<?xml version="1.0" encoding="UTF-8"?>
<Project xmlns="https://metadata.pithia.eu/schemas/2.2" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:gmd="http://www.isotc211.org/2005/gmd" xmlns:gco="http://www.isotc211.org/2005/gco" xsi:schemaLocation="https://metadata.pithia.eu/schemas/2.2 https://metadata.pithia.eu/schemas/2.2/pithia.xsd">
<identifier>
<PITHIA_Identifier>
<localID>Project_CNRS_IPIM</localID>
<namespace>cnrs</namespace>
<version>1</version>
<creationDate>2022-11-24T15:20:00Z</creationDate>
<lastModificationDate>2022-11-24T15:45:00Z</lastModificationDate>
</PITHIA_Identifier>
</identifier>
<name>IPIM : Ionosphere-Plasmasphere IRAP Model</name>
<shortName>IPIM</shortName>
<abstract>
The IRAP plasmasphere-ionosphere model (IPIM) describes the transport of the multispecies ionospheric plasma from one
hemisphere to the other along convecting and corotating magnetic field lines, taking into account source
processes at low altitude such as photoproduction, chemistry, and energization through the coupling
with a kinetic code solving the transport of suprathermal electron along the field line. Among the new
developments, a 16-moment-based approach is used for the transport equations in order to allow
development of strong temperature anisotropy at high altitude and we consider important but often
neglected effects, such as inertial acceleration (centrifugal and Coriolis). This model is accessible through transplanet web page for online runs.
</abstract>
<description>
</description>
<URL><gmd:URL>http://transplanet.irap.omp.eu/</gmd:URL></URL>
<documentation>
<Citation>
<gmd:title><gco:CharacterString>A web service dedicated to modeling of planetary ionospheres</gco:CharacterString></gmd:title>
<date xmlns="http://www.isotc211.org/2005/gmd">
<CI_Date>
<date><gco:Date>2021-09-07</gco:Date></date>
<dateType>
<CI_DateTypeCode codeList="" codeListValue="">Publication Date</CI_DateTypeCode>
</dateType>
</CI_Date>
</date>
<identifier xmlns="http://www.isotc211.org/2005/gmd">
<MD_Identifier><code><gco:CharacterString>doi:10.1016/j.pss.2019.02.008</gco:CharacterString></code></MD_Identifier>
</identifier>
<gmd:otherCitationDetails>
<gco:CharacterString>
Blelly, P. -L.; Marchaudon, A.; Indurain, M.; Witasse, O.; Amaya, J.; Chide, B.; André, N.; Génot, V.; Goutenoir, A.; Bouchemit, M., Transplanet: A web service dedicated to modeling of planetary ionospheres, Planet. Space Sci., 169, 35-44, doi:10.1016/j.pss.2019.02.008, 2019.
</gco:CharacterString>
</gmd:otherCitationDetails>
<onlineResource>
<CI_OnlineResource xmlns="http://www.isotc211.org/2005/gmd">
<linkage>
<URL>https://www.sciencedirect.com/science/article/pii/S003206331830401X</URL>
</linkage>
</CI_OnlineResource>
</onlineResource>
</Citation>
</documentation>
<keywords>
<MD_Keywords xmlns="http://www.isotc211.org/2005/gmd">
<keyword><gco:CharacterString>Ionosphere</gco:CharacterString></keyword>
<type><MD_KeywordTypeCode codeList="#pr1" codeListValue="Simulated Region"/></type>
</MD_Keywords>
</keywords>
<keywords>
<MD_Keywords xmlns="http://www.isotc211.org/2005/gmd">
<keyword><gco:CharacterString>Ionospheric Specification</gco:CharacterString></keyword>
<type><MD_KeywordTypeCode codeList="#pr1" codeListValue="Miscellaneous"/></type>
</MD_Keywords>
</keywords>
<relatedParty>
<ResponsiblePartyInfo>
<role xlink:href="https://metadata.pithia.eu/ontology/2.2/relatedPartyRole/PointOfContact"/>
<party xlink:href="https://metadata.pithia.eu/resources/2.2/individual/CNRS/Individual_CNRS_Marchaudon"/>
</ResponsiblePartyInfo>
</relatedParty>
<relatedParty>
<ResponsiblePartyInfo>
<role xlink:href="https://metadata.pithia.eu/ontology/2.2/relatedPartyRole/DataProvider"/>
<party xlink:href="https://metadata.pithia.eu/resources/2.2/organisation/pithia/Organisation_CNRS"/>
</ResponsiblePartyInfo>
</relatedParty>
<status xlink:href="https://metadata.pithia.eu/ontology/2.2/status/OnGoing"/>
</Project>
