LEADER 03627nam 22006015 450 001 9910427692203321 005 20200812180846.0 010 $a3-030-51510-9 024 7 $a10.1007/978-3-030-51510-2 035 $a(CKB)4100000011384300 035 $a(DE-He213)978-3-030-51510-2 035 $a(MiAaPQ)EBC6299443 035 $a(PPN)250215640 035 $a(EXLCZ)994100000011384300 100 $a20200812d2020 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aMathematical Modelling of Meteoroid Streams /$fby Galina O. Ryabova 205 $a1st ed. 2020. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2020. 215 $a1 online resource (VIII, 68 p. 16 illus., 8 illus. in color.) 225 1 $aSpringerBriefs in Astronomy,$x2191-9100 311 $a3-030-51509-5 320 $aIncludes bibliographical references and index. 327 $aPreface -- 1. Introduction -- 2. Initial stage: the model stream generation -- 3. The model stream evolution -- 4. The end stage: the model stream now -- 5. Visualization of the results -- 6. Application to real streams, analysis -- Notation conventions -- Glossary -- References -- A1. Transition from the rectangular coordinates to the orbital elements and back -- A2. Transition between the coordinate systems -- A3. Random number generation -- Index. 330 $aModern computer power and high-precision observational data have greatly improved the reliability of meteoroid stream models. At present, scientific research calls for two kinds of models: precise ones for individual streams, and statistically averaged ones for Solar System dust distribution models. Thus, there is a wide field of study open to stream modellers. This brief describes step-by-step computer simulations of meteoroid stream formation and evolution. Detailed derivations of relevant formulae are given, along with plenty of helpful, digestible figures explaining the subtleties of the method. Each theoretical section ends with examples aimed to help readers practice and master the material. Most of the examples are based on the Geminid meteoroid stream model, which has been developed by the author in the last 30 years. The book is intended for researchers interested in meteor astronomy and mathematical modelling, and it is also accessible to physics and astrophysics students. 410 0$aSpringerBriefs in Astronomy,$x2191-9100 606 $aAstrophysics 606 $aMathematical physics 606 $aSociophysics 606 $aEconophysics 606 $aTheoretical Astrophysics$3https://scigraph.springernature.com/ontologies/product-market-codes/P22080 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aData-driven Science, Modeling and Theory Building$3https://scigraph.springernature.com/ontologies/product-market-codes/P33030 615 0$aAstrophysics. 615 0$aMathematical physics. 615 0$aSociophysics. 615 0$aEconophysics. 615 14$aTheoretical Astrophysics. 615 24$aAstrophysics and Astroparticles. 615 24$aData-driven Science, Modeling and Theory Building. 676 $a523.01 700 $aRyabova$b Galina O$4aut$4http://id.loc.gov/vocabulary/relators/aut$0843207 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910427692203321 996 $aMathematical Modelling of Meteoroid Streams$91881675 997 $aUNINA LEADER 00762nam0-2200241 --450 001 9910985191903321 005 20250317155214.0 100 $a20250317d1939----kmuy0itay5050 ba 101 0 $aita$cita 102 $aIT 105 $a 001yy 200 1 $aLabranda e labyrinthos$fGiovanni Pugliese Carratelli 210 $aNapoli$cArti grafiche$d1939 215 $a20 p.$d24 cm 300 $aEstr. da: Rendiconti della R. Accademia di archeologia, lettere e belle arti della Società Reale di Napoli, 1939 700 1$aPugliese Carratelli,$bGiovanni$023324 801 0$aIT$bUNINA$gREICAT$2UNIMARC 901 $aLG 912 $a9910985191903321 952 $aOPUSC. 46 (030)$fFLFBC 959 $aFLFBC 996 $aLabranda e labyrinthos$9595593 997 $aUNINA