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Titlebook: Mathematical Modelling of Meteoroid Streams; Galina O. Ryabova Book 2020 The Editor(s) (if applicable) and The Author(s), under exclusive

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11#
發(fā)表于 2025-3-23 10:08:51 | 只看該作者
978-3-030-51509-6The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerl
12#
發(fā)表于 2025-3-23 13:53:42 | 只看該作者
Mathematical Modelling of Meteoroid Streams978-3-030-51510-2Series ISSN 2191-9100 Series E-ISSN 2191-9119
13#
發(fā)表于 2025-3-23 19:58:32 | 只看該作者
14#
發(fā)表于 2025-3-23 23:34:31 | 只看該作者
Initial Stage: The Model Stream Generation,rent body orbit we choose points of ejection according to some law of distribution using a generator of pseudo-random numbers. Then the meteoroid orbital elements are calculated. The chapter explains how to do that. The computer code for the main points is provided.
15#
發(fā)表于 2025-3-24 04:25:19 | 只看該作者
Application to Real Streams,at attracted your particular interest. Since you read as far as the sixth chapter, I hope you are interested. So I suggest the Geminid 2007 model as the concluding exercise to master the studied theory and to test your software.
16#
發(fā)表于 2025-3-24 08:13:51 | 只看該作者
Introduction,This chapter explains what is mathematical modelling of meteoroid streams and outlines its history.
17#
發(fā)表于 2025-3-24 12:29:44 | 只看該作者
The Model Stream Evolution,The chapter discusses the numerical integration of the model stream orbits, and gives a ready for use half-analytical method for the Geminid stream modelling.
18#
發(fā)表于 2025-3-24 17:30:30 | 只看該作者
The End Stage: The Model Stream Now,At this stage of modelling we have a final model stream consisting of millions of orbits. To compare the model and observations we use mainly flux density profile of the meteor shower, mass distribution profile, and radiant configuration. In this chapter they are discussed in the style ‘how to do’.
19#
發(fā)表于 2025-3-24 21:43:32 | 只看該作者
20#
發(fā)表于 2025-3-25 01:20:06 | 只看該作者
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