@Article{MunakataKEKKTSDMBSJSDHSK:2018:CoShBu,
author = "Munakata, K. and Kozai, M. and Evenson, Paul and Kuwabara, T. and
Kato, C. and Tokumaru, Munetoshi and Silva, Marlos Rockenbach da
and Dal Lago, Alisson and Mendon{\c{c}}a, Rafael Rodrigues Souza
de and Braga, Carlos Roberto and Schuch, Nelson Jorge and Jassar,
H. K. Al and Sharma, M. M. and Duldig, M. L. and Humble, J. E. and
Sabbah, I. and K{\'o}ta, J.",
affiliation = "{Shinshu University} and Institute of Space and Astronautical
Science, Japan Aerospace Exploration Agency (ISAS/JAXA) and
{University of Delaware} and {University of Delaware} and {Shinshu
University} and {Nagoya University} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Kuwait
University} and {Kuwait University} and {University of Tasmania}
and {University of Tasmania} and College of Health Sciences,
Public Authority of Applied Education and Training, Kuwait City
and {University of Arizona}",
title = "Cosmic-Ray Short Burst Observed with the Global Muon Detector
Network (GMDN) on 2015 June 22",
journal = "Astrophysical Journal",
year = "2018",
volume = "862",
number = "2",
pages = "e170",
month = "Aug.",
keywords = "cosmic rays, interplanetary medium, Sun: coronal mass ejections
(CMEs).",
abstract = "We analyze the short cosmic-ray intensity increase ({"}cosmic-ray
burst{"}: CRB) on 2015 June 22 utilizing a global network of muon
detectors and derive the global anisotropy of cosmic-ray intensity
and the density (i.e., the omnidirectional intensity) with 10
minute time resolution. We find that the CRB was caused by a local
density maximum and an enhanced anisotropy of cosmic rays, both of
which appeared in association with Earth's crossing of the
heliospheric current sheet (HCS). This enhanced anisotropy was
normal to the HCS and consistent with a diamagnetic drift arising
from the spatial gradient of cosmic-ray density, which indicates
that cosmic rays were drifting along the HCS from the north of
Earth. We also find a significant anisotropy along the HCS,
lasting a few hours after the HCS crossing, indicating that cosmic
rays penetrated into the inner heliosphere along the HCS. Based on
the latest geomagnetic field model, we quantitatively evaluate the
reduction of the geomagnetic cutoff rigidity and the variation of
the asymptotic viewing direction of cosmic rays due to a major
geomagnetic storm that occurred during the CRB and conclude that
the CRB is not caused by the geomagnetic storm, but by a rapid
change in the cosmic-ray anisotropy and density outside the
magnetosphere.",
doi = "10.3847/1538-4357/aacdfe",
url = "http://dx.doi.org/10.3847/1538-4357/aacdfe",
issn = "0004-637X and 1538-4357",
language = "en",
targetfile = "munakata_cosmic.pdf",
urlaccessdate = "23 maio 2024"
}