@Article{TsurutaniLaEcHaNaMaMe:2018:Co“MEx,
author = "Tsurutani, Bruce T. and Lakhina, Gurbax S. and Echer, Ezequiel and
Hajra, Rajkumar and Nayak, Chinmaya and Mannucci, Anthony J. and
Meng, Xing",
affiliation = "{California Institute of Technology} and {Indian Institute of
Geomagnetism} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and LPC2E, CNRS and {George Mason University} and
{California Institute of Technology} and {California Institute of
Technology}",
title = "Comment on “Modeling Extreme “Carrington-Type” Space Weather
Events Using Three-Dimensional Global MHD Simulations” by C. M.
Ngwira, A. Pulkkinen, M. M. Kuznetsova, and A. Glocer”",
journal = "Journal of Geophysical Research: Space Physics",
year = "2018",
volume = "123",
number = "2",
pages = "1388--1392",
month = "Feb.",
abstract = "An alternative scenario to the Ngwira et al. (2014,
https://doi.org/10.1002/2013JA019661) high sheath densities is
proposed for modeling the Carrington magnetic storm. Typical slow
solar wind densities (~5 cm3 ) and lower interplanetary magnetic
cloud magnetic field intensities (~90 nT) can be used to explain
the observed initial and main phase storm features. A second point
is that the fast storm recovery may be explained by ring current
losses due to electromagnetic ion cyclotron wave scattering.",
doi = "10.1002/2017JA024779",
url = "http://dx.doi.org/10.1002/2017JA024779",
issn = "2169-9402",
language = "en",
targetfile = "tsurutani_comment.pdf",
urlaccessdate = "21 maio 2024"
}