A Sketch of an Orbital—Momentum—Based Criterion of Diversity of Two Keplerian Orbits View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2001

AUTHORS

L. Neslušan

ABSTRACT

If a database of meteors contains not only the data on their radiant and geocentric velocity, but also their orbits, then the meteors of a particular shower can be separated from the database evaluating the similarity of orbits of individual shower-members. The Southworth-Hawkins’ D-criterion has most frequently been utilized in this evaluation. This criterion is based on a mathematical quantification of diversity of two cone-section curves in space. Though it has appeared to be quite well applicable, some authors have objected that no dynamical aspects of evolution of a given orbit into other are respected within the criterion. The objection cannot be accepted absolutely, because we usually solve an inverse problem in the practice: to study the dynamical evolution of a meteor stream separated on the basis of considered criterion. A knowledge of the dynamics is aim of study and it cannot be included in the initial assumptions. More... »

PAGES

365-366

Book

TITLE

Dynamics of Natural and Artificial Celestial Bodies

ISBN

978-90-481-5865-2
978-94-017-1327-6

Author Affiliations

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-017-1327-6_61

DOI

http://dx.doi.org/10.1007/978-94-017-1327-6_61

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1037052558


Indexing Status Check whether this publication has been indexed by Scopus and Web Of Science using the SN Indexing Status Tool
Incoming Citations Browse incoming citations for this publication using opencitations.net

JSON-LD is the canonical representation for SciGraph data.

TIP: You can open this SciGraph record using an external JSON-LD service: JSON-LD Playground Google SDTT

[
  {
    "@context": "https://springernature.github.io/scigraph/jsonld/sgcontext.json", 
    "about": [
      {
        "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/0101", 
        "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
        "name": "Pure Mathematics", 
        "type": "DefinedTerm"
      }, 
      {
        "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/01", 
        "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
        "name": "Mathematical Sciences", 
        "type": "DefinedTerm"
      }
    ], 
    "author": [
      {
        "affiliation": {
          "alternateName": "Astronomical Institute", 
          "id": "https://www.grid.ac/institutes/grid.493212.f", 
          "name": [
            "Astronomical Institute, Slovak Academy of Sciences, 059 60\u00a0Tatransk\u00e1 Lomnica, Slovakia"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Neslu\u0161an", 
        "givenName": "L.", 
        "id": "sg:person.012152240735.08", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.012152240735.08"
        ], 
        "type": "Person"
      }
    ], 
    "datePublished": "2001", 
    "datePublishedReg": "2001-01-01", 
    "description": "If a database of meteors contains not only the data on their radiant and geocentric velocity, but also their orbits, then the meteors of a particular shower can be separated from the database evaluating the similarity of orbits of individual shower-members. The Southworth-Hawkins\u2019 D-criterion has most frequently been utilized in this evaluation. This criterion is based on a mathematical quantification of diversity of two cone-section curves in space. Though it has appeared to be quite well applicable, some authors have objected that no dynamical aspects of evolution of a given orbit into other are respected within the criterion. The objection cannot be accepted absolutely, because we usually solve an inverse problem in the practice: to study the dynamical evolution of a meteor stream separated on the basis of considered criterion. A knowledge of the dynamics is aim of study and it cannot be included in the initial assumptions.", 
    "editor": [
      {
        "familyName": "Pretka-Ziomek", 
        "givenName": "Halina", 
        "type": "Person"
      }, 
      {
        "familyName": "Wnuk", 
        "givenName": "Edwin", 
        "type": "Person"
      }, 
      {
        "familyName": "Seidelmann", 
        "givenName": "P. Kenneth", 
        "type": "Person"
      }, 
      {
        "familyName": "Richardson", 
        "givenName": "David L.", 
        "type": "Person"
      }
    ], 
    "genre": "chapter", 
    "id": "sg:pub.10.1007/978-94-017-1327-6_61", 
    "inLanguage": [
      "en"
    ], 
    "isAccessibleForFree": false, 
    "isPartOf": {
      "isbn": [
        "978-90-481-5865-2", 
        "978-94-017-1327-6"
      ], 
      "name": "Dynamics of Natural and Artificial Celestial Bodies", 
      "type": "Book"
    }, 
    "name": "A Sketch of an Orbital\u2014Momentum\u2014Based Criterion of Diversity of Two Keplerian Orbits", 
    "pagination": "365-366", 
    "productId": [
      {
        "name": "doi", 
        "type": "PropertyValue", 
        "value": [
          "10.1007/978-94-017-1327-6_61"
        ]
      }, 
      {
        "name": "readcube_id", 
        "type": "PropertyValue", 
        "value": [
          "b0813b81901cf5bda3916776937f664df085079e9722e509e60cff5e20896891"
        ]
      }, 
      {
        "name": "dimensions_id", 
        "type": "PropertyValue", 
        "value": [
          "pub.1037052558"
        ]
      }
    ], 
    "publisher": {
      "location": "Dordrecht", 
      "name": "Springer Netherlands", 
      "type": "Organisation"
    }, 
    "sameAs": [
      "https://doi.org/10.1007/978-94-017-1327-6_61", 
      "https://app.dimensions.ai/details/publication/pub.1037052558"
    ], 
    "sdDataset": "chapters", 
    "sdDatePublished": "2019-04-15T22:43", 
    "sdLicense": "https://scigraph.springernature.com/explorer/license/", 
    "sdPublisher": {
      "name": "Springer Nature - SN SciGraph project", 
      "type": "Organization"
    }, 
    "sdSource": "s3://com-uberresearch-data-dimensions-target-20181106-alternative/cleanup/v134/2549eaecd7973599484d7c17b260dba0a4ecb94b/merge/v9/a6c9fde33151104705d4d7ff012ea9563521a3ce/jats-lookup/v90/0000000001_0000000264/records_8695_00000063.jsonl", 
    "type": "Chapter", 
    "url": "http://link.springer.com/10.1007/978-94-017-1327-6_61"
  }
]
 

