{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1360574092883299072.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2014ja020419"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2014JA020419"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2014JA020419"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2014JA020419"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2014JA020419"}}],"dc:title":[{"@value":"Magnetic field power spectra and magnetic radial diffusion coefficients using CRRES magnetometer data"}],"description":[{"type":"abstract","notation":[{"@value":"AbstractWe used the fluxgate magnetometer data from Combined Release and Radiation Effects Satellite (CRRES) to estimate the power spectral density (PSD) of the compressional component of the geomagnetic field in the ∼1 mHz to ∼8 mHz range. We conclude that magnetic wave power is generally higher in the noon sector for quiet times with no significant difference between the dawn, dusk, and the midnight sectors. However, during high Kp activity, the noon sector is not necessarily dominant anymore. The magnetic PSDs have a very distinct dependence on Kp. In addition, the PSDs appear to have a weak dependence on McIlwain parameter L with power slightly increasing as L increases. The magnetic wave PSDs are used along with the Fei et al. (2006) formulation to compute as a function of L and Kp. The L dependence of is systematically studied and is shown to depend on Kp. More significantly, we conclude that is the dominant term driving radial diffusion, typically exceeding by 1–2 orders of magnitude."}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380574092883299075","@type":"Researcher","foaf:name":[{"@value":"Ashar F. Ali"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092883299077","@type":"Researcher","foaf:name":[{"@value":"Scot R. Elkington"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder Colorado USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092883299072","@type":"Researcher","foaf:name":[{"@value":"Weichao Tu"}],"jpcoar:affiliationName":[{"@value":"Los Alamos National Laboratory Los Alamos New Mexico USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092883299074","@type":"Researcher","foaf:name":[{"@value":"Louis G. Ozeke"}],"jpcoar:affiliationName":[{"@value":"Department of Physics University of Alberta Edmonton Alberta Canada"}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092883299076","@type":"Researcher","foaf:name":[{"@value":"Anthony A. Chan"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy Rice University Houston Texas USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380574092883299073","@type":"Researcher","foaf:name":[{"@value":"Reiner H. W. Friedel"}],"jpcoar:affiliationName":[{"@value":"Los Alamos National Laboratory Los Alamos New Mexico USA"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"21699380"},{"@type":"EISSN","@value":"21699402"}],"prism:publicationName":[{"@value":"Journal of Geophysical Research: Space Physics"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2015-02","prism:volume":"120","prism:number":"2","prism:startingPage":"973","prism:endingPage":"995"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2014JA020419"},{"@id":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2014JA020419"},{"@id":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2014JA020419"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2014JA020419"}],"createdAt":"2015-01-08","modifiedAt":"2023-09-17","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050282813184511232","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"The ARASE (ERG) magnetic field investigation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588380144824576","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Simulating the Ring Current Proton Dynamics in Response to Radial Diffusion by Ultra‐Low‐Frequency (ULF) Waves"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861707357326592","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Distribution of ULF Wave Power in Magnetic Latitude and Local Time Using THEMIS and Arase Measurements"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1002/2014ja020419"},{"@type":"CROSSREF","@value":"10.1186/s40623-018-0800-1_references_DOI_6sq6dzuRhoVIVBneWuSwkXPdTDo"},{"@type":"CROSSREF","@value":"10.1029/2023gl107326_references_DOI_Vx1GxjEnZnhLV1QkJx0tYahD3e3"},{"@type":"CROSSREF","@value":"10.1029/2022ja030469_references_DOI_6sq6dzuRhoVIVBneWuSwkXPdTDo"}]}