@Article{MunakataKKHKKTMEDSSBBASDHSEMKRSMNK:2022:LaBiAn,
author = "Munakata, K. and Kozai, M. and Kato, C. and Hayashi, Y. and
Kataoka, R. and Kadokura, A. and Tokumaru, M. and Mendon{\c{c}}a,
Rafael Rodrigues Souza and Echer, Ezequiel and Dal Lago, Alisson
and Silva, Marlos Rockenbach da and Schuch, Nelson Jorge and
Bageston, Jos{\'e} Valentin and Braga, C. R. and Al Jassar, H. K.
and Sharma, M. M. and Duldig, M. L. and Humble, J. E. and Sabbah,
I. and Evenson, P. and Mangeard, P-S. and Kuwabara, T. and
Ruffolo, D. and Saiz, A. and Mitthumsiri, W. and Nuntiyakul, W.
and Kota, J.",
affiliation = "{Shinshu University } and {Polar Environment Data Science Center }
and {Shinshu University } and {Shinshu University } and {National
Institute of Polar Research } and {Polar Environment Data Science
Center } 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 {Instituto
Nacional de Pesquisas Espaciais (INPE) } and {George Mason
University } 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 Delaware } and
{University of Delaware } and {University of Delaware } and
{Mahidol University } and {Mahidol University } and {Mahidol
University } and {Chiang Mai University } and {University of
Arizona}",
title = "Large-amplitude Bidirectional Anisotropy of Cosmic-Ray Intensity
Observed with Worldwide Networks of Ground-based Neutron Monitors
and Muon Detectors in 2021 November",
journal = "Astrophysical Journal",
year = "2022",
volume = "938",
number = "1",
pages = "e30",
month = "Oct.",
abstract = "We analyze the cosmic-ray variations during a significant Forbush
decrease observed with worldwide networks of ground-based neutron
monitors and muon detectors during 2021 November 3-5. Utilizing
the difference between primary cosmic-ray rigidities monitored by
neutron monitors and muon detectors, we deduce the rigidity
spectra of the cosmic-ray density (or omnidirectional intensity)
and the first- and second-order anisotropies separately for each
hour of data. A clear two-step decrease is seen in the cosmic-ray
density with the first similar to 2% decrease after the
interplanetary shock arrival followed by the second similar to 5%
decrease inside the magnetic flux rope (MFR) at 15 GV. Most
strikingly, a large bidirectional streaming along the magnetic
field is observed in the MFR with a peak amplitude of similar to
5% at 15 GV, which is comparable to the total density decrease
inside the MFR. The bidirectional streaming could be explained by
adiabatic deceleration and/or focusing in the expanding MFR, which
have stronger effects for pitch angles near 90 degrees, or by
selective entry of GCRs along a leg of the MFR. The peak
anisotropy and density depression in the flux rope both decrease
with increasing rigidity. The spectra vary dynamically, indicating
that the temporal variations of density and anisotropy appear
different in neutron monitor and muon detector data.",
doi = "10.3847/1538-4357/ac91c5",
url = "http://dx.doi.org/10.3847/1538-4357/ac91c5",
issn = "0004-637X and 1538-4357",
language = "en",
targetfile = "Munakata_2022_ApJ_938_30.pdf",
urlaccessdate = "13 maio 2024"
}