Show simple item record

dc.contributor.authorWurster, J
dc.date.accessioned2017-01-24T14:34:44Z
dc.date.issued2016-09-09
dc.description.abstractIn this paper, we introduce Nicil: Non-Ideal magnetohydrodynamics Coefficients and Ionisation Library. Nicil is a stand-alone Fortran90 module that calculates the ionisation values and the coefficients of the non-ideal magnetohydrodynamics terms of Ohmic resistivity, the Hall effect, and ambipolar diffusion. The module is fully parameterised such that the user can decide which processes to include and decide upon the values of the free parameters, making this a versatile and customisable code. The module includes both cosmic ray and thermal ionisation; the former includes two ion species and three species of dust grains (positively charged, negatively charged, and neutral), and the latter includes five elements which can be doubly ionised. We demonstrate tests of the module, and then describe how to implement it into an existing numerical code.en_GB
dc.description.sponsorshipJW acknowledges support from the Australian Research Council (ARC) Discovery Projects Grant DP130102078 and from the European Research Council under the European Community’s Seventh Framework Programme (FP7/2007–2013 grant agreement no. 339248).en_GB
dc.identifier.citationVol. 33, e041en_GB
dc.identifier.doi10.1017/pasa.2016.34
dc.identifier.urihttp://hdl.handle.net/10871/25383
dc.language.isoenen_GB
dc.publisherCambridge University Press (CUP)en_GB
dc.relation.urlhttp://hdl.handle.net/10871/25398en_GB
dc.rights.embargoreasonPublisher policyen_GB
dc.rights© Astronomical Society of Australia 2016; published by Cambridge University Press.en_GB
dc.subjectmagnetohydrodynamicsen_GB
dc.subjectMHDen_GB
dc.subjectmethods: numericalen_GB
dc.titleNICIL: a stand alone library to self-consistently calculate non-ideal magnetohydrodynamic coefficients in molecular cloud cores (article)en_GB
dc.typeArticleen_GB
dc.identifier.issn1323-3580
dc.descriptionThis is the author accepted manuscript. The final version is available from the publisher via the DOI in this record.en_GB
dc.descriptionThe dataset associated with this article is available in ORE at: http://hdl.handle.net/10871/25398en_GB
dc.identifier.journalPublications of the Astronomical Society of Australiaen_GB


Files in this item

This item appears in the following Collection(s)

Show simple item record