Ideal and resistive ballooning modes are investigated for different ratios of a two-layer stratified density region representing a model for the photospheric/coronal boundary. Construction of the ballooning equations using a WKB approach is justified by comparison between the values of the growth rate obtained using Hain-Luest and ballooning equations together with a WKB integral relation. Different values of the density ratio, radius, and resistivity are considered. Sausage-type and kink-type instabilities are found. One of these, depending on the value of r, remained unstable for large density ratios. The other instability tended to marginal stability as the density ratio was increased, and allowed parallel and perpendicular flows across ...
Pressure-driven, ideal ballooning stability calculations are often used to predict the achievable pl...
Conditions under which the compressibility can be neglected for the magnetospheric ballooning instab...
We investigate the influence of the finite extent of the computational domain and of specific bounda...
The stability of coronal arcades to localized resistive interchange modes in the ballooning ordering...
A method for analyzing the stability of cylindrical loops and arcades to ballooning modes is present...
The resistive stability of coronal loops to perturbations with short wavelength across the magnetic ...
The study of resistive ballooning instabilities in line-tied coronal magnetic fields is extended by ...
The stability equations for localized (or ballooning) modes in the solar atmosphere are formulated. ...
The resistive ballooning mode equations are cast in a new form appropriate for evaluation near the p...
The equations describing the linear evolution of resistive ballooning modes are obtained by using a ...
The stability characteristics of resistive ballooning modes are examined near a tokamak edge region ...
We study the influence of gravitational stratification of the solar atmosphere on the stability of c...
We study the influence of gravitational stratification of the solar atmosphere on the stability of c...
Using the localised, ballooning ordering, the effect of a density stratification on the ideal MHD st...
Magnetohydrodynamic stability theory provides a powerful tool for understanding and testing hypothes...
Pressure-driven, ideal ballooning stability calculations are often used to predict the achievable pl...
Conditions under which the compressibility can be neglected for the magnetospheric ballooning instab...
We investigate the influence of the finite extent of the computational domain and of specific bounda...
The stability of coronal arcades to localized resistive interchange modes in the ballooning ordering...
A method for analyzing the stability of cylindrical loops and arcades to ballooning modes is present...
The resistive stability of coronal loops to perturbations with short wavelength across the magnetic ...
The study of resistive ballooning instabilities in line-tied coronal magnetic fields is extended by ...
The stability equations for localized (or ballooning) modes in the solar atmosphere are formulated. ...
The resistive ballooning mode equations are cast in a new form appropriate for evaluation near the p...
The equations describing the linear evolution of resistive ballooning modes are obtained by using a ...
The stability characteristics of resistive ballooning modes are examined near a tokamak edge region ...
We study the influence of gravitational stratification of the solar atmosphere on the stability of c...
We study the influence of gravitational stratification of the solar atmosphere on the stability of c...
Using the localised, ballooning ordering, the effect of a density stratification on the ideal MHD st...
Magnetohydrodynamic stability theory provides a powerful tool for understanding and testing hypothes...
Pressure-driven, ideal ballooning stability calculations are often used to predict the achievable pl...
Conditions under which the compressibility can be neglected for the magnetospheric ballooning instab...
We investigate the influence of the finite extent of the computational domain and of specific bounda...