Mathematical model of formation of Kordylewski cosmic dust clouds
Abstract The question of occurrence of cosmic dust clouds, which were found by Kordylewski in 1961 in the vicinity of libration point L5 of the Earth–Moon system, still causes debates and concern. We explain theoretically the phenomenon of the apparent vanishing and appearance of the Kordylewski cos...
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| Autor*in: |
Sal’nikova, T. V. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Schlagwörter: |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2015 |
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| Übergeordnetes Werk: |
Enthalten in: Doklady physics - Pleiades Publishing, 1998, 60(2015), 7 vom: Juli, Seite 323-326 |
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| Übergeordnetes Werk: |
volume:60 ; year:2015 ; number:7 ; month:07 ; pages:323-326 |
| Links: |
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| DOI / URN: |
10.1134/S1028335815070071 |
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OLC2040660712 |
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| 520 | |a Abstract The question of occurrence of cosmic dust clouds, which were found by Kordylewski in 1961 in the vicinity of libration point L5 of the Earth–Moon system, still causes debates and concern. We explain theoretically the phenomenon of the apparent vanishing and appearance of the Kordylewski cosmic dust clouds in the vicinity of triangular libration points L4 and L5 of the Earth–Moon system. The possibility of occurrence of two such clouds rotating around libration points L4 and two clouds rotating around point L5 is shown and optimal times for their observation from the Earth are determined. The investigation is performed based on analysis of a stable periodic motion in a planar restricted circular problem of three bodies, Earth–Moon—Particle, allowing for perturbations from the Sun under the assumption that the orbits of the Earth and Moon are circular and lie in one plane. | ||
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10.1134/S1028335815070071 doi (DE-627)OLC2040660712 (DE-He213)S1028335815070071-p DE-627 ger DE-627 rakwb eng 530 VZ Sal’nikova, T. V. verfasserin aut Mathematical model of formation of Kordylewski cosmic dust clouds 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2015 Abstract The question of occurrence of cosmic dust clouds, which were found by Kordylewski in 1961 in the vicinity of libration point L5 of the Earth–Moon system, still causes debates and concern. We explain theoretically the phenomenon of the apparent vanishing and appearance of the Kordylewski cosmic dust clouds in the vicinity of triangular libration points L4 and L5 of the Earth–Moon system. The possibility of occurrence of two such clouds rotating around libration points L4 and two clouds rotating around point L5 is shown and optimal times for their observation from the Earth are determined. The investigation is performed based on analysis of a stable periodic motion in a planar restricted circular problem of three bodies, Earth–Moon—Particle, allowing for perturbations from the Sun under the assumption that the orbits of the Earth and Moon are circular and lie in one plane. Periodic Solution Libration Point Dust Cloud Moon System Triangular Libration Point Stepanov, S. Ya. aut Enthalten in Doklady physics Pleiades Publishing, 1998 60(2015), 7 vom: Juli, Seite 323-326 (DE-627)241206545 (DE-600)1418838-7 (DE-576)064883841 1028-3358 nnns volume:60 year:2015 number:7 month:07 pages:323-326 https://doi.org/10.1134/S1028335815070071 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_70 AR 60 2015 7 07 323-326 |
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10.1134/S1028335815070071 doi (DE-627)OLC2040660712 (DE-He213)S1028335815070071-p DE-627 ger DE-627 rakwb eng 530 VZ Sal’nikova, T. V. verfasserin aut Mathematical model of formation of Kordylewski cosmic dust clouds 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2015 Abstract The question of occurrence of cosmic dust clouds, which were found by Kordylewski in 1961 in the vicinity of libration point L5 of the Earth–Moon system, still causes debates and concern. We explain theoretically the phenomenon of the apparent vanishing and appearance of the Kordylewski cosmic dust clouds in the vicinity of triangular libration points L4 and L5 of the Earth–Moon system. The possibility of occurrence of two such clouds rotating around libration points L4 and two clouds rotating around point L5 is shown and optimal times for their observation from the Earth are determined. The investigation is performed based on analysis of a stable periodic motion in a planar restricted circular problem of three bodies, Earth–Moon—Particle, allowing for perturbations from the Sun under the assumption that the orbits of the Earth and Moon are circular and lie in one plane. Periodic Solution Libration Point Dust Cloud Moon System Triangular Libration Point Stepanov, S. Ya. aut Enthalten in Doklady physics Pleiades Publishing, 1998 60(2015), 7 vom: Juli, Seite 323-326 (DE-627)241206545 (DE-600)1418838-7 (DE-576)064883841 1028-3358 nnns volume:60 year:2015 number:7 month:07 pages:323-326 https://doi.org/10.1134/S1028335815070071 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_70 AR 60 2015 7 07 323-326 |
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10.1134/S1028335815070071 doi (DE-627)OLC2040660712 (DE-He213)S1028335815070071-p DE-627 ger DE-627 rakwb eng 530 VZ Sal’nikova, T. V. verfasserin aut Mathematical model of formation of Kordylewski cosmic dust clouds 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2015 Abstract The question of occurrence of cosmic dust clouds, which were found by Kordylewski in 1961 in the vicinity of libration point L5 of the Earth–Moon system, still causes debates and concern. We explain theoretically the phenomenon of the apparent vanishing and appearance of the Kordylewski cosmic dust clouds in the vicinity of triangular libration points L4 and L5 of the Earth–Moon system. The possibility of occurrence of two such clouds rotating around libration points L4 and two clouds rotating around point L5 is shown and optimal times for their observation from the Earth are determined. The investigation is performed based on analysis of a stable periodic motion in a planar restricted circular problem of three bodies, Earth–Moon—Particle, allowing for perturbations from the Sun under the assumption that the orbits of the Earth and Moon are circular and lie in one plane. Periodic Solution Libration Point Dust Cloud Moon System Triangular Libration Point Stepanov, S. Ya. aut Enthalten in Doklady physics Pleiades Publishing, 1998 60(2015), 7 vom: Juli, Seite 323-326 (DE-627)241206545 (DE-600)1418838-7 (DE-576)064883841 1028-3358 nnns volume:60 year:2015 number:7 month:07 pages:323-326 https://doi.org/10.1134/S1028335815070071 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_70 AR 60 2015 7 07 323-326 |
