In this poster, recent theoretical predictions on the amplitude of the solar gravity modes are addressed. The contribution of penetrative convection to the g-mode excitation and the case of the solar mixed modes are particularly discussed
Solare g Moden sind potenziell wichtig für die Erforschung des Sonnenkerns, aber die Erkennung von g...
Solar p-mode oscillations are excited by stochastic, non-adiabatic gas pressure fluctuations, which ...
Context. Over the past 40 years, helioseismology has been enormously successful in the study of the ...
International audienceSolar gravity modes are considered the Rosetta Stone for probing and subsequen...
Context. Solar gravity modes (g modes) are buoyancy waves that are trapped in the solar radiative zo...
International audienceContext: Detection of solar gravity modes remains a major challenge to our und...
Present theories suggest two different classes of excitation mechanisms which may be responsible for...
The excitation of internal gravity waves by penetrative convective plumes is investigated using 2-D ...
Context. Detection of solar gravity modes remains a major challenge to our understanding of the in...
With over 5 years of GOLF data having some 90% continuity, a new attempt has been made to search fo...
This dissertation explores some of the nonlinear properties of gravity-mode oscillations in the sola...
We present numerical simulations of penetrative convection and gravity wave excitation in the Sun. G...
Context. The detection of asymptotic solar g-mode parameters was the main goal of the GOLF instrumen...
The internal gravity modes of the Sun are notoriously difficult to detect, and the claimed detection...
Intermediate-degree g-modes (those with angular order ℓ ≈ 30) were first observed in the late 1970's...
Solare g Moden sind potenziell wichtig für die Erforschung des Sonnenkerns, aber die Erkennung von g...
Solar p-mode oscillations are excited by stochastic, non-adiabatic gas pressure fluctuations, which ...
Context. Over the past 40 years, helioseismology has been enormously successful in the study of the ...
International audienceSolar gravity modes are considered the Rosetta Stone for probing and subsequen...
Context. Solar gravity modes (g modes) are buoyancy waves that are trapped in the solar radiative zo...
International audienceContext: Detection of solar gravity modes remains a major challenge to our und...
Present theories suggest two different classes of excitation mechanisms which may be responsible for...
The excitation of internal gravity waves by penetrative convective plumes is investigated using 2-D ...
Context. Detection of solar gravity modes remains a major challenge to our understanding of the in...
With over 5 years of GOLF data having some 90% continuity, a new attempt has been made to search fo...
This dissertation explores some of the nonlinear properties of gravity-mode oscillations in the sola...
We present numerical simulations of penetrative convection and gravity wave excitation in the Sun. G...
Context. The detection of asymptotic solar g-mode parameters was the main goal of the GOLF instrumen...
The internal gravity modes of the Sun are notoriously difficult to detect, and the claimed detection...
Intermediate-degree g-modes (those with angular order ℓ ≈ 30) were first observed in the late 1970's...
Solare g Moden sind potenziell wichtig für die Erforschung des Sonnenkerns, aber die Erkennung von g...
Solar p-mode oscillations are excited by stochastic, non-adiabatic gas pressure fluctuations, which ...
Context. Over the past 40 years, helioseismology has been enormously successful in the study of the ...
DOI
Add to ORKG