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@Article{Echer:2019:InShPa,
               author = "Echer, Ezequiel",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "Interplanetary shock parameters near Jupiter's orbit",
              journal = "Geophysical Research Letters",
                 year = "2019",
               volume = "2019",
                pages = "082126",
             abstract = "Fast interplanetary shocks occurrence, their parameters, and 
                         drivers near Jupiter's orbit are determined in this paper. It was 
                         found that 70% of the fast shocks are forward (FS) and 30% are 
                         reverse (RS). Interplanetary coronal mass ejection\‐driven 
                         FS occur more frequently in all solar cycle phases except in the 
                         declining phase, when corotating interaction region\‐driven 
                         shocks predominate. Most of the shocks were 
                         quasi\‐perpendicularly (65 to 70) propagating relative to 
                         the ambient interplanetary magnetic field. The average shock 
                         magnetosonic Mach number is slightly higher for FS (2.6) than for 
                         RS (2.4), which in turn are stronger than shocks near 1 and 10 AU 
                         reported in previous works. This occurs because of the full 
                         development of corotating interaction region shocks and higher 
                         occurrence of strong interplanetary coronal mass ejections near 5 
                         AU and that the magnetosonic speed at 5 AU has only 60% of its 
                         value at 1 AU.",
                  doi = "10.1029/2019GL082126",
                  url = "http://dx.doi.org/10.1029/2019GL082126",
                 issn = "0094-8276",
             language = "en",
           targetfile = "Interplanetary Shock Parameters Near Jupiter's Orbit.pdf",
        urlaccessdate = "29 nov. 2020"
}


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