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Abstract The question of occurrence of cosmic dust clouds, which were found by Kordylewski in 1961 in the vicinity of libration point L5 of the Earth–Moon system, still causes debates and concern. We explain theoretically the phenomenon of the apparent vanishing and appearance of the Kordylewski cosmic dust clouds in the vicinity of triangular libration points L4 and L5 of the Earth–Moon system. The possibility of occurrence of two such clouds rotating around libration points L4 and two clouds rotating around point L5 is shown and optimal times for their observation from the Earth are determined. The investigation is performed based on analysis of a stable periodic motion in a planar restricted circular problem of three bodies, Earth–Moon—Particle, allowing for perturbations from the Sun under the assumption that the orbits of the Earth and Moon are circular and lie in one plane. © Pleiades Publishing, Ltd. 2015 |
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Abstract The question of occurrence of cosmic dust clouds, which were found by Kordylewski in 1961 in the vicinity of libration point L5 of the Earth–Moon system, still causes debates and concern. We explain theoretically the phenomenon of the apparent vanishing and appearance of the Kordylewski cosmic dust clouds in the vicinity of triangular libration points L4 and L5 of the Earth–Moon system. The possibility of occurrence of two such clouds rotating around libration points L4 and two clouds rotating around point L5 is shown and optimal times for their observation from the Earth are determined. The investigation is performed based on analysis of a stable periodic motion in a planar restricted circular problem of three bodies, Earth–Moon—Particle, allowing for perturbations from the Sun under the assumption that the orbits of the Earth and Moon are circular and lie in one plane. © Pleiades Publishing, Ltd. 2015 |
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Abstract The question of occurrence of cosmic dust clouds, which were found by Kordylewski in 1961 in the vicinity of libration point L5 of the Earth–Moon system, still causes debates and concern. We explain theoretically the phenomenon of the apparent vanishing and appearance of the Kordylewski cosmic dust clouds in the vicinity of triangular libration points L4 and L5 of the Earth–Moon system. The possibility of occurrence of two such clouds rotating around libration points L4 and two clouds rotating around point L5 is shown and optimal times for their observation from the Earth are determined. The investigation is performed based on analysis of a stable periodic motion in a planar restricted circular problem of three bodies, Earth–Moon—Particle, allowing for perturbations from the Sun under the assumption that the orbits of the Earth and Moon are circular and lie in one plane. © Pleiades Publishing, Ltd. 2015 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2040660712</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504103517.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2015 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1134/S1028335815070071</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2040660712</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)S1028335815070071-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Sal’nikova, T. V.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Mathematical model of formation of Kordylewski cosmic dust clouds</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2015</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Pleiades Publishing, Ltd. 2015</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The question of occurrence of cosmic dust clouds, which were found by Kordylewski in 1961 in the vicinity of libration point L5 of the Earth–Moon system, still causes debates and concern. We explain theoretically the phenomenon of the apparent vanishing and appearance of the Kordylewski cosmic dust clouds in the vicinity of triangular libration points L4 and L5 of the Earth–Moon system. The possibility of occurrence of two such clouds rotating around libration points L4 and two clouds rotating around point L5 is shown and optimal times for their observation from the Earth are determined. The investigation is performed based on analysis of a stable periodic motion in a planar restricted circular problem of three bodies, Earth–Moon—Particle, allowing for perturbations from the Sun under the assumption that the orbits of the Earth and Moon are circular and lie in one plane.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Periodic Solution</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Libration Point</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Dust Cloud</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Moon System</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Triangular Libration Point</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stepanov, S. Ya.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Doklady physics</subfield><subfield code="d">Pleiades Publishing, 1998</subfield><subfield code="g">60(2015), 7 vom: Juli, Seite 323-326</subfield><subfield code="w">(DE-627)241206545</subfield><subfield code="w">(DE-600)1418838-7</subfield><subfield code="w">(DE-576)064883841</subfield><subfield code="x">1028-3358</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:60</subfield><subfield code="g">year:2015</subfield><subfield code="g">number:7</subfield><subfield code="g">month:07</subfield><subfield code="g">pages:323-326</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1134/S1028335815070071</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">60</subfield><subfield code="j">2015</subfield><subfield code="e">7</subfield><subfield code="c">07</subfield><subfield code="h">323-326</subfield></datafield></record></collection>
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