Some Features of Interacting Solar Wind Disturbances.
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| Title: | Some Features of Interacting Solar Wind Disturbances. |
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| Authors: | Shlyk, N. S.1 (AUTHOR) nshlyk@izmiran.ru, Belov, A. V.1 (AUTHOR), Abunina, M. A.1 (AUTHOR), Belov, S. M.1 (AUTHOR), Abunin, A. A.1 (AUTHOR), Oleneva, V. A.1 (AUTHOR), Yanke, V. G.1 (AUTHOR) |
| Source: | Geomagnetism & Aeronomy. Aug2024, Vol. 64 Issue 4, p457-467. 11p. |
| Subject Terms: | *Interplanetary medium, *Galactic cosmic rays, *Coronal holes, *Coronal mass ejections, *Earth's orbit, *Solar wind |
| Abstract: | The updated database of Forbush effects and interplanetary disturbances (https://tools.izmiran.ru/feid) is used for an extensive analysis of various characteristics of events caused by the influence of interacting solar wind disturbances on the near-Earth space. In particular, the cases of different combinations of the pair interaction of high-speed streams from coronal holes and coronal mass ejections over the long period from 1995 to 2022 are considered. Variations in the flux of galactic cosmic rays (with a rigidity of 10 GV) and changes in the parameters of the interplanetary medium and geomagnetic activity are described. It is shown that the degree of mutual influence depends on the time between the detection of neighboring events; with the most pronounced changes in various parameters for events whose interaction occurred before reaching Earth's orbit. It is also established that in interacting solar wind disturbances not only the extremes of the parameters of cosmic rays, interplanetary medium, and geomagnetic activity but also their time profiles are subject to changes. [ABSTRACT FROM AUTHOR] |
| Database: | Energy & Power Source |
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| Header | DbId: enr DbLabel: Energy & Power Source An: 179041206 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| Items | – Name: Title Label: Title Group: Ti Data: Some Features of Interacting Solar Wind Disturbances. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Shlyk%2C+N%2E+S%2E%22">Shlyk, N. S.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> nshlyk@izmiran.ru</i><br /><searchLink fieldCode="AR" term="%22Belov%2C+A%2E+V%2E%22">Belov, A. V.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Abunina%2C+M%2E+A%2E%22">Abunina, M. A.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Belov%2C+S%2E+M%2E%22">Belov, S. M.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Abunin%2C+A%2E+A%2E%22">Abunin, A. A.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Oleneva%2C+V%2E+A%2E%22">Oleneva, V. A.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Yanke%2C+V%2E+G%2E%22">Yanke, V. G.</searchLink><relatesTo>1</relatesTo> (AUTHOR) – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Geomagnetism+%26+Aeronomy%22">Geomagnetism & Aeronomy</searchLink>. Aug2024, Vol. 64 Issue 4, p457-467. 11p. – Name: Subject Label: Subject Terms Group: Su Data: *<searchLink fieldCode="DE" term="%22Interplanetary+medium%22">Interplanetary medium</searchLink><br />*<searchLink fieldCode="DE" term="%22Galactic+cosmic+rays%22">Galactic cosmic rays</searchLink><br />*<searchLink fieldCode="DE" term="%22Coronal+holes%22">Coronal holes</searchLink><br />*<searchLink fieldCode="DE" term="%22Coronal+mass+ejections%22">Coronal mass ejections</searchLink><br />*<searchLink fieldCode="DE" term="%22Earth's+orbit%22">Earth's orbit</searchLink><br />*<searchLink fieldCode="DE" term="%22Solar+wind%22">Solar wind</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: The updated database of Forbush effects and interplanetary disturbances (https://tools.izmiran.ru/feid) is used for an extensive analysis of various characteristics of events caused by the influence of interacting solar wind disturbances on the near-Earth space. In particular, the cases of different combinations of the pair interaction of high-speed streams from coronal holes and coronal mass ejections over the long period from 1995 to 2022 are considered. Variations in the flux of galactic cosmic rays (with a rigidity of 10 GV) and changes in the parameters of the interplanetary medium and geomagnetic activity are described. It is shown that the degree of mutual influence depends on the time between the detection of neighboring events; with the most pronounced changes in various parameters for events whose interaction occurred before reaching Earth's orbit. It is also established that in interacting solar wind disturbances not only the extremes of the parameters of cosmic rays, interplanetary medium, and geomagnetic activity but also their time profiles are subject to changes. [ABSTRACT FROM AUTHOR] |
| PLink | https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=enr&AN=179041206 |
| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1134/S0016793224600280 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 11 StartPage: 457 Subjects: – SubjectFull: Interplanetary medium Type: general – SubjectFull: Galactic cosmic rays Type: general – SubjectFull: Coronal holes Type: general – SubjectFull: Coronal mass ejections Type: general – SubjectFull: Earth's orbit Type: general – SubjectFull: Solar wind Type: general Titles: – TitleFull: Some Features of Interacting Solar Wind Disturbances. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Shlyk, N. S. – PersonEntity: Name: NameFull: Belov, A. V. – PersonEntity: Name: NameFull: Abunina, M. A. – PersonEntity: Name: NameFull: Belov, S. M. – PersonEntity: Name: NameFull: Abunin, A. A. – PersonEntity: Name: NameFull: Oleneva, V. A. – PersonEntity: Name: NameFull: Yanke, V. G. IsPartOfRelationships: – BibEntity: Dates: – D: 01 M: 08 Text: Aug2024 Type: published Y: 2024 Identifiers: – Type: issn-print Value: 00167932 Numbering: – Type: volume Value: 64 – Type: issue Value: 4 Titles: – TitleFull: Geomagnetism & Aeronomy Type: main |
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