{"id":618,"date":"2018-08-20T16:15:31","date_gmt":"2018-08-20T23:15:31","guid":{"rendered":"https:\/\/chuckrino.com\/?p=618"},"modified":"2019-07-11T21:21:37","modified_gmt":"2019-07-12T04:21:37","slug":"power-law-parameter-estimation","status":"publish","type":"post","link":"https:\/\/chuckrino.com\/?p=618","title":{"rendered":"Power-Law Parameter Estimation"},"content":{"rendered":"\n<p>The basic structure and dynamics of the ionosphere are captured by deterministic models.&nbsp; At the next level, physics-based ionospheric simulations produce stochastic structure, which is characterized by a statistical model.&nbsp; Statistical models characterize an ensemble of realizations that support well-defined average measures, such as means, higher moments, probability density functions, and covariance. &nbsp;Such models require statistical uniformity, whereas real processes not strictly homogeneous.<\/p>\n\n\n\n<p>Analyzing real diagnostic data requires segmentation and averaging.&nbsp; The length of the segment and the sample interval determine the scale or frequency measurement range.&nbsp; Selecting a segmentation requires and assessment of the largest scale that supports statistical substructure.&nbsp; In our 2014 paper <em>Wavelet-based analysis and power law classification of C\/NOFS high-resolution electron density data<\/em>, <a href=\"https:\/\/chuckrino.com\/wp-content\/uploads\/2018\/08\/Rino_et_al-2014-Radio_Science.pdf\">REF<\/a> wavelets were introduced because of their ability to measure the variation of the scale over as many scale replications supported by the interval.&nbsp; Scale spectra measure scale versus distance, and thereby provide scale measures and scale dependent uniformity.&nbsp; A classification procedure was then developed to estimate two-component power-law parameters.<\/p>\n\n\n\n<p>In a second study the classification procedure was applied to C\/NOFS data accumulated over a four-year period <a href=\"https:\/\/chuckrino.com\/wp-content\/uploads\/2018\/08\/Rino_et_al-2016-Radio_Science.pdf\">REF<\/a>.&nbsp; It was found that the most highly disturbed passes supported two-component power-law, giving way to a single power-law at smaller disturbance levels.&nbsp; All the classified SDFs showed a correlation between the turbulent strength and the large-scale spectral index.&nbsp; It had also been noted that the correlation was observed in remote diagnostics as well.<\/p>\n\n\n\n<p>Because of the persistence of the correlation between the turbulent strength and the large-scale power-law index and some published papers discovered in development of Maximum Likelihood IPE, we began to suspect that the correlation was intrinsic to power-law parameter estimation.&nbsp; A detailed study, which has been submitted for publication, <a href=\"https:\/\/chuckrino.com\/wp-content\/uploads\/2018\/08\/Carrano_et_al-2016-Radio_Science.pdf\">REF<\/a>, show that this was indeed the case.<\/p>\n\n\n\n<p>It was shown further that wavelet-based estimators exaggerate the correlation.&nbsp; The ramifications for the C\/NOFS results change mainly the interpretation.&nbsp; The correlation is intrinsic power-law measurements, not a property of the underlying structure.&nbsp; Regarding wavelets, we believe they are useful for identifying segmentation, but should not be used in place of periodograms for IPE.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The basic structure and dynamics of the ionosphere are captured by deterministic models.&nbsp; At the next level, physics-based ionospheric simulations produce stochastic structure, which is characterized by a statistical model.&nbsp; Statistical models characterize an ensemble of realizations that support well-defined &hellip; <a href=\"https:\/\/chuckrino.com\/?p=618\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[17],"tags":[],"class_list":["post-618","post","type-post","status-publish","format-standard","hentry","category-new-results"],"_links":{"self":[{"href":"https:\/\/chuckrino.com\/index.php?rest_route=\/wp\/v2\/posts\/618","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/chuckrino.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/chuckrino.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/chuckrino.com\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/chuckrino.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=618"}],"version-history":[{"count":9,"href":"https:\/\/chuckrino.com\/index.php?rest_route=\/wp\/v2\/posts\/618\/revisions"}],"predecessor-version":[{"id":831,"href":"https:\/\/chuckrino.com\/index.php?rest_route=\/wp\/v2\/posts\/618\/revisions\/831"}],"wp:attachment":[{"href":"https:\/\/chuckrino.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=618"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/chuckrino.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=618"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/chuckrino.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=618"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}