Turbulence in the Solar Wind - 8 Angebote vergleichen
| Preise | Nov. 16 | März 19 | Sep. 19 |
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| Schnitt | € 30,59 | € 42,92 | € 36,08 |
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1
Turbulence in Solar Wind
EN EBISBN: 9783319434407 bzw. 3319434403, in Englisch, Vitalsource Technologies, Inc. E-Book.
Lieferung aus: Vereinigte Staaten von Amerika, Lagernd, zzgl. Versandkosten.
9783319434407,3319434403,turbulence,solar,wind,roberto,bruno, A digital copy of "Turbulence in Solar Wind" by Roberto Bruno and Vincenzo Carbone. Download is immediately available upon purchase! eBook, Format: VitalSource. Type: . Copying: Allowed, .2Â.36 selections may be copied every 2Â.365 days. Printable: Allowed, .2Â.36 prints for 2Â.365 days. Expires: No Expiration. Read Aloud?: Allowed. Sharing: Not Allowed. Software: Online: No additional software required Offline: VitalSource Bookshelf. Shipping to USA only!
9783319434407,3319434403,turbulence,solar,wind,roberto,bruno, A digital copy of "Turbulence in Solar Wind" by Roberto Bruno and Vincenzo Carbone. Download is immediately available upon purchase! eBook, Format: VitalSource. Type: . Copying: Allowed, .2Â.36 selections may be copied every 2Â.365 days. Printable: Allowed, .2Â.36 prints for 2Â.365 days. Expires: No Expiration. Read Aloud?: Allowed. Sharing: Not Allowed. Software: Online: No additional software required Offline: VitalSource Bookshelf. Shipping to USA only!
2
Turbulence in Solar Wind
EN EBISBN: 9783319434407 bzw. 3319434403, in Englisch, Vitalsource Technologies, Inc. E-Book.
Lieferung aus: Vereinigte Staaten von Amerika, Lagernd, zzgl. Versandkosten.
9783319434407,3319434403,turbulence,solar,wind,roberto,bruno, A digital copy of "Turbulence in Solar Wind" by Roberto Bruno and Vincenzo Carbone. Download is immediately available upon purchase! eBook, Format: VitalSource. Type: . Copying: Allowed, .2Â.36 selections may be copied every 2Â.365 days. Printable: Allowed, .2Â.36 prints for 2Â.365 days. Expires: No Expiration. Read Aloud?: Allowed. Sharing: Not Allowed. Software: Online: No additional software required Offline: VitalSource Bookshelf. Shipping to USA only!
9783319434407,3319434403,turbulence,solar,wind,roberto,bruno, A digital copy of "Turbulence in Solar Wind" by Roberto Bruno and Vincenzo Carbone. Download is immediately available upon purchase! eBook, Format: VitalSource. Type: . Copying: Allowed, .2Â.36 selections may be copied every 2Â.365 days. Printable: Allowed, .2Â.36 prints for 2Â.365 days. Expires: No Expiration. Read Aloud?: Allowed. Sharing: Not Allowed. Software: Online: No additional software required Offline: VitalSource Bookshelf. Shipping to USA only!
3
Turbulence in the Solar Wind (2016)
DE NW EBISBN: 9783319434407 bzw. 3319434403, in Deutsch, Springer, neu, E-Book.
Lieferung aus: Deutschland, Sofort per Download lieferbar.
