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@Article{Kane:2011:BaDiCM,
               author = "Kane, Rajaram Purushottam",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "Bartel diagrams for CME occurrence frequency, sunspot numbers and 
                         2800 MHz solar radio emission flux during 2007",
              journal = "Indian Journal of Radio and Space Physics",
                 year = "2011",
               volume = "40",
               number = "3",
                pages = "121--123",
                month = "June",
             keywords = "Coronal mass ejection (CME), Sunspot number, Solar radio emission 
                         flux.",
             abstract = "During 2007, the relationship of the variations in the daily 
                         values of sunspot number (Rz) and the 2800 MHz solar radio 
                         emission F-10 was good only in some intervals, while relationship 
                         of both Rz and F-10 with the coronal mass ejections (CMEs) was 
                         very poor, indicating that CMEs evolve independently of Rz and 
                         F-10.",
                 issn = "0367-8393 and 0975-105X",
             language = "en",
           targetfile = "Kane-IJRSP-v40-n3-p121-123- 40(3) 121-123[1].pdf",
        urlaccessdate = "17 jan. 2021"
}


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