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@article{Leclercq2016,
	author = {Leclercq, L. and Modolo, R. and Leblanc, F. and Hess, S. and Mancini, M.},
	date-added = {2021-08-21 20:44:15 +0200},
	date-modified = {2021-08-21 20:44:15 +0200},
	doi = {https://doi.org/10.1016/j.jcp.2016.01.005},
	issn = {0021-9991},
	journal = {Journal of Computational Physics},
	keywords = {Hybrid model, Mesh refinement, Particle splitting, Planet--plasma interaction},
	pages = {295 - 313},
	title = {3D magnetospheric parallel hybrid multi-grid method applied to planet--plasma interactions},
	url = {http://www.sciencedirect.com/science/article/pii/S0021999116000061},
	volume = {309},
	year = {2016},
	abstract = {We present a new method to exploit multiple refinement levels within a 3D parallel hybrid model, developed to study planet--plasma interactions. This model is based on the hybrid formalism: ions are kinetically treated whereas electrons are considered as a inertia-less fluid. Generally, ions are represented by numerical particles whose size equals the volume of the cells. Particles that leave a coarse grid subsequently entering a refined region are split into particles whose volume corresponds to the volume of the refined cells. The number of refined particles created from a coarse particle depends on the grid refinement rate. In order to conserve velocity distribution functions and to avoid calculations of average velocities, particles are not coalesced. Moreover, to ensure the constancy of particles' shape function sizes, the hybrid method is adapted to allow refined particles to move within a coarse region. Another innovation of this approach is the method developed to compute grid moments at interfaces between two refinement levels. Indeed, the hybrid method is adapted to accurately account for the special grid structure at the interfaces, avoiding any overlapping grid considerations. Some fundamental test runs were performed to validate our approach (e.g. quiet plasma flow, Alfven wave propagation). Lastly, we also show a planetary application of the model, simulating the interaction between Jupiter's moon Ganymede and the Jovian plasma.}}

@article{Mann1947,
	author = {Mann, H. B. and Whitney, D. R.},
	date-added = {2021-08-21 20:42:26 +0200},
	date-modified = {2021-08-21 20:56:45 +0200},
	doi = {10.1214/aoms/1177730491},
	fjournal = {The Annals of Mathematical Statistics},
	journal = {Ann. Math. Statist.},
	month = {03},
	number = {1},
	pages = {50--60},
	publisher = {The Institute of Mathematical Statistics},
	title = {On a Test of Whether one of Two Random Variables is Stochastically Larger than the Other},
	url = {https://doi.org/10.1214/aoms/1177730491},
	volume = {18},
	year = {1947}}

@article{Gurnett2007,
	author = {Gurnett, D. A. and Persoon, a. M. and Kurth, William S. and Groene, J. B. and Averkamp, T. F. and Dougherty, Michele K. and Southwood, D. J.},
	date-added = {2021-08-21 20:41:53 +0200},
	date-modified = {2021-08-21 20:41:53 +0200},
	doi = {10.1126/science.1138562},
	file = {:Users/husker/B\"{u}cher/Gurnett et al. - 2007 - The variable rotation period of the inner region of Saturn's plasma disk.pdf:pdf},
	issn = {1095-9203},
	journal = {Science (New York, N.Y.)},
	keywords = {, SKM, Saturn Kilometric Radiation, Space Physics},
	mendeley-tags = {Paper,SKM,Saturn Kilometric Radiation,Space Physics},
	month = apr,
	number = {5823},
	pages = {442--5},
	pmid = {17379775},
	title = {{The variable rotation period of the inner region of Saturn's plasma disk.}},
	url = {http://www.ncbi.nlm.nih.gov/pubmed/17379775},
	volume = {316},
	year = {2007},
	abstract = {We show that the plasma and magnetic fields in the inner region of Saturn's plasma disk rotate in synchronism with the time-variable modulation period of Saturn's kilometric radio emission. This relation suggests that the radio modulation has its origins in the inner region of the plasma disk, most likely from a centrifugally driven convective instability and an associated plasma outflow that slowly slips in phase relative to Saturn's internal rotation. The slippage rate is determined by the electrodynamic coupling of the plasma disk to Saturn and by the drag force exerted by its interaction with the Enceladus neutral gas torus.}}