TY - JOUR

T1 - On application of asymmetric Kan-like exact equilibria to the Earth magnetotail modeling

AU - Korovinskiy, Daniil B.

AU - Kubyshkina, Darya I.

AU - Semenov, Vladimir S.

AU - Kubyshkina, Marina V.

AU - Erkaev, Nikolai V.

AU - Kiehas, Stefan A.

PY - 2018/4/19

Y1 - 2018/4/19

N2 - A specific class of solutions of the Vlasov-Maxwell equations, developed by means of generalization of the well-known Harris-Fadeev-Kan-Manankova family of exact two-dimensional equilibria, is studied. The examined model reproduces the current sheet bending and shifting in the vertical plane, arising from the Earth dipole tilting and the solar wind nonradial propagation. The generalized model allows magnetic configurations with equatorial magnetic fields decreasing in a tailward direction as slow as 1/x, contrary to the original Kan model (1/x(3)); magnetic configurations with a single X point are also available. The analytical solution is compared with the empirical T96 model in terms of the magnetic flux tube volume. It is found that parameters of the analytical model may be adjusted to fit a wide range of averaged magnetotail configurations. The best agreement between analytical and empirical models is obtained for the midtail at distances beyond 10-15 R-E at high levels of magnetospheric activity. The essential model parameters (current sheet scale, current density) are compared to Cluster data of magnetotail crossings. The best match of parameters is found for single-peaked current sheets with medium values of number density, proton temperature and drift velocity.

AB - A specific class of solutions of the Vlasov-Maxwell equations, developed by means of generalization of the well-known Harris-Fadeev-Kan-Manankova family of exact two-dimensional equilibria, is studied. The examined model reproduces the current sheet bending and shifting in the vertical plane, arising from the Earth dipole tilting and the solar wind nonradial propagation. The generalized model allows magnetic configurations with equatorial magnetic fields decreasing in a tailward direction as slow as 1/x, contrary to the original Kan model (1/x(3)); magnetic configurations with a single X point are also available. The analytical solution is compared with the empirical T96 model in terms of the magnetic flux tube volume. It is found that parameters of the analytical model may be adjusted to fit a wide range of averaged magnetotail configurations. The best agreement between analytical and empirical models is obtained for the midtail at distances beyond 10-15 R-E at high levels of magnetospheric activity. The essential model parameters (current sheet scale, current density) are compared to Cluster data of magnetotail crossings. The best match of parameters is found for single-peaked current sheets with medium values of number density, proton temperature and drift velocity.

KW - THIN CURRENT SHEETS

KW - PLASMA SHEET

KW - MAGNETIC-FIELD

KW - CLUSTER OBSERVATIONS

KW - SUBSTORM

KW - CONFIGURATIONS

KW - TAIL

UR - http://www.mendeley.com/research/application-asymmetric-kanlike-exact-equilibria-earth-magnetotail-modeling

U2 - 10.5194/angeo-36-641-2018

DO - 10.5194/angeo-36-641-2018

M3 - статья

VL - 36

SP - 641

EP - 653

JO - Annales Geophysicae

JF - Annales Geophysicae

SN - 0992-7689

IS - 2

ER -