Theoretical spectrum of solar convection View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1991

AUTHORS

H. M. Antia , S. M. Chitre

ABSTRACT

The theoretical power spectrum of solar velocity field and flux variation is obtained with amplitudes of the unstable convective eigenmodes determined by linearly superposing these modes to yield the model convective flux profile. The numerical results are compared with the observed spectrum of solar convection and the technique is applied to other stars. More... »

PAGES

157-162

Book

TITLE

Challenges to Theories of the Structure of Moderate-Mass Stars

ISBN

978-3-540-54420-3
978-3-540-38355-0

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/3-540-54420-8_62

DOI

http://dx.doi.org/10.1007/3-540-54420-8_62

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1047882289


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/2008/09", 
        "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
        "name": "Engineering", 
        "type": "DefinedTerm"
      }, 
      {
        "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/0915", 
        "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
        "name": "Interdisciplinary Engineering", 
        "type": "DefinedTerm"
      }
    ], 
    "author": [
      {
        "affiliation": {
          "alternateName": "Tata Institute of Fundamental Research, Homi Bhabha Road, 400 005, Colaba, Bombay, India", 
          "id": "http://www.grid.ac/institutes/grid.22401.35", 
          "name": [
            "Tata Institute of Fundamental Research, Homi Bhabha Road, 400 005, Colaba, Bombay, India"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Antia", 
        "givenName": "H. M.", 
        "id": "sg:person.011311320105.13", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.011311320105.13"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Tata Institute of Fundamental Research, Homi Bhabha Road, 400 005, Colaba, Bombay, India", 
          "id": "http://www.grid.ac/institutes/grid.22401.35", 
          "name": [
            "Tata Institute of Fundamental Research, Homi Bhabha Road, 400 005, Colaba, Bombay, India"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Chitre", 
        "givenName": "S. M.", 
        "id": "sg:person.015153633273.13", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.015153633273.13"
        ], 
        "type": "Person"
      }
    ], 
    "datePublished": "1991", 
    "datePublishedReg": "1991-01-01", 
    "description": "The theoretical power spectrum of solar velocity field and flux variation is obtained with amplitudes of the unstable convective eigenmodes determined by linearly superposing these modes to yield the model convective flux profile. The numerical results are compared with the observed spectrum of solar convection and the technique is applied to other stars.", 
    "editor": [
      {
        "familyName": "Gough", 
        "givenName": "Douglas", 
        "type": "Person"
      }, 
      {
        "familyName": "Toomre", 
        "givenName": "Juri", 
        "type": "Person"
      }
    ], 
    "genre": "chapter", 
    "id": "sg:pub.10.1007/3-540-54420-8_62", 
    "inLanguage": "en", 
    "isAccessibleForFree": false, 
    "isPartOf": {
      "isbn": [
        "978-3-540-54420-3", 
        "978-3-540-38355-0"
      ], 
      "name": "Challenges to Theories of the Structure of Moderate-Mass Stars", 
      "type": "Book"
    }, 
    "keywords": [
      "solar convection", 
      "velocity field", 
      "flux profiles", 
      "solar velocity field", 
      "convection", 
      "numerical results", 
      "theoretical power spectrum", 
      "flux variations", 
      "power spectrum", 
      "eigenmodes", 
      "field", 
      "mode", 
      "amplitude", 
      "technique", 
      "spectra", 
      "results", 
      "profile", 
      "variation", 
      "observed spectra", 
      "theoretical spectra", 
      "stars", 
      "unstable convective eigenmodes", 
      "convective eigenmodes", 
      "model convective flux profile", 
      "convective flux profile"
    ], 
    "name": "Theoretical spectrum of solar convection", 
    "pagination": "157-162", 
    "productId": [
      {
        "name": "dimensions_id", 
        "type": "PropertyValue", 
        "value": [
          "pub.1047882289"
        ]
      }, 
      {
        "name": "doi", 
        "type": "PropertyValue", 
        "value": [
          "10.1007/3-540-54420-8_62"
        ]
      }
    ], 
    "publisher": {
      "name": "Springer Nature", 
      "type": "Organisation"
    }, 
    "sameAs": [
      "https://doi.org/10.1007/3-540-54420-8_62", 
      "https://app.dimensions.ai/details/publication/pub.1047882289"
    ], 
    "sdDataset": "chapters", 
    "sdDatePublished": "2021-12-01T20:12", 
    "sdLicense": "https://scigraph.springernature.com/explorer/license/", 
    "sdPublisher": {
      "name": "Springer Nature - SN SciGraph project", 
      "type": "Organization"
    }, 
    "sdSource": "s3://com-springernature-scigraph/baseset/20211201/entities/gbq_results/chapter/chapter_81.jsonl", 
    "type": "Chapter", 
    "url": "https://doi.org/10.1007/3-540-54420-8_62"
  }
]
 

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.10.1007/3-540-54420-8_62'

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

curl -H 'Accept: application/n-triples' 'https://scigraph.springernature.com/pub.10.1007/3-540-54420-8_62'

Turtle is a human-readable linked data format.

curl -H 'Accept: text/turtle' 'https://scigraph.springernature.com/pub.10.1007/3-540-54420-8_62'

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

curl -H 'Accept: application/rdf+xml' 'https://scigraph.springernature.com/pub.10.1007/3-540-54420-8_62'


