Evidence for distinctive changes in the solar wind helium abundance in solar cycle 24

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dc.contributor.author Yogesh
dc.contributor.author Chakrabarty, D.
dc.contributor.author Srivastava, N.
dc.coverage.spatial United Kingdom
dc.date.accessioned 2012-09-26T07:22:34Z
dc.date.available 2012-09-26T07:22:34Z
dc.date.issued 2021-05
dc.identifier.citation Yogesh; Chakrabarty, D.; Srivastava, N., "Evidence for distinctive changes in the solar wind helium abundance in solar cycle 24", Monthly Notices of the Royal Astronomical Society: Letters, DOI: 10.1093/mnrasl/slab016, vol. 503, no. 1, pp. L17�L22, May 2021 en_US
dc.identifier.issn 1745-3933
dc.identifier.uri https://doi.org/10.1093/mnrasl/slab016
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/6713
dc.description.statementofresponsibility by D. Chakrabarty Yogesh and N. Srivastava
dc.format.extent vol. 503, no. 1, pp. L17�L22
dc.language.iso en_US en_US
dc.publisher Oxford University Press en_US
dc.title Evidence for distinctive changes in the solar wind helium abundance in solar cycle 24 en_US
dc.type Article en_US
dc.relation.journal Monthly Notices of the Royal Astronomical Society: Letters


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