Frequency shift of acoustic gravity waves in a stratified, isothermal, turbulent atmosphere

被引:0
作者
Nocera, L
Murawski, K
机构
[1] CNR, IPCF, I-56124 Pisa, Italy
[2] Marie Curie Sklodowska Univ, Inst Phys, Dept Complex Phys Syst, PL-20031 Lublin, Poland
关键词
turbulence; random waves; atmospheres; solar oscillations;
D O I
10.1080/03091920410001654320
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the modification of the frequency of small amplitude acoustic gravity waves which propagate in an isothermal turbulent atmosphere that is stratified by a homogeneous gravitational field. Using a Green's function method, the dispersion relation for the frequency of the waves is formulated as an integral eigenvalue equation and it is solved by perturbation techniques. We draw the following main conclusions: (a) for an arbitrary turbulent correlation spectrum the dispersion relation has a root with a negative imaginary part in the unphysical Riemann sheet of the dispersion function, leading to wave attenuation, much in the same way as it happens for Landau damping; (b) the real part of this root differs from the frequency of an acoustic gravity wave propagating in a nonturbulent medium and, for all forms of the turbulent correlation spectrum, the absolute value of this difference increases if gravity increases; (c) for a Gaussian turbulent correlation spectrum, this difference is always positive; (d) conversely if this frequency difference is known from observations, the auto-correlation function of the temperature fluctuations can be calculated through a simple inversion formula.
引用
收藏
页码:63 / 84
页数:22
相关论文
共 63 条
[1]  
[Anonymous], HDB MATH FUNCTIONS F
[2]  
[Anonymous], ANAL FUNCTIONS DISTR
[3]  
APPOURCHAUX T, 1995, ASTRON ASTROPHYS, V294, pL13
[4]  
BANERJEE D, 1997, CORE96 SOLAR CONVECT, V225, P277
[5]   EFFECT OF A FIBRIL MAGNETIC-FIELD ON SOLAR P-MODES [J].
BOGDAN, TJ ;
ZWEIBEL, EG .
ASTROPHYSICAL JOURNAL, 1985, 298 (02) :867-875
[6]   THE NORMAL-MODES OF A RESONANT CAVITY CONTAINING DISCRETE INHOMOGENEITIES - THE INFLUENCE OF FIBRIL MAGNETIC-FIELDS ON THE SOLAR ACOUSTIC-OSCILLATIONS [J].
BOGDAN, TJ ;
CATTANEO, F .
ASTROPHYSICAL JOURNAL, 1989, 342 (01) :545-557
[7]   UMBRAL OSCILLATIONS IN SUNSPOTS - ABSORPTION OF P-MODES AND ACTIVE-REGION HEATING BY MODE CONVERSION [J].
CALLY, PS ;
BOGDAN, TJ ;
ZWEIBEL, EG .
ASTROPHYSICAL JOURNAL, 1994, 437 (01) :505-521
[8]   SOLAR P-MODES IN A VERTICAL MAGNETIC-FIELD - TRAPPED AND DAMPED PI-MODES [J].
CALLY, PS ;
BOGDAN, TJ .
ASTROPHYSICAL JOURNAL, 1993, 402 (02) :721-732
[9]   THE INFLUENCE OF A CHROMOSPHERIC MAGNETIC-FIELD ON THE SOLAR P-MODES AND F-MODES [J].
CAMPBELL, WR ;
ROBERTS, B .
ASTROPHYSICAL JOURNAL, 1989, 338 (01) :538-556
[10]   On solar p-mode frequency shifts caused by near-surface model changes [J].
ChristensenDalsgaard, J ;
Thompson, MJ .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 284 (03) :527-540