@InProceedings{VermaSawa:2004:ReCoMa,
               author = "Verma, V. K. and Sawant, Hanumant Shankar",
          affiliation = "State Observatory, Manora Peak, Naini Tal - 263 129, INDIA",
                title = "Relatioship of coronal mass ejections observed by lasco/soho with 
                         solar flares and coronal holes",
            booktitle = "Proceedings...",
                 year = "2004",
         organization = "COSPAR Scientific Assembly, 35.",
            publisher = "INPE",
             abstract = "The CMEs observed by LASCO coronagraph and associated solar 
                         activity phenomena whose locations were identified by EIT 
                         instruments and solar H-alpha flares observations during years 
                         2000, 2001, 2002 and 2003 indicate that about 40%, 26% and 30% 
                         CMEs were observed when there were coronal holes (CHs) within 
                         1-10, 11-20 and 21-40 degrees, respectively from the location of 
                         solar H-alpha flares. The CHs data used in the study were taken 
                         from KPNO, USA website. From the study carried out in the present 
                         paper we are of the view that CMEs might have been produced by 
                         some mechanism by which the mass ejected by some solar flares or 
                         active prominences, gets connected with open magnetic lines of CHs 
                         (source of high speed solar wind streams) and moves along them to 
                         appear as CMEs.",
  conference-location = "Par{\'{\i}}s, Fran{\c{c}}a",
      conference-year = "18-25 Jul.",
                label = "self-archiving-INPE-MCTIC-GOV-BR",
             language = "en",
                  ibi = "6qtX3pFwXQZsFDuKxG/Fcxws",
                  url = "http://urlib.net/ibi/6qtX3pFwXQZsFDuKxG/Fcxws",
           targetfile = "verma_relationship.pdf",
        urlaccessdate = "04 maio 2024"
}