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 |