dc.creatorHysell, D. L.
dc.date.accessioned2018-10-30T13:24:02Z
dc.date.accessioned2023-05-24T14:22:32Z
dc.date.available2018-10-30T13:24:02Z
dc.date.available2023-05-24T14:22:32Z
dc.date.created2018-10-30T13:24:02Z
dc.date.issued2007-08-18
dc.identifierHysell, D. L. (2007). Inverting ionospheric radio occultation measurements using maximum entropy.==$Radio science, 42$==(4), RS4022. https://doi.org/10.1029/2007RS003635
dc.identifierhttp://hdl.handle.net/20.500.12816/3223
dc.identifierRadio science
dc.identifierhttps://doi.org/10.1029/2007RS003635
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/6428943
dc.description.abstractPractical aspects of the inversion of ionospheric radio occultation data using the Abel transform and its inverse are discussed. The linear inverse transform exhibits poor error propagation characteristics, producing significant artifacts preferentially at low altitudes where they might easily be mistaken for intermediate or sporadic layers in the ionosphere. Tikhonov regularization, which can be viewed as fixed linear filtering, reduces the artifacts at the expense of discarding fine structure in the profiles. Improved results are obtained using maximum entropy and Bayesian statistics. The maximum entropy algorithm can be viewed as a nonlinear adaptive filter which suppresses artifacts while preserving fine structure to the degree the data can support. Other advantages of and avenues for improving the basic maximum entropy algorithm are discussed.
dc.languageeng
dc.publisherAmerican Geophysical Union
dc.relationurn:issn:0048-6604
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectRadio occultation
dc.subjectInverse methods
dc.subjectIonosphere
dc.titleInverting ionospheric radio occultation measurements using maximum entropy
dc.typeinfo:eu-repo/semantics/article


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