2016
DOI: 10.1016/j.jqsrt.2016.02.009
|View full text |Cite
|
Sign up to set email alerts
|

Controlled time integration for the numerical simulation of meteor radar reflections

Abstract: We model meteoroids entering the Earth's atmosphere as objects surrounded by non-magnetized plasma, and consider ecient numerical simulation of radar reections from meteors in the time domain. Instead of the widely used nite dierence time domain method (FDTD), we use more generalized nite dierences by applying the discrete exterior calculus (DEC) and non-uniform leapfrog-style time discretization. The computational domain is presented by convex polyhedral elements. The convergence of the time integration is ac… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
6
0

Year Published

2016
2016
2022
2022

Publication Types

Select...
4
2

Relationship

4
2

Authors

Journals

citations
Cited by 9 publications
(7 citation statements)
references
References 50 publications
0
6
0
Order By: Relevance
“…1998;William & Murad 2002;Vondrak et al 2008). The high temperature ablated and ionized meteor atoms and electrons, together with ionized and dissociated atmospheric atoms, explosively form a dynamically stable meteor trail cylindrical volume with an initial radius r 0 , which is approximated as a quasineutral plasma that can subsequently be observed by meteor radars (McKinley 1961;Baggaley & Fisher 1980;Räbinä et al 2016). Here, the term initial radius refers to the half-width of the initial (assumed) Gaussian distribution of the ions (or in the case of radio studies, electrons) that has "instantaneously" and adiabatically formed immediately after the passage of the meteoroid, where the volume density of the free electrons is a function of meteoroid mass, size and ionization coefficient (e.g.…”
Section: Shocksmentioning
confidence: 99%
“…1998;William & Murad 2002;Vondrak et al 2008). The high temperature ablated and ionized meteor atoms and electrons, together with ionized and dissociated atmospheric atoms, explosively form a dynamically stable meteor trail cylindrical volume with an initial radius r 0 , which is approximated as a quasineutral plasma that can subsequently be observed by meteor radars (McKinley 1961;Baggaley & Fisher 1980;Räbinä et al 2016). Here, the term initial radius refers to the half-width of the initial (assumed) Gaussian distribution of the ions (or in the case of radio studies, electrons) that has "instantaneously" and adiabatically formed immediately after the passage of the meteoroid, where the volume density of the free electrons is a function of meteoroid mass, size and ionization coefficient (e.g.…”
Section: Shocksmentioning
confidence: 99%
“…We The described algorithms are implemented in C++ programming language, and the parallelization is applied with a message passing interface (MPI). Similarly to other nite dierence approaches, the particular implementation parallelizes almost perfectly, as our previous studies suggest [33].…”
Section: Numerical Experimentsmentioning
confidence: 66%
“…We have further developed the geometric approach and created a generic software system based on it. The system can be employed to solve hyperbolic application problems from classical and quantum physics [24], [29], [31], such as electromagnetic, elastic, and acoustic wave problems, the Schrödinger equation [13], or Gross-Pitayevskii equations [30], and so on. We explain the mathematical foundations of the software system in [22].…”
Section: Differential Geometric Modelsmentioning
confidence: 99%
“…In our earlier papers, we have demonstrated the proposed approach with several numerical experiments. Such experiments include simulations with acoustic, elastodymanic, electromagnetic and quantum mechanic waves [28], [29], [30], [31]. For the extended accuracy, the mesh structures play an essential role [29].…”
Section: Some Numerical Experiments With Space-time Modelsmentioning
confidence: 99%
See 1 more Smart Citation