Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4601
Full metadata record
DC FieldValueLanguage
dc.contributor.authorGeorgieva, K-
dc.contributor.authorKirov, B-
dc.contributor.authorJavaraiah, J-
dc.date.accessioned2009-06-29T10:41:46Z-
dc.date.available2009-06-29T10:41:46Z-
dc.date.issued2003-09-
dc.identifier.citationA. Wilson., ed., Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, ESA SP-535, Noordwijk: ESA Publications Division, 23 - 28 June 2003, Tatranská Lomnica, Slovak Republic., pp. 323 - 328en
dc.identifier.isbn92-9092-845-X-
dc.identifier.urihttp://hdl.handle.net/2248/4601-
dc.description.abstractThe effect of solar activity on climate depends on the North-South solar activity asymmetry: the correlation between solar activity and a number of meteorological elements has opposite signs for predominantly more active Northern or Southern solar hemispheres. We find that the two hemispheres rotate differently, and show that the interplanetary magnetic field at the Earth's orbit is related to the differential rotation of the more active hemisphere. One feature that is persistently different in the two solar hemispheres is the prevailing magnetic helicity, which is carried to the Earth by magnetic clouds preserving the helicity of the source region of their origin. We show that the reaction of the atmosphere to the arrival of magnetic clouds depends on the helicity of the clouds.en
dc.language.isoenen
dc.publisherEuropean Space Agencyen
dc.relation.ispartofseriesESA SP No. 535-
dc.relation.urihttp://adsabs.harvard.edu/abs/2003ESASP.535..323Gen
dc.subjectSolar-Terrestrial Relationsen
dc.titleSolar asymmetry and sun-earth connectionsen
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Solar asymmetry776.79 kBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.