Turbulence in the Solar Wind This book provides an overview of solar wind turbulence from both the theoretical and observational perspective. It argues that the interplanetary medium offers the best opportunity to directly study turbulent fluctuations in collisionless plasmas. In fact, during expansion, the solar wind evolves towards a state characterized by large-amplitude fluctuations in all observed parameters, which resembles, at least at large scales, the well-known hydrodynamic turbulence. This text starts with historical references to past observations and experiments on turbulent flows. It then introduces the Navier-Stokes equations for a magnetized plasma whose low-frequency turbulence evolution is described within the framework of the MHD approximation. It also considers the scaling of plasma and magnetic field fluctuations and the study of nonlinear energy cascades within the same framework. It reports observations of turbulence in the ecliptic and at high latitude, treating Alfvénic and compressive fluctuations separately in order to explain the transport of mass, momentum and energy during the expansion. Further, existing models are compared with direct observations in the heliosphere. The problem of self-similar and anomalous fluctuations in the solar wind is then addressed using tools provided by dynamical system theory and discussed on the basis of available models and observations. The book highlights observations of Yagloms law in solar wind turbulence, which is one of the most important findings in fully developed turbulence and directly related to the long-lasting and still unsolved problem of solar wind plasma heating. Lastly, it includes a short chapter dedicated to the kinetic range of fluctuations, which has recently been receiving more attention from the space plasma community, since this is inherently related to turbulent energy dissipation and consequent plasma heating. It particularly focuses on the nature and role of the fluctuations populating this frequency range, and discusses several model predictions and recent observational findings in this context. 07.10.2016, PDF.
Turbulence in the Solar Wind This book provides an overview of solar wind turbulence from both the theoretical and observational perspective. It argues that the interplanetary medium offers the best opportunity to directly study turbulent fluctuations in collisionless plasmas. In fact, during expansion, the solar wind evolves towards a state characterized by large-amplitude fluctuations in all observed parameters, which resembles, at least at large scales, the well-known hydrodynamic turbulence. This text starts with historical references to past observations and experiments on turbulent flows. It then introduces the Navier-Stokes equations for a magnetized plasma whose low-frequency turbulence evolution is described within the framework of the MHD approximation. It also considers the scaling of plasma and magnetic field fluctuations and the study of nonlinear energy cascades within the same framework. It reports observations of turbulence in the ecliptic and at high latitude, treating Alfvénic and compressive fluctuations separately in order to explain the transport of mass, momentum and energy during the expansion. Further, existing models are compared with direct observations in the heliosphere. The problem of self-similar and anomalous fluctuations in the solar wind is then addressed using tools provided by dynamical system theory and discussed on the basis of available models and observations. The book highlights observations of Yagloms law in solar wind turbulence, which is one of the most important findings in fully developed turbulence and directly related to the long-lasting and still unsolved problem of solar wind plasma heating. Lastly, it includes a short chapter dedicated to the kinetic range of fluctuations, which has recently been receiving more attention from the space plasma community, since this is inherently related to turbulent energy dissipation and consequent plasma heating. It particularly focuses on the nature and role of the fluctuations populating this frequency range, and discusses several model predictions and recent observational findings in this context. 07.10.2016, PDF.
4
Turbulence in the Solar Wind
DE NW EB DLISBN: 9783319434407 bzw. 3319434403, in Deutsch, Springer Shop, neu, E-Book, elektronischer Download.
Lieferung aus: Italien, Lagernd, zzgl. Versandkosten.
This book provides an overview of solar wind turbulence from both the theoretical and observational perspective. It argues that the interplanetary medium offers the best opportunity to directly study turbulent fluctuations in collisionless plasmas. In fact, during expansion, the solar wind evolves towards a state characterized by large-amplitude fluctuations in all observed parameters, which resembles, at least at large scales, the well-known hydrodynamic turbulence. This text starts with historical references to past observations and experiments on turbulent flows. It then introduces the Navier-Stokes equations for a magnetized plasma whose low-frequency turbulence evolution is described within the framework of the MHD approximation. It also considers the scaling of plasma and magnetic field fluctuations and the study of nonlinear energy cascades within the same framework. It reports observations of turbulence in the ecliptic and at high latitude, treating Alfvénic and compressive fluctuations separately in order to explain the transport of mass, momentum and energy during the expansion. Further, existing models are compared with direct observations in the heliosphere. The problem of self-similar and anomalous fluctuations in the solar wind is then addressed using tools provided by dynamical system theory and discussed on the basis of available models and observations. The book highlights observations of Yaglom’s law in solar wind turbulence, which is one of the most important findings in fully developed turbulence and directly related to the long-lasting and still unsolved problem of solar wind plasma heating. Lastly, it includes a short chapter dedicated to the kinetic range of fluctuations, which has recently been receiving more attention from the space plasma community, since this is inherently related to turbulent energy dissipation and consequent plasