Electron dynamics in a subproton‐gyroscale magnetic hole
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U. Gliese | J. Sauvaud | T. Moore | B. Lavraud | Y. Saito | D. Gershman | W. Paterson | R. Torbert | J. Burch | E. MacDonald | C. Pollock | J. Dorelli | R. Strangeway | A. Viñas | Christopher T. Russell | B. Giles | K. Goodrich | Li‐Jen Chen | V. Coffey | L. Avanov | M. Chandler | A. Barrie | M. Holland | C. Salo | Charles Dickson | Yoshifumi Saito | C. Russell
[1] U. Gliese,et al. Fast Plasma Investigation for Magnetospheric Multiscale , 2016 .
[2] Wolfgang Baumjohann,et al. The Magnetospheric Multiscale Magnetometers , 2016 .
[3] D. Gershman,et al. The calculation of moment uncertainties from velocity distribution functions with random errors , 2015 .
[4] H. Karimabadi,et al. Generation of magnetic holes in fully kinetic simulations of collisionless turbulence , 2015, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences.
[5] T. Sundberg,et al. Properties and origin of subproton‐scale magnetic holes in the terrestrial plasma sheet , 2015 .
[6] T. Sundberg,et al. Electron vortex magnetic holes: A nonlinear coherent plasma structure , 2014, 1412.5928.
[7] M. Balikhin,et al. Magnetic holes in the vicinity of dipolarization fronts: Mirror or tearing structures? , 2012 .
[8] M. Dunlop,et al. Cluster and TC-1 observation of magnetic holes in the plasma sheet , 2012 .
[9] O. Amariutei,et al. Occurrence rate of magnetic holes between 0.72 and 1 AU: comparative study of Cluster and VEX data , 2011 .
[10] D. Constantinescu,et al. Magnetosheath and heliosheath mirror mode structures, interplanetary magnetic decreases, and linear magnetic decreases: Differences and distinguishing features , 2011 .
[11] O. D. Constantinescu,et al. Case studies of mirror‐mode structures observed by THEMIS in the near‐Earth tail during substorms , 2011 .
[12] N. Omidi,et al. Mirror mode waves: Messengers from the coronal heating region , 2008 .
[13] P. Shukla,et al. Theory for two-dimensional electron and ion Bernstein-Greene-Kruskal modes in a magnetized plasma , 2007 .
[14] J. Kasper,et al. A scale-free analysis of magnetic holes at 1 AU , 2007 .
[15] A. Bhattacharjee,et al. Bernstein-Greene-Kruskal modes in a three-dimensional plasma. , 2005, Physical review letters.
[16] A. Balogh,et al. Relationship between discontinuities, magnetic holes, magnetic decreases, and nonlinear Alfvén waves: Ulysses observations over the solar poles , 2002 .
[17] P. Seeluangsawat. Magnetic holes in the solar wind , 2002 .
[18] B. Tsurutani,et al. Generation mechanism for magnetic holes in the solar wind , 2001 .
[19] J. Richardson,et al. Evolution of mirror structures in the magnetosheath of Saturn from the bow shock to the magnetopause , 1998 .
[20] A. Balogh,et al. Ulysses field and plasma observations of magnetic holes in the solar wind and their relation to mirror‐mode structures , 1994 .
[21] B. Tsurutani,et al. Nonlinear magnetosonic waves and mirror mode structures in the March 1991 Ulysses interplanetary event , 1992 .
[22] C. Russell,et al. Mirror instability in the magnetosphere of comet Halley , 1987 .
[23] L. Burlaga,et al. Structure of current sheets in magnetic holes at 1 AU. [regions of low magnetic field intensity in the solar wind , 1978 .
[24] L. Burlaga,et al. Magnetic holes in the solar wind , 1976 .
[25] A. Hasegawa. Drift Mirror Instability in the Magnetosphere , 1969 .