 

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

97 TRIPLES      23 PREDICATES      51 URIs      44 LITERALS      7 BLANK NODES

Subject Predicate Object
1 sg:pub.10.1007/3-540-54420-8_62 schema:about anzsrc-for:09
2 anzsrc-for:0915
3 schema:author Nb6b8284f5f01498e880f600f94f724cf
4 schema:datePublished 1991
5 schema:datePublishedReg 1991-01-01
6 schema:description The theoretical power spectrum of solar velocity field and flux variation is obtained with amplitudes of the unstable convective eigenmodes determined by linearly superposing these modes to yield the model convective flux profile. The numerical results are compared with the observed spectrum of solar convection and the technique is applied to other stars.
7 schema:editor N6488db26eda24e50b482533d772f0855
8 schema:genre chapter
9 schema:inLanguage en
10 schema:isAccessibleForFree false
11 schema:isPartOf N5d4a335ac1c84116b6183b5f7cb06098
12 schema:keywords amplitude
13 convection
14 convective eigenmodes
15 convective flux profile
16 eigenmodes
17 field
18 flux profiles
19 flux variations
20 mode
21 model convective flux profile
22 numerical results
23 observed spectra
24 power spectrum
25 profile
26 results
27 solar convection
28 solar velocity field
29 spectra
30 stars
31 technique
32 theoretical power spectrum
33 theoretical spectra
34 unstable convective eigenmodes
35 variation
36 velocity field
37 schema:name Theoretical spectrum of solar convection
38 schema:pagination 157-162
39 schema:productId N5cbc865b70d440e992fb60bea1c5fb22
40 Ncaca54c8ceb64f03be8eb0e6bf512d6b
41 schema:publisher N8eeed54bb5334feca06887ac84271768
42 schema:sameAs https://app.dimensions.ai/details/publication/pub.1047882289
43 https://doi.org/10.1007/3-540-54420-8_62
44 schema:sdDatePublished 2021-12-01T20:12
45 schema:sdLicense https://scigraph.springernature.com/explorer/license/
46 schema:sdPublisher N45a2b59d9fbc41fbb5ea0b814364c0e3
47 schema:url https://doi.org/10.1007/3-540-54420-8_62
48 sgo:license sg:explorer/license/
49 sgo:sdDataset chapters
50 rdf:type schema:Chapter
51 N046d9837636e46f9852ffe1d9ecce126 rdf:first sg:person.015153633273.13
52 rdf:rest rdf:nil
53 N2e248d3d71d74e07bf1487b18b7bf974 schema:familyName Gough
54 schema:givenName Douglas
55 rdf:type schema:Person
56 N45a2b59d9fbc41fbb5ea0b814364c0e3 schema:name Springer Nature - SN SciGraph project
57 rdf:type schema:Organization
58 N5cbc865b70d440e992fb60bea1c5fb22 schema:name doi
59 schema:value 10.1007/3-540-54420-8_62
60 rdf:type schema:PropertyValue
61 N5d4a335ac1c84116b6183b5f7cb06098 schema:isbn 978-3-540-38355-0
62 978-3-540-54420-3
63 schema:name Challenges to Theories of the Structure of Moderate-Mass Stars
64 rdf:type schema:Book
65 N6488db26eda24e50b482533d772f0855 rdf:first N2e248d3d71d74e07bf1487b18b7bf974
66 rdf:rest N8a3bcc415300470bbdde248c9995de8b
67 N8a3bcc415300470bbdde248c9995de8b rdf:first N95d295755dd4467ab87d8332826c390f
68 rdf:rest rdf:nil
69 N8eeed54bb5334feca06887ac84271768 schema:name Springer Nature
70 rdf:type schema:Organisation
71 N95d295755dd4467ab87d8332826c390f schema:familyName Toomre
72 schema:givenName Juri
73 rdf:type schema:Person
74 Nb6b8284f5f01498e880f600f94f724cf rdf:first sg:person.011311320105.13
75 rdf:rest N046d9837636e46f9852ffe1d9ecce126
76 Ncaca54c8ceb64f03be8eb0e6bf512d6b schema:name dimensions_id
77 schema:value pub.1047882289
78 rdf:type schema:PropertyValue
79 anzsrc-for:09 schema:inDefinedTermSet anzsrc-for:
80 schema:name Engineering
81 rdf:type schema:DefinedTerm
82 anzsrc-for:0915 schema:inDefinedTermSet anzsrc-for:
83 schema:name Interdisciplinary Engineering
84 rdf:type schema:DefinedTerm
85 sg:person.011311320105.13 schema:affiliation grid-institutes:grid.22401.35
86 schema:familyName Antia
87 schema:givenName H. M.
88 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.011311320105.13
89 rdf:type schema:Person
90 sg:person.015153633273.13 schema:affiliation grid-institutes:grid.22401.35
91 schema:familyName Chitre
92 schema:givenName S. M.
93 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.015153633273.13
94 rdf:type schema:Person
95 grid-institutes:grid.22401.35 schema:alternateName Tata Institute of Fundamental Research, Homi Bhabha Road, 400 005, Colaba, Bombay, India
96 schema:name Tata Institute of Fundamental Research, Homi Bhabha Road, 400 005, Colaba, Bombay, India
97 rdf:type schema:Organization
 




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


...