@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 = "28 abr. 2024"
}