Modelling of nonlinear ion-acoustic wave structures due to Martian ionospheric loss
Abstract The ion escape process of the ionosphere of an unmagnetized planet, Mars, gets highly stimulated by the interaction with the solar wind. A mathematical model is constructed to investigate the nonlinear dynamics of ionized particles by studying the propagation dynamics of ion-acoustic waves...
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| Autor*in: |
Kolay, Debaditya [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2023 |
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© The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Springer Netherlands, 1968, 368(2023), 1 vom: Jan. |
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| Übergeordnetes Werk: |
volume:368 ; year:2023 ; number:1 ; month:01 |
| Links: |
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| DOI / URN: |
10.1007/s10509-022-04161-3 |
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| 520 | |a Abstract The ion escape process of the ionosphere of an unmagnetized planet, Mars, gets highly stimulated by the interaction with the solar wind. A mathematical model is constructed to investigate the nonlinear dynamics of ionized particles by studying the propagation dynamics of ion-acoustic waves (IAWs) formed due to the interaction of Martian ionospheric plasma consisting of the positive ion beam ($O^{+}$) and negative ions ($Cl^{-}$) with the solar wind composed by $H^{+}$ ions and electrons. The Sagdeev Pseudopotential formalism is deployed to investigate the nonlinear properties of the ion-acoustic waves. Using the phase plane analysis, the unperturbed dynamical systems are examined for solitary as well as other nonlinear waves. The three-dimensional total energy functions are plotted to support the existence of nonlinear and super nonlinear wave structures and the existence region of the solitary waves is explored. A relevant set of plasma parameters for Martian ionospheric plasma is chosen to discuss the analytical solution of the energy equation by using the concept of the Jacobi elliptic function. The perturbed dynamical system is investigated to examine the existence of quasiperiodic and chaotic trajectories. The effects of different plasma parameters on nonlinear wave features are discussed. | ||
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10.1007/s10509-022-04161-3 doi (DE-627)OLC208027239X (DE-He213)s10509-022-04161-3-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Kolay, Debaditya verfasserin aut Modelling of nonlinear ion-acoustic wave structures due to Martian ionospheric loss 2023 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract The ion escape process of the ionosphere of an unmagnetized planet, Mars, gets highly stimulated by the interaction with the solar wind. A mathematical model is constructed to investigate the nonlinear dynamics of ionized particles by studying the propagation dynamics of ion-acoustic waves (IAWs) formed due to the interaction of Martian ionospheric plasma consisting of the positive ion beam ($O^{+}$) and negative ions ($Cl^{-}$) with the solar wind composed by $H^{+}$ ions and electrons. The Sagdeev Pseudopotential formalism is deployed to investigate the nonlinear properties of the ion-acoustic waves. Using the phase plane analysis, the unperturbed dynamical systems are examined for solitary as well as other nonlinear waves. The three-dimensional total energy functions are plotted to support the existence of nonlinear and super nonlinear wave structures and the existence region of the solitary waves is explored. A relevant set of plasma parameters for Martian ionospheric plasma is chosen to discuss the analytical solution of the energy equation by using the concept of the Jacobi elliptic function. The perturbed dynamical system is investigated to examine the existence of quasiperiodic and chaotic trajectories. The effects of different plasma parameters on nonlinear wave features are discussed. Sagdeev pseudopotential Total energy function Superperiodic wave Phase portrait Chaos Dutta, Debjit aut Saha, Asit aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 368(2023), 1 vom: Jan. (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:368 year:2023 number:1 month:01 https://doi.org/10.1007/s10509-022-04161-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_2279 AR 368 2023 1 01 |
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10.1007/s10509-022-04161-3 doi (DE-627)OLC208027239X (DE-He213)s10509-022-04161-3-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Kolay, Debaditya verfasserin aut Modelling of nonlinear ion-acoustic wave structures due to Martian ionospheric loss 2023 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract The ion escape process of the ionosphere of an unmagnetized planet, Mars, gets highly stimulated by the interaction with the solar wind. A mathematical model is constructed to investigate the nonlinear dynamics of ionized particles by studying the propagation dynamics of ion-acoustic waves (IAWs) formed due to the interaction of Martian ionospheric plasma consisting of the positive ion beam ($O^{+}$) and negative ions ($Cl^{-}$) with the solar wind composed by $H^{+}$ ions and electrons. The Sagdeev Pseudopotential formalism is deployed to investigate the nonlinear properties of the ion-acoustic waves. Using the phase plane analysis, the unperturbed dynamical systems are examined for solitary as well as other nonlinear waves. The three-dimensional total energy functions are plotted to support the existence of nonlinear and super nonlinear wave structures and the existence region of the solitary waves is explored. A relevant set of plasma parameters for Martian ionospheric plasma is chosen to discuss the analytical solution of the energy equation by using the concept of the Jacobi elliptic function. The perturbed dynamical system is investigated to examine the existence of quasiperiodic and chaotic trajectories. The effects of different plasma parameters on nonlinear wave features are discussed. Sagdeev pseudopotential Total energy function Superperiodic wave Phase portrait Chaos Dutta, Debjit aut Saha, Asit aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 368(2023), 1 vom: Jan. (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:368 year:2023 number:1 month:01 https://doi.org/10.1007/s10509-022-04161-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_2279 AR 368 2023 1 01 |
