{"@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/1363388844504006656.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2015rs005903"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015RS005903"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015RS005903"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2015RS005903"}},{"identifier":{"@type":"URI","@value":"http://api.wiley.com/onlinelibrary/chorus/v1/articles/10.1002%2F2015RS005903"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2015RS005903"}}],"dc:title":[{"@value":"A theory of scintillation for two‐component power law irregularity spectra: Overview and numerical results"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>We extend the power law phase screen theory for ionospheric scintillation to account for the case where the refractive index irregularities follow a two‐component inverse power law spectrum. The two‐component model includes, as special cases, an unmodified power law and a modified power law with spectral break that may assume the role of an outer scale, intermediate break scale, or inner scale. As such, it provides a framework for investigating the effects of a spectral break on the scintillation statistics. Using this spectral model, we solve the fourth moment equation governing intensity variations following propagation through two‐dimensional field‐aligned irregularities in the ionosphere. A specific normalization is invoked that exploits self‐similar properties of the structure to achieve a universal scaling, such that different combinations of perturbation strength, propagation distance, and frequency produce the same results. The numerical algorithm is validated using new theoretical predictions for the behavior of the scintillation index and intensity correlation length under strong scatter conditions. A series of numerical experiments are conducted to investigate the morphologies of the intensity spectrum, scintillation index, and intensity correlation length as functions of the spectral indices and strength of scatter; retrieve phase screen parameters from intensity scintillation observations; explore the relative contributions to the scintillation due to large‐ and small‐scale ionospheric structures; and quantify the conditions under which a general spectral break will influence the scintillation statistics.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1383388844504006657","@type":"Researcher","foaf:name":[{"@value":"Charles S. Carrano"}],"jpcoar:affiliationName":[{"@value":"Institute for Scientific Research Boston College  Chestnut Hill Massachusetts USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844504006656","@type":"Researcher","foaf:name":[{"@value":"Charles L. Rino"}],"jpcoar:affiliationName":[{"@value":"Institute for Scientific Research Boston College  Chestnut Hill Massachusetts USA"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00486604"},{"@type":"EISSN","@value":"1944799X"}],"prism:publicationName":[{"@value":"Radio Science"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2016-06","prism:volume":"51","prism:number":"6","prism:startingPage":"789","prism:endingPage":"813"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015RS005903"},{"@id":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015RS005903"},{"@id":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2015RS005903"},{"@id":"http://api.wiley.com/onlinelibrary/chorus/v1/articles/10.1002%2F2015RS005903"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2015RS005903"}],"createdAt":"2016-06-30","modifiedAt":"2023-09-17","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360017282189349760","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"GPS Scintillations and TEC Variations in Association With a Polar Cap Arc"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021391865415808","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A three-dimensional stochastic structure model derived from high-resolution isolated equatorial plasma bubble simulations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285708269572096","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A Configuration Space Model for Intermediate‐Scale Ionospheric Structure"}]},{"@id":"https://cir.nii.ac.jp/crid/2051433317007350400","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecasting"}]},{"@id":"https://cir.nii.ac.jp/crid/2051996266973437696","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dynamic spectral characteristics of high-resolution simulated equatorial plasma bubbles"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1002/2015rs005903"},{"@type":"CROSSREF","@value":"10.1029/2020ja028968_references_DOI_YQyyrcyumfSgbcX03S7KMAhWrJU"},{"@type":"CROSSREF","@value":"10.1186/s40623-023-01823-6_references_DOI_YQyyrcyumfSgbcX03S7KMAhWrJU"},{"@type":"CROSSREF","@value":"10.1029/2018rs006678_references_DOI_YQyyrcyumfSgbcX03S7KMAhWrJU"},{"@type":"CROSSREF","@value":"10.1186/s40645-017-0153-6_references_DOI_YQyyrcyumfSgbcX03S7KMAhWrJU"},{"@type":"CROSSREF","@value":"10.1186/s40645-018-0243-0_references_DOI_YQyyrcyumfSgbcX03S7KMAhWrJU"}]}