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<ref>V. Kornilov, R. Kleiber, R. Hatzky, L. Villard, and G. Jost. [[doi:10.1063/1.1737393|Phys. Plasmas '''11''': 3196 (2004)]]</ref> | <ref>V. Kornilov, R. Kleiber, R. Hatzky, L. Villard, and G. Jost. [[doi:10.1063/1.1737393|Phys. Plasmas '''11''': 3196 (2004)]]</ref> | ||
<ref>V. Kornilov, R. Kleiber, and R. Hatzky, [[doi:10.1088/0029-5515/45/4/003|Nucl. Fusion '''45''': 238 (2005)]]</ref> | <ref>V. Kornilov, R. Kleiber, and R. Hatzky, [[doi:10.1088/0029-5515/45/4/003|Nucl. Fusion '''45''': 238 (2005)]]</ref> | ||
<ref>R. Kleiber, ''Global linear gyrokinetic simulations for stellarator and axisymmetric equilibria'', Joint Varenna-Lausanne International Workshop. [[doi:10.1063/1.2404546|AIP Conference Proceedings, 871, p. 136, 2006]]</ref>. | <ref>R. Kleiber, ''Global linear gyrokinetic simulations for stellarator and axisymmetric equilibria'', Joint Varenna-Lausanne International Workshop. [[doi:10.1063/1.2404546|AIP Conference Proceedings, 871, p. 136, 2006]]</ref> | ||
<ref>[[http://fusionsites.ciemat.es/picgklnf/]]</ref>. | |||
Afterwards, the code has been heavily optimized and improved. The perturbation to the magnetic field, a third species (in adition to electrons and ions) and the non-linear dynamics have been included. | Afterwards, the code has been heavily optimized and improved. The perturbation to the magnetic field, a third species (in adition to electrons and ions) and the non-linear dynamics have been included. | ||