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10.1007/s10509-022-04161-3 doi (DE-627)OLC208027239X (DE-He213)s10509-022-04161-3-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Kolay, Debaditya verfasserin aut Modelling of nonlinear ion-acoustic wave structures due to Martian ionospheric loss 2023 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract The ion escape process of the ionosphere of an unmagnetized planet, Mars, gets highly stimulated by the interaction with the solar wind. A mathematical model is constructed to investigate the nonlinear dynamics of ionized particles by studying the propagation dynamics of ion-acoustic waves (IAWs) formed due to the interaction of Martian ionospheric plasma consisting of the positive ion beam ($O^{+}$) and negative ions ($Cl^{-}$) with the solar wind composed by $H^{+}$ ions and electrons. The Sagdeev Pseudopotential formalism is deployed to investigate the nonlinear properties of the ion-acoustic waves. Using the phase plane analysis, the unperturbed dynamical systems are examined for solitary as well as other nonlinear waves. The three-dimensional total energy functions are plotted to support the existence of nonlinear and super nonlinear wave structures and the existence region of the solitary waves is explored. A relevant set of plasma parameters for Martian ionospheric plasma is chosen to discuss the analytical solution of the energy equation by using the concept of the Jacobi elliptic function. The perturbed dynamical system is investigated to examine the existence of quasiperiodic and chaotic trajectories. The effects of different plasma parameters on nonlinear wave features are discussed. Sagdeev pseudopotential Total energy function Superperiodic wave Phase portrait Chaos Dutta, Debjit aut Saha, Asit aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 368(2023), 1 vom: Jan. (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:368 year:2023 number:1 month:01 https://doi.org/10.1007/s10509-022-04161-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_2279 AR 368 2023 1 01 |
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10.1007/s10509-022-04161-3 doi (DE-627)OLC208027239X (DE-He213)s10509-022-04161-3-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Kolay, Debaditya verfasserin aut Modelling of nonlinear ion-acoustic wave structures due to Martian ionospheric loss 2023 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract The ion escape process of the ionosphere of an unmagnetized planet, Mars, gets highly stimulated by the interaction with the solar wind. A mathematical model is constructed to investigate the nonlinear dynamics of ionized particles by studying the propagation dynamics of ion-acoustic waves (IAWs) formed due to the interaction of Martian ionospheric plasma consisting of the positive ion beam ($O^{+}$) and negative ions ($Cl^{-}$) with the solar wind composed by $H^{+}$ ions and electrons. The Sagdeev Pseudopotential formalism is deployed to investigate the nonlinear properties of the ion-acoustic waves. Using the phase plane analysis, the unperturbed dynamical systems are examined for solitary as well as other nonlinear waves. The three-dimensional total energy functions are plotted to support the existence of nonlinear and super nonlinear wave structures and the existence region of the solitary waves is explored. A relevant set of plasma parameters for Martian ionospheric plasma is chosen to discuss the analytical solution of the energy equation by using the concept of the Jacobi elliptic function. The perturbed dynamical system is investigated to examine the existence of quasiperiodic and chaotic trajectories. The effects of different plasma parameters on nonlinear wave features are discussed. Sagdeev pseudopotential Total energy function Superperiodic wave Phase portrait Chaos Dutta, Debjit aut Saha, Asit aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 368(2023), 1 vom: Jan. (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:368 year:2023 number:1 month:01 https://doi.org/10.1007/s10509-022-04161-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_2279 AR 368 2023 1 01 |
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10.1007/s10509-022-04161-3 doi (DE-627)OLC208027239X (DE-He213)s10509-022-04161-3-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Kolay, Debaditya verfasserin aut Modelling of nonlinear ion-acoustic wave structures due to Martian ionospheric loss 2023 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract The ion escape process of the ionosphere of an unmagnetized planet, Mars, gets highly stimulated by the interaction with the solar wind. A mathematical model is constructed to investigate the nonlinear dynamics of ionized particles by studying the propagation dynamics of ion-acoustic waves (IAWs) formed due to the interaction of Martian ionospheric plasma consisting of the positive ion beam ($O^{+}$) and negative ions ($Cl^{-}$) with the solar wind composed by $H^{+}$ ions and electrons. The Sagdeev Pseudopotential formalism is deployed to investigate the nonlinear properties of the ion-acoustic waves. Using the phase plane analysis, the