Watson Transformation for the Coherent Electromagnetic Field Scattered by a Statistically Rough Sphere. IV. Numerical Analysis
Analytical properties of the earlier derived expressions for the effective impedance of the coherent scattered field are investigated. A sufficiently general type of the spectrum surface roughness has been calculated numerically and compared versus known heuristic models for evaluation of the field...
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| Дата: | 2013 |
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| Автори: | , |
| Формат: | Стаття |
| Мова: | rus |
| Опубліковано: |
Видавничий дім «Академперіодика»
2013
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| Онлайн доступ: | http://rpra-journal.org.ua/index.php/ra/article/view/698 |
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| Назва журналу: | Radio physics and radio astronomy |
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oai:ri.kharkov.ua:article-6982013-02-09T23:15:03Z Watson Transformation for the Coherent Electromagnetic Field Scattered by a Statistically Rough Sphere. IV. Numerical Analysis Преобразование Ватсона для когерентного электромагнитного поля, рассеянного статистически неровной сферой. IV. Численный анализ Bryukhovetski, A. S. Pazynin, L. A. Analytical properties of the earlier derived expressions for the effective impedance of the coherent scattered field are investigated. A sufficiently general type of the spectrum surface roughness has been calculated numerically and compared versus known heuristic models for evaluation of the field attenuation in the shadow zone of a large statistically rough sphere. Исследуются аналитические свойства выражений для эффективного импеданса когерентного рассеянного поля, полученные ранее. Для спектра неровностей достаточно общего вида выполнен численный счет и проведено сравнение с известными эвристическими моделями оценок ослабления поля в зоне тени большой статистически неровной сферы. Видавничий дім «Академперіодика» 2013-02-09 Article Article application/pdf http://rpra-journal.org.ua/index.php/ra/article/view/698 РАДИОФИЗИКА И РАДИОАСТРОНОМИЯ; Vol 10, No 2 (2005); 135 RADIO PHYSICS AND RADIO ASTRONOMY; Vol 10, No 2 (2005); 135 РАДІОФІЗИКА І РАДІОАСТРОНОМІЯ; Vol 10, No 2 (2005); 135 2415-7007 1027-9636 rus http://rpra-journal.org.ua/index.php/ra/article/view/698/249 |
| institution |
Radio physics and radio astronomy |
| collection |
OJS |
| language |
rus |
| format |
Article |
| author |
Bryukhovetski, A. S. Pazynin, L. A. |
| spellingShingle |
Bryukhovetski, A. S. Pazynin, L. A. Watson Transformation for the Coherent Electromagnetic Field Scattered by a Statistically Rough Sphere. IV. Numerical Analysis |
| author_facet |
Bryukhovetski, A. S. Pazynin, L. A. |
| author_sort |
Bryukhovetski, A. S. |
| title |
Watson Transformation for the Coherent Electromagnetic Field Scattered by a Statistically Rough Sphere. IV. Numerical Analysis |
| title_short |
Watson Transformation for the Coherent Electromagnetic Field Scattered by a Statistically Rough Sphere. IV. Numerical Analysis |
| title_full |
Watson Transformation for the Coherent Electromagnetic Field Scattered by a Statistically Rough Sphere. IV. Numerical Analysis |
| title_fullStr |
Watson Transformation for the Coherent Electromagnetic Field Scattered by a Statistically Rough Sphere. IV. Numerical Analysis |
| title_full_unstemmed |
Watson Transformation for the Coherent Electromagnetic Field Scattered by a Statistically Rough Sphere. IV. Numerical Analysis |
| title_sort |
watson transformation for the coherent electromagnetic field scattered by a statistically rough sphere. iv. numerical analysis |
| title_alt |
Преобразование Ватсона для когерентного электромагнитного поля, рассеянного статистически неровной сферой. IV. Численный анализ |
| description |
Analytical properties of the earlier derived expressions for the effective impedance of the coherent scattered field are investigated. A sufficiently general type of the spectrum surface roughness has been calculated numerically and compared versus known heuristic models for evaluation of the field attenuation in the shadow zone of a large statistically rough sphere. |
| publisher |
Видавничий дім «Академперіодика» |
| publishDate |
2013 |
| url |
http://rpra-journal.org.ua/index.php/ra/article/view/698 |
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2024-05-26T06:32:18Z |
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2024-05-26T06:32:18Z |
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