Download the RDF metadata as:  json-ld nt turtle xml License info

HOW TO GET THIS DATA PROGRAMMATICALLY:

JSON-LD is a popular format for linked data which is fully compatible with JSON.

curl -H 'Accept: application/ld+json' 'https://scigraph.springernature.com/pub.10.1007/978-94-017-1327-6_61'

N-Triples is a line-based linked data format ideal for batch operations.

curl -H 'Accept: application/n-triples' 'https://scigraph.springernature.com/pub.10.1007/978-94-017-1327-6_61'

Turtle is a human-readable linked data format.

curl -H 'Accept: text/turtle' 'https://scigraph.springernature.com/pub.10.1007/978-94-017-1327-6_61'

RDF/XML is a standard XML format for linked data.

curl -H 'Accept: application/rdf+xml' 'https://scigraph.springernature.com/pub.10.1007/978-94-017-1327-6_61'


 

This table displays all metadata directly associated to this object as RDF triples.

80 TRIPLES      22 PREDICATES      27 URIs      20 LITERALS      8 BLANK NODES

Subject Predicate Object
1 sg:pub.10.1007/978-94-017-1327-6_61 schema:about anzsrc-for:01
2 anzsrc-for:0101
3 schema:author N628d2acd5e804824b58478d4c98c273f
4 schema:datePublished 2001
5 schema:datePublishedReg 2001-01-01
6 schema:description If a database of meteors contains not only the data on their radiant and geocentric velocity, but also their orbits, then the meteors of a particular shower can be separated from the database evaluating the similarity of orbits of individual shower-members. The Southworth-Hawkins’ D-criterion has most frequently been utilized in this evaluation. This criterion is based on a mathematical quantification of diversity of two cone-section curves in space. Though it has appeared to be quite well applicable, some authors have objected that no dynamical aspects of evolution of a given orbit into other are respected within the criterion. The objection cannot be accepted absolutely, because we usually solve an inverse problem in the practice: to study the dynamical evolution of a meteor stream separated on the basis of considered criterion. A knowledge of the dynamics is aim of study and it cannot be included in the initial assumptions.
7 schema:editor Nacb948fc05024daf9f1c632042e877b4
8 schema:genre chapter
9 schema:inLanguage en
10 schema:isAccessibleForFree false
11 schema:isPartOf N5864e5c205c7441b84156c65f1eefe06
12 schema:name A Sketch of an Orbital—Momentum—Based Criterion of Diversity of Two Keplerian Orbits
13 schema:pagination 365-366
14 schema:productId N7ae43abe68d14e66a8fd375d989ea4db
15 N7ca7f373fc63460d9319e843846a6b55
16 Nac0e6096288141f0b7a25e94a0447060
17 schema:publisher N385c0db997d045af9ba0ac1d537b70ea
18 schema:sameAs https://app.dimensions.ai/details/publication/pub.1037052558
19 https://doi.org/10.1007/978-94-017-1327-6_61
20 schema:sdDatePublished 2019-04-15T22:43
21 schema:sdLicense https://scigraph.springernature.com/explorer/license/
