Simulation dataset of "Whistler-mode waves trapped by density irregularities in the Earth's magnetosphere"
Creators
- 1. CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Science, University of Science and Technology of China, Hefei 230026, China
- 2. Department of Physics, University of Texas at Dallas, Richardson, Texas, USA
- 3. Physics Department, Auburn University, Auburn, Alabama, USA
Description
Bx1, By1 and Bz1 are three components of magnetic fields in field-oriented coordinate system for simulation case 1.
Bx2, By2 and Bz2 are three components of magnetic fields in field-oriented coordinate system for simulation case 2.
Bx3, By3 and Bz3 are three components of magnetic fields in field-oriented coordinate system for simulation case 3.
Each file such as Bx1 stores an array with the form Bx1[Nper,Npar,1,Nt], where Nper=301 and Npar=1001 are perpendicular and parallel (to magnetic field lines) output grid-point numbers in the whole simulation domain, Nt=1251 is output time steps. The output time interval is 2 time unit.
grid_points.dat stores output grid-point locations: x and z in Cartesian coordinates with the form x[Nper,Npar] and z[Nper,Npar], which can be read by grid_points.pro (an Interactive Data Language IDL procedure).
Files
Files
(13.6 GB)
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md5:1a6892a11024857ad4bdd3f8cfd5c4ea
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1.5 GB | Download |
md5:68fec4b0aad6c7e1e9964a4267b9df65
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md5:c5140234e7215e42ba570f155865c125
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md5:8e922e8212f550157864a4e4e4c20b55
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1.5 GB | Download |
md5:b25a586600c3c3f23275f364bda1ab3c
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1.5 GB | Download |
md5:db5698c2dbdb3feb549b16157f9e120e
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1.5 GB | Download |
md5:9a7a444098d4de44c5fb27a51c50c43a
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1.5 GB | Download |
md5:d768f26e54d40cec21d478116cd65615
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1.5 GB | Download |
md5:6e033ba36fed20287aa30f105dfca559
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1.5 GB | Download |
md5:321ef647d6fe6c145081ef654dfb5d13
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8.0 MB | Download |
md5:05fb2ccf68bc96693e54e35dfe703156
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154 Bytes | Download |