4 Conferences false [["minutes", "Minutes"], ["1", "More information about the venue"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]] ICN-UNAM 1482bc95ee34f0461176da21871284c8 3 icrc2007@icrc2007.unam.mx The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico. True Merida, Mexico

2007-07-03T08:00:00 2007-07-11T19:00:00 2005-09-26T05:04:53 2024-04-12T17:46:55 Mexico/General IGeof-UNAM 40af9343b8bb9d18708b4f0252d5f53c 448 false [["minutes", "Minutes"], ["1", "More information about the venue"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]] SH.3.2 1 Poster A.P.S. University, Rewa (M.P.)-486 003, INDIA ab042a7f772a87b727c4f7a6882f3df8 A.P.S. University, Rewa (M.P.)-486 003, INDIA ab042a7f772a87b727c4f7a6882f3df8 A.P.S. University, Rewa (M.P.)-486 003, INDIA 4cd86e9638ed7b6c7b23aa18b6ad80a2 A.P.S. University, Rewa (M.P.)-486 003, INDIA c8ef0630f4c9153486469ba7c74ae7d4 A.P.S. University, Rewa (M.P.)-486 003, INDIA 899e764bfbe756deff19f50409a456b0 Merida, Mexico

Regency (Hyatt) The modulation in cosmic ray intensity is observed due to long-term and short- term variation in solar activity. The concept of multi-parametric modulation of CRI may play an important role in the study of long-term modulation of CRI. Keeping in view the said idea/concept, we have tried to investigate the combined effect of a set of two SA parameters in the long-term modulation of CRI. For this study, we have used a new statistical technique called “Running multiple correlation method”, based on the “Running cross correlation method”. The running multiple correlation functions among different sets of two SA parameters (e.g. sunspot numbers and solar flux, sunspot numbers and coronal index, sunspot numbers and grouped solar flares etc.) and CRI have been correlated separately. The strength of multiple correlation (among two SA parameters and CRI) and cross correlation (between individual SA parameter and CRI) has been found to be almost similar throughout the period of investigation. Furthermore, It is observed that the multiple correlations among various SA parameters and CRI is stronger during ascending and descending phases and it becomes weaker during maxima and minima of the solar cycles, which is in accordance with the linear relationship between SA parameters and CRI.. The strange behaviour of cycle 23 (odd cycle) in view of odd-even hypothesis of solar cycles, lead us to speculate the solar cycle 24 (even cycle) might be of exceptional nature. 1 http://www.icrc2007.unam.mx/ link http://www.icrc2007.unam.mx/ doc http://indico.nucleares.unam.mx/images/word.png word file ppt http://indico.nucleares.unam.mx/images/powerpoint.png powerpoint file pdf http://indico.nucleares.unam.mx/images/pdf_small.png pdf file odt http://indico.nucleares.unam.mx/images/writer.png writer file odp http://indico.nucleares.unam.mx/images/impress.png presentation file ods http://indico.nucleares.unam.mx/images/calc.png spreadsheet file other http://indico.nucleares.unam.mx/images/file_small.png unknown type file link http://indico.nucleares.unam.mx/images/link.png link