Time Delays in Cosmic Ray Propagation
Cosmic Rays (CR) travel at speeds essentially indistinguishable from the speed of light. However whilst travelling through magnetic fields, both regular and turbulent, they are delayed behind the light since they are usually charged particles and their paths are not linear. Those delays can be so lo...
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| Format: | Article |
| Language: | English |
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University of Tehran
2011-03-01
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| Series: | Journal of Sciences, Islamic Republic of Iran |
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| Online Access: | https://jsciences.ut.ac.ir/article_22216_6b1ef9ee616fbf34a1371bde91c9835c.pdf |
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| author | P. Davoudifar |
| author_facet | P. Davoudifar |
| author_sort | P. Davoudifar |
| collection | DOAJ |
| description | Cosmic Rays (CR) travel at speeds essentially indistinguishable from the speed of light. However whilst travelling through magnetic fields, both regular and turbulent, they are delayed behind the light since they are usually charged particles and their paths are not linear. Those delays can be so long that they are an impediment to correctly identifying sources which may be variable in time. Furthermore deduction of CR sources without knowing CR time delays is not possible, so the magnitude of such delays will be discussed and compared to the characteristic time variation of possible cosmic ray sources. |
| format | Article |
| id | doaj-art-cabc94884fc247d799792e08a6c42caa |
| institution | OA Journals |
| issn | 1016-1104 2345-6914 |
| language | English |
| publishDate | 2011-03-01 |
| publisher | University of Tehran |
| record_format | Article |
| series | Journal of Sciences, Islamic Republic of Iran |
| spelling | doaj-art-cabc94884fc247d799792e08a6c42caa2025-08-20T02:25:52ZengUniversity of TehranJournal of Sciences, Islamic Republic of Iran1016-11042345-69142011-03-012217515822216Time Delays in Cosmic Ray PropagationP. Davoudifar0Research Institute for Astronomy and Astrophysics of MaraghaCosmic Rays (CR) travel at speeds essentially indistinguishable from the speed of light. However whilst travelling through magnetic fields, both regular and turbulent, they are delayed behind the light since they are usually charged particles and their paths are not linear. Those delays can be so long that they are an impediment to correctly identifying sources which may be variable in time. Furthermore deduction of CR sources without knowing CR time delays is not possible, so the magnitude of such delays will be discussed and compared to the characteristic time variation of possible cosmic ray sources.https://jsciences.ut.ac.ir/article_22216_6b1ef9ee616fbf34a1371bde91c9835c.pdfcosmic raysgalaxies: generalism: magnetic fields |
| spellingShingle | P. Davoudifar Time Delays in Cosmic Ray Propagation Journal of Sciences, Islamic Republic of Iran cosmic rays galaxies: general ism: magnetic fields |
| title | Time Delays in Cosmic Ray Propagation |
| title_full | Time Delays in Cosmic Ray Propagation |
| title_fullStr | Time Delays in Cosmic Ray Propagation |
| title_full_unstemmed | Time Delays in Cosmic Ray Propagation |
| title_short | Time Delays in Cosmic Ray Propagation |
| title_sort | time delays in cosmic ray propagation |
| topic | cosmic rays galaxies: general ism: magnetic fields |
| url | https://jsciences.ut.ac.ir/article_22216_6b1ef9ee616fbf34a1371bde91c9835c.pdf |
| work_keys_str_mv | AT pdavoudifar timedelaysincosmicraypropagation |