THE INFLUENCE OF A MODIFIED MIXING-LENGTH THEORY AND OF AN ADOPTED DESCRIPTION OF THE ATMOSPHERE ON THE SOLAR 5-MINUTE OSCILLATIONS

被引：0

作者：

PAMYATNYKH, AA ^{[1
]}

机构：

[1] EUROPEAN SO OBSERV,D-8046 GARCHING,FED REP GER

来源：

IAU SYMPOSIA | 1988年 / 123期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

下载

页码：99 / 103

页数：5

共 50 条

[41] Calibration of the mixing-length theory for structures of helium-dominated atmosphere white dwarfs
Cukanovaite, E.
Tremblay, P-E
Freytag, B.
Ludwig, H-G
Fontaine, G.
Brassard, P.
Toloza, O.
Koester, D.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 490 (01) : 1010 - 1025
[42] A STUDY OF CONVECTIVE MODEL STELLAR ATMOSPHERES USING A MODIFIED MIXING-LENGTH THEORY
LESTER, JB
LANE, MC
KURUCZ, RL
ASTROPHYSICAL JOURNAL, 1982, 260 (01): : 272 - 285
[43] New theory of stellar convection without the mixing-length parameter: new stellar atmosphere model
Pasetto, Stefano
Chiosi, Cesare
Cropper, Mark
Grebel, Eva K.
NUCLEAR PHYSICS IN ASTROPHYSICS CONFERENCE (NPA VII), 2018, 940
[44] THEORETICAL EIGENFREQUENCIES OF SOLAR OSCILLATIONS OF LOW HARMONIC DEGREE-L IN 5-MINUTE RANGE
SHIBAHASHI, H
OSAKI, Y
SOLAR PHYSICS, 1983, 82 (1-2) : 231 - 232
[45] INFLUENCE OF THE EQUATIONS OF STATE AND OF THE Z-VALUE ON THE SOLAR 5-MINUTE OSCILLATION
SHIBAHASHI, H
NOELS, A
GABRIEL, M
ASTRONOMY & ASTROPHYSICS, 1983, 123 (02) : 283 - 288
[46] THEORETICAL EIGENFREQUENCIES OF SOLAR OSCILLATIONS OF LOW HARMONIC DEGREE-L IN 5-MINUTE RANGE
SHIBAHASHI, H
OSAKI, Y
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1981, 33 (04) : 713 - 719
[47] A BAYESIAN-APPROACH TO RIDGE FITTING IN THE OMEGA-KAPPA-DIAGRAM OF THE SOLAR 5-MINUTE OSCILLATIONS
MORROW, CA
BROWN, TM
IAU SYMPOSIA, 1988, (123): : 485 - 489
[48] What mechanisms allow 5-minute oscillations in active regions of the solar surface to penetrate from the photosphere into the chromosphere?
Kostyk, R. I.
KINEMATICS AND PHYSICS OF CELESTIAL BODIES, 2015, 31 (04) : 188 - 192
[49] What mechanisms allow 5-minute oscillations in active regions of the solar surface to penetrate from the photosphere into the chromosphere?
R. I. Kostyk
Kinematics and Physics of Celestial Bodies, 2015, 31 : 188 - 192
[50] MAGNETIC QUENCHING OF TURBULENT DIFFUSIVITY: RECONCILING MIXING-LENGTH THEORY ESTIMATES WITH KINEMATIC DYNAMO MODELS OF THE SOLAR CYCLE
Munoz-Jaramillo, Andres
Nandy, Dibyendu
Martens, Petrus C. H.
ASTROPHYSICAL JOURNAL LETTERS, 2011, 727 (01)

← 1 2 3 4 5 →