22 schema:sdPublisher Ne8379742de7b46fca9bb616a84cd649c
23 schema:url http://link.springer.com/10.1007/978-94-017-1327-6_61
24 sgo:license sg:explorer/license/
25 sgo:sdDataset chapters
26 rdf:type schema:Chapter
27 N0befac8ee291492b9dbb6bcb49455558 rdf:first Nef86e1ce6be84ab5bdb50942d0bbd03c
28 rdf:rest N9d43dcf4366a46a084da0ee69372cdf3
29 N1a0f7aa435c54a68a3a7423e85461608 rdf:first N89c0f126f10445c488dbe8bdedd3104e
30 rdf:rest N0befac8ee291492b9dbb6bcb49455558
31 N385c0db997d045af9ba0ac1d537b70ea schema:location Dordrecht
32 schema:name Springer Netherlands
33 rdf:type schema:Organisation
34 N5864e5c205c7441b84156c65f1eefe06 schema:isbn 978-90-481-5865-2
35 978-94-017-1327-6
36 schema:name Dynamics of Natural and Artificial Celestial Bodies
37 rdf:type schema:Book
38 N5f6fb66da03a4dc59f27b32c83843bce schema:familyName Pretka-Ziomek
39 schema:givenName Halina
40 rdf:type schema:Person
41 N62856d0ea4d94263bfbd279b52e10f02 schema:familyName Richardson
42 schema:givenName David L.
43 rdf:type schema:Person
44 N628d2acd5e804824b58478d4c98c273f rdf:first sg:person.012152240735.08
45 rdf:rest rdf:nil
46 N7ae43abe68d14e66a8fd375d989ea4db schema:name dimensions_id
47 schema:value pub.1037052558
48 rdf:type schema:PropertyValue
49 N7ca7f373fc63460d9319e843846a6b55 schema:name doi
50 schema:value 10.1007/978-94-017-1327-6_61
51 rdf:type schema:PropertyValue
52 N89c0f126f10445c488dbe8bdedd3104e schema:familyName Wnuk
53 schema:givenName Edwin
54 rdf:type schema:Person
55 N9d43dcf4366a46a084da0ee69372cdf3 rdf:first N62856d0ea4d94263bfbd279b52e10f02
56 rdf:rest rdf:nil
57 Nac0e6096288141f0b7a25e94a0447060 schema:name readcube_id
58 schema:value b0813b81901cf5bda3916776937f664df085079e9722e509e60cff5e20896891
59 rdf:type schema:PropertyValue
60 Nacb948fc05024daf9f1c632042e877b4 rdf:first N5f6fb66da03a4dc59f27b32c83843bce
61 rdf:rest N1a0f7aa435c54a68a3a7423e85461608
62 Ne8379742de7b46fca9bb616a84cd649c schema:name Springer Nature - SN SciGraph project
63 rdf:type schema:Organization
64 Nef86e1ce6be84ab5bdb50942d0bbd03c schema:familyName Seidelmann
65 schema:givenName P. Kenneth
66 rdf:type schema:Person
67 anzsrc-for:01 schema:inDefinedTermSet anzsrc-for:
68 schema:name Mathematical Sciences
69 rdf:type schema:DefinedTerm
70 anzsrc-for:0101 schema:inDefinedTermSet anzsrc-for:
71 schema:name Pure Mathematics
72 rdf:type schema:DefinedTerm
73 sg:person.012152240735.08 schema:affiliation https://www.grid.ac/institutes/grid.493212.f
74 schema:familyName Neslušan
75 schema:givenName L.
76 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.012152240735.08
77 rdf:type schema:Person
78 https://www.grid.ac/institutes/grid.493212.f schema:alternateName Astronomical Institute
79 schema:name Astronomical Institute, Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Slovakia
80 rdf:type schema:Organization
 




Preview window. Press ESC to close (or click here)


...