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Cosmic-ray periodicity at 170 days

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dc.contributor.author Joshi, A.
dc.date.accessioned 2009-08-19T11:07:02Z
dc.date.available 2009-08-19T11:07:02Z
dc.date.issued 1998
dc.identifier.uri http://hdl.handle.net/123456789/288
dc.description.abstract Power-spectral analysis of cosmic-ray indices (CRI) data for the years 1989–1991 shows a 170-day periodicity of cosmic rays. The periodicity is related to a strong magnetic field. Power- spectral analysis of the long-term periodicity (∼11 years) of the CRI data for the years 1953– 1997 shows that the period 1989 – 1991 is a unique one in the sense of the discussed pronounced periodicity. The 170-day periodicity of cosmic rays was interpreted in the base of six solar rotations (1 SR = 28.3-day periodicity of 10.7 cm solar radio flux) and may be connected to the instability of the solar core. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries sp185-397
dc.subject CRI en_US
dc.title Cosmic-ray periodicity at 170 days en_US
dc.type Article en_US


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