLT models
are found large enough for main sequence stars to suggest that measurements of
P in this mass range will be able to discriminate between different models of
turbulent convection.

33
The categories of this paper are: plasm-ph
27
The categories of this paper are: comp-gas
13
The categories of this paper are: quant-ph
24
The categories of this paper are: dg-ga
28
The categories of this paper are: alg-geom
21
The categories of this paper are: adap-org
22
The categories of this paper are: chao-dyn
11
The categories of this paper are: hep-lat
18
The categories of this paper are: econ
9
The categories of this paper are: nlin
29
The categories of this paper are: funct-an
15
The categories of this paper are: nucl-ex
34
The categories of this paper are: chem-ph
7
The categories of this paper are: hep-th
4
The categories of this paper are: cond-mat
0
The categories of this paper are: hep-ph