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Browsing by Author "Echer, Ezequiel"

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Comment on “Comment on the abundances of rotational and tangential discontinuities in the solar wind” by M. Neugebauer

Tsurutani, B.T.; Lakhina, G.S.; Verkhoglyadova, O.P.; Echer, Ezequiel; Guarnieri, Fernando L. (2007)
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”

Tsurutani, Bruce T.; Lakhina, G.S.; Echer, Ezequiel; Hajra, Rajkumar; Nayak, Chinmaya; Mannucci, Anthony J.; Meng, Xing (2018)

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 cm 3) and lower ...
Cross-field diffusion of energetic (100 ke V to 2 Me V) protons in interplanetary space

Costa Jr, Edio da; Tsurutani, B.T.; Alves, Maria Virgínia; Echer, Ezequiel; Lakhina, G.S. (2013)

Magnetic field magnitude decreases (MDs) are observed in several regions of the interplanetary medium. In this paper, we characterize MDs observed by the Ulysses spacecraft instrumentation over the solar south pole by using ...
Magnetic decrease formation from <1 AU to ∼5 AU: Corotating interaction region reverse shocks

Tsurutani, B.T.; Guarnieri, Fernando L.; Echer, Ezequiel; Lakhina, G.S.; Verkhoglyadova, Olga P. (2009)

Magnetic decreases (MDs) have been identified and studied throughout a Ulysses fast latitude scan that lasted from 29 February 1992 to 14 September 1993. Ulysses' distance was ∼5 AU from the Sun. MDs were unbiasedly selected ...
Magnetosheath and heliosheath mirror mode structures, interplanetary magnetic decreases, and linear magnetic decreases: Differences and distinguishing features

Tsurutani, B.T.; Lakhina, G.S.; Verkhoglyadova, Olga P.; Echer, Ezequiel; Guarnieri, Fernando L.; Narita, Yasuhito; Constantinescu, Dragos O. (2011)

There has been considerable confusion in the literature about what mirror mode (MM), magnetic decrease (MD), and linear magnetic decrease (LMD) structures are and are not. We will reexamine past spacecraft observations to ...
Mirror instability upstream of the termination shock (TS) and in the heliosheath

Tsurutani, B.T.; Echer, Ezequiel; Verkhoglyadova, Olga P.; Lakhina, G.S.; Guarnieri, F.L. (2011)

We experimentally identify mirror mode (MM) structures in the Voyager 1 heliosheath data for the first time. This is done using the magnetic field data alone. The heliosheath MM structures are found to have the following ...

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Browsing by Author "Echer, Ezequiel"

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