Ideal ballooning modes are investigated for the case of plane magnetized slab geometry. Toroidal effects are simulated by a gravitational acceleration periodically varying along magnetic field lines. High shear is shown to be very effective in stabilizing these modes even when field line curvature is most unfavorable to their stability
"The stability properties of pressure driven ballooning and Mercier modes in general stellarator con...
In heliotron/torsantron systems that have a large Shafranov shift, the local magnetic shear is found...
A unified theory of the linear stability of the Roberts and Taylor type of resistive interchange and...
The stability properties of ideal ballooning modes on toroidal flux surfaces near a quasistatic magn...
The resistive ballooning mode equations are cast in a new form appropriate for evaluation near the p...
There is a well established theory of Ballooning modes in a toroidal plasma. The cornerstone of this...
A new code demonstrates the stabilization of MHD ballooning modes by sheared toroidal rotation. A sh...
The stability of ideal ballooning modes in the presence of a rigid toroidal rotation is revisited. T...
Conditions under which the compressibility can be neglected for the magnetospheric ballooning instab...
Modern tokamaks can produce transport barriers ͑TBs͒-localized regions with an increased energy conf...
"The characteristics of the high-n ballooning modes and the corresponding beta ( = kinetic pressure/...
The kinetic effects of trapped electron dynamics and finite gyroradii and magnetic drift motion of i...
By perturbing the pressure and rotational-transform profiles at a selected surface in a given equili...
Pressure-driven, ideal ballooning stability calculations are often used to predict the achievable pl...
The recent revival of interest in the application of the ''ballooning formaiism'' to low-frequency p...
"The stability properties of pressure driven ballooning and Mercier modes in general stellarator con...
In heliotron/torsantron systems that have a large Shafranov shift, the local magnetic shear is found...
A unified theory of the linear stability of the Roberts and Taylor type of resistive interchange and...
The stability properties of ideal ballooning modes on toroidal flux surfaces near a quasistatic magn...
The resistive ballooning mode equations are cast in a new form appropriate for evaluation near the p...
There is a well established theory of Ballooning modes in a toroidal plasma. The cornerstone of this...
A new code demonstrates the stabilization of MHD ballooning modes by sheared toroidal rotation. A sh...
The stability of ideal ballooning modes in the presence of a rigid toroidal rotation is revisited. T...
Conditions under which the compressibility can be neglected for the magnetospheric ballooning instab...
Modern tokamaks can produce transport barriers ͑TBs͒-localized regions with an increased energy conf...
"The characteristics of the high-n ballooning modes and the corresponding beta ( = kinetic pressure/...
The kinetic effects of trapped electron dynamics and finite gyroradii and magnetic drift motion of i...
By perturbing the pressure and rotational-transform profiles at a selected surface in a given equili...
Pressure-driven, ideal ballooning stability calculations are often used to predict the achievable pl...
The recent revival of interest in the application of the ''ballooning formaiism'' to low-frequency p...
"The stability properties of pressure driven ballooning and Mercier modes in general stellarator con...
In heliotron/torsantron systems that have a large Shafranov shift, the local magnetic shear is found...
A unified theory of the linear stability of the Roberts and Taylor type of resistive interchange and...
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