Study Of High-Speed Solar Wind Streams Events & Solar Proton Density During Solar Cycles 22 & 23.

dc.contributor.authorSingh, S. G.en_US
dc.contributor.authorPatel, N. K.en_US
dc.contributor.authorSingh, P. R.en_US
dc.contributor.authorChaturvedi, S. Cen_US
dc.date.accessioned2023-07-14T07:45:52Z
dc.date.available2023-07-14T07:45:52Z
dc.date.issued2022-11
dc.description.abstractA geomagnetic storms is a global disturbance in Earth's magnetic field usually occurred due to abnormal conditions in the interplanetary magnetic field (IMF) & solar wind plasma emissions caused by various solar phenomenon. 138 solar wind streams in solar cycle 22 & 173 solar wind streams in solar cycle 23, have been found, which are associated with proton density, observed during 1986 to 2010. We have analyzed & studied them statistically. We have found that yearly occurrences of geomagnetic streams are strongly correlated with proton density in 11-years sunspot cycle, but no significant correlation between the maximum & minimum phase of solar cycle 22 & 23 have observeden_US
dc.identifier.affiliationsDepartment of physics Govt. P.G. College Panna (M.P.).en_US
dc.identifier.affiliationsDepartment of physics Govt. P.G. College Panna (M.P.)en_US
dc.identifier.affiliationsDepartment of physics Govt. P.G. College Panna (M.P.).en_US
dc.identifier.affiliationsDepartment of physics Govt. Lahiri College Chirimiri, Koriya (C.G.)en_US
dc.identifier.citationSingh S. G., Patel N. K., Singh P. R., Chaturvedi S. C. Study Of High-Speed Solar Wind Streams Events & Solar Proton Density During Solar Cycles 22 & 23.. Paripex - Indian Journal Of Research. 2022 Nov; 11(11): 106-107en_US
dc.identifier.issn2250-1991
dc.identifier.placeIndiaen_US
dc.identifier.urihttps://imsear.searo.who.int/handle/123456789/218739
dc.languageenen_US
dc.publisherIndian Society for Health and Advanced Researchen_US
dc.relation.issuenumber11en_US
dc.relation.volume11en_US
dc.source.urihttps://www.doi.org/10.36106/paripexen_US
dc.subjectSolar wind streams (V)en_US
dc.subjectCosmic ray intensity (CRI)en_US
dc.subjectSolar Proton density (D).en_US
dc.titleStudy Of High-Speed Solar Wind Streams Events & Solar Proton Density During Solar Cycles 22 & 23.en_US
dc.typeJournal Articleen_US
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