unperturbed dynamical systems are examined for solitary as well as other nonlinear waves. The three-dimensional total energy functions are plotted to support the existence of nonlinear and super nonlinear wave structures and the existence region of the solitary waves is explored. A relevant set of plasma parameters for Martian ionospheric plasma is chosen to discuss the analytical solution of the energy equation by using the concept of the Jacobi elliptic function. The perturbed dynamical system is investigated to examine the existence of quasiperiodic and chaotic trajectories. The effects of different plasma parameters on nonlinear wave features are discussed. Sagdeev pseudopotential Total energy function Superperiodic wave Phase portrait Chaos Dutta, Debjit aut Saha, Asit aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 368(2023), 1 vom: Jan. (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:368 year:2023 number:1 month:01 https://doi.org/10.1007/s10509-022-04161-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_2279 AR 368 2023 1 01 |
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Kolay, Debaditya Dutta, Debjit Saha, Asit |
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modelling of nonlinear ion-acoustic wave structures due to martian ionospheric loss |
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Modelling of nonlinear ion-acoustic wave structures due to Martian ionospheric loss |
| abstract |
Abstract The ion escape process of the ionosphere of an unmagnetized planet, Mars, gets highly stimulated by the interaction with the solar wind. A mathematical model is constructed to investigate the nonlinear dynamics of ionized particles by studying the propagation dynamics of ion-acoustic waves (IAWs) formed due to the interaction of Martian ionospheric plasma consisting of the positive ion beam ($O^{+}$) and negative ions ($Cl^{-}$) with the solar wind composed by $H^{+}$ ions and electrons. The Sagdeev Pseudopotential formalism is deployed to investigate the nonlinear properties of the ion-acoustic waves. Using the phase plane analysis, the unperturbed dynamical systems are examined for solitary as well as other nonlinear waves. The three-dimensional total energy functions are plotted to support the existence of nonlinear and super nonlinear wave structures and the existence region of the solitary waves is explored. A relevant set of plasma parameters for Martian ionospheric plasma is chosen to discuss the analytical solution of the energy equation by using the concept of the Jacobi elliptic function. The perturbed dynamical system is investigated to examine the existence of quasiperiodic and chaotic trajectories. The effects of different plasma parameters on nonlinear wave features are discussed. © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
| abstractGer |
Abstract The ion escape process of the ionosphere of an unmagnetized planet, Mars, gets highly stimulated by the interaction with the solar wind. A mathematical model is constructed to investigate the nonlinear dynamics of ionized particles by studying the propagation dynamics of ion-acoustic waves (IAWs) formed due to the interaction of Martian ionospheric plasma consisting of the positive ion beam ($O^{+}$) and negative ions ($Cl^{-}$) with the solar wind composed by $H^{+}$ ions and electrons. The Sagdeev Pseudopotential formalism is deployed to investigate the nonlinear properties of the ion-acoustic waves. Using the phase plane analysis, the unperturbed dynamical systems are examined for solitary as well as other nonlinear waves. The three-dimensional total energy functions are plotted to support the existence of nonlinear and super nonlinear wave structures and the existence region of the solitary waves is explored. A relevant set of plasma parameters for Martian ionospheric plasma is chosen to discuss the analytical solution of the energy equation by using the concept of the Jacobi elliptic function. The perturbed dynamical system is investigated to examine the existence of quasiperiodic and chaotic trajectories. The effects of different plasma parameters on nonlinear wave features are discussed. © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
| abstract_unstemmed |
Abstract The ion escape process of the ionosphere of an unmagnetized planet, Mars, gets highly stimulated by the interaction with the solar wind. A mathematical model is constructed to investigate the nonlinear dynamics of ionized particles by studying the propagation dynamics of ion-acoustic waves (IAWs) formed due to the interaction of Martian ionospheric plasma consisting of the positive ion beam ($O^{+}$) and negative ions ($Cl^{-}$) with the solar wind composed by $H^{+}$ ions and electrons. The Sagdeev Pseudopotential formalism is deployed to investigate the nonlinear properties of the ion-acoustic waves. Using the phase plane analysis, the unperturbed dynamical systems are examined for solitary as well as other nonlinear waves. The three-dimensional total energy functions are plotted to support the existence of nonlinear and super nonlinear wave structures and the existence region of the solitary waves is explored. A relevant set of plasma parameters for Martian ionospheric plasma is chosen to discuss the analytical solution of the energy equation by using the concept of the Jacobi elliptic function. The perturbed dynamical system is investigated to examine the existence of quasiperiodic and chaotic trajectories. The effects of different plasma parameters on nonlinear wave features are discussed. © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
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Modelling of nonlinear ion-acoustic wave structures due to Martian ionospheric loss |
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