{"@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/1360011144545325568.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2006gl025966"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2006GL025966"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2006GL025966"}}],"dc:title":[{"@value":"Effect of interplanetary shock strengths and orientations on storm sudden commencement rise times"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>We make a statistical survey of interplanetary (IP) shocks and storm sudden commencements (SSCs) observed between 1995 and 2004. We find that 75% of SSCs are associated with shocks, consistent with previous work. We use this survey to investigate the effect of the interplanetary shock strength and orientation on the SSC rise time. We find that the higher the speed of an IP shock, the less time it takes to sweep by the magnetosphere, and thus the shorter the rise time of the corresponding SSC. The orientation of an IP shock also effects the SSC rise time. Generally speaking, a highly oblique shock causes asymmetric compression of the magnetosphere with respect to the noon‐midnight meridian, takes more time to sweep by magnetosphere, and thus results in a longer rise time of the SSC.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380011144545325569","@type":"Researcher","foaf:name":[{"@value":"C. Wang"}],"jpcoar:affiliationName":[{"@value":"State Key Laboratory of Space Weather Chinese Academy of Sciences  Beijing China"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011144545325568","@type":"Researcher","foaf:name":[{"@value":"C. X. Li"}],"jpcoar:affiliationName":[{"@value":"State Key Laboratory of Space Weather Chinese Academy of Sciences  Beijing China"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011144545325571","@type":"Researcher","foaf:name":[{"@value":"Z. H. Huang"}],"jpcoar:affiliationName":[{"@value":"State Key Laboratory of Space Weather Chinese Academy of Sciences  Beijing China"}]},{"@id":"https://cir.nii.ac.jp/crid/1380011144545325570","@type":"Researcher","foaf:name":[{"@value":"J. D. Richardson"}],"jpcoar:affiliationName":[{"@value":"Kavli Institute for Astrophysics and Space Research Massachusetts Institute of Technology  Cambridge Massachusetts USA"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00948276"},{"@type":"EISSN","@value":"19448007"}],"prism:publicationName":[{"@value":"Geophysical Research Letters"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2006-07","prism:volume":"33","prism:number":"14","prism:startingPage":"L14104"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2006GL025966"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2006GL025966"}],"createdAt":"2006-07-20","modifiedAt":"2023-10-31","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050845760771158272","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Evolution of the current system during solar wind pressure pulses based on aurora and magnetometer observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567181940136576","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The role of interplanetary shock orientation on SC/SI rise time and geoeffectiveness"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848658218763904","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Coronal mass ejection–driven shocks and the associated sudden commencements/sudden impulses"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/2006gl025966"},{"@type":"CROSSREF","@value":"10.1186/s40623-016-0517-y_references_DOI_NkC4jCmydywHz1yw0TyaTaGdVkT"},{"@type":"CROSSREF","@value":"10.1029/2011ja017216_references_DOI_NkC4jCmydywHz1yw0TyaTaGdVkT"},{"@type":"CROSSREF","@value":"10.1016/j.asr.2016.12.010_references_DOI_NkC4jCmydywHz1yw0TyaTaGdVkT"}]}