A Overview of Interplanetary Scintillation Method for Studying Solar Wind Physics
Interplanetary scintillation is the fluctuation produced in the apparent brightness of a radio source, due to refractive effects in the turbulent solar wind flowing from the sun. If this medium is illuminated coherently, analysis of the spatial and temporal properties of the radiation reaching the e...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
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The Korean Space Science Society
1988-12-01
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| Series: | Journal of Astronomy and Space Sciences |
| Online Access: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1988/v5n2/OJOOBS_1988_v5n2_123.pdf |
| _version_ | 1797368736845398016 |
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| author | S. Y. Kim N. H. Myung Y. S. Choi H. K. Kim T. H. Kim |
| author_facet | S. Y. Kim N. H. Myung Y. S. Choi H. K. Kim T. H. Kim |
| author_sort | S. Y. Kim |
| collection | DOAJ |
| description | Interplanetary scintillation is the fluctuation produced in the apparent brightness of a radio source, due to refractive effects in the turbulent solar wind flowing from the sun. If this medium is illuminated coherently, analysis of the spatial and temporal properties of the radiation reaching the earth allows the stochastic properties of the medium to be understood. Here, a brief review of method of interplanetary scintillation to study solar wind behavior will be introduced. |
| first_indexed | 2024-03-08T17:36:59Z |
| format | Article |
| id | doaj.art-84c007b8deeb46299f937064679ed347 |
| institution | Directory Open Access Journal |
| issn | 2093-5587 2093-1409 |
| language | English |
| last_indexed | 2024-03-08T17:36:59Z |
| publishDate | 1988-12-01 |
| publisher | The Korean Space Science Society |
| record_format | Article |
| series | Journal of Astronomy and Space Sciences |
| spelling | doaj.art-84c007b8deeb46299f937064679ed3472024-01-02T11:50:37ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14091988-12-0152123127A Overview of Interplanetary Scintillation Method for Studying Solar Wind PhysicsS. Y. Kim0N. H. Myung1Y. S. Choi2H. K. Kim3T. H. Kim4Korea Institute of TechnologyKorea Institute of TechnologyInstitute of Space Science and AstronomyInstitute of Space Science and AstronomyInstitute of Space Science and AstronomyInterplanetary scintillation is the fluctuation produced in the apparent brightness of a radio source, due to refractive effects in the turbulent solar wind flowing from the sun. If this medium is illuminated coherently, analysis of the spatial and temporal properties of the radiation reaching the earth allows the stochastic properties of the medium to be understood. Here, a brief review of method of interplanetary scintillation to study solar wind behavior will be introduced.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1988/v5n2/OJOOBS_1988_v5n2_123.pdf |
| spellingShingle | S. Y. Kim N. H. Myung Y. S. Choi H. K. Kim T. H. Kim A Overview of Interplanetary Scintillation Method for Studying Solar Wind Physics Journal of Astronomy and Space Sciences |
| title | A Overview of Interplanetary Scintillation Method for Studying Solar Wind Physics |
| title_full | A Overview of Interplanetary Scintillation Method for Studying Solar Wind Physics |
| title_fullStr | A Overview of Interplanetary Scintillation Method for Studying Solar Wind Physics |
| title_full_unstemmed | A Overview of Interplanetary Scintillation Method for Studying Solar Wind Physics |
| title_short | A Overview of Interplanetary Scintillation Method for Studying Solar Wind Physics |
| title_sort | overview of interplanetary scintillation method for studying solar wind physics |
| url | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1988/v5n2/OJOOBS_1988_v5n2_123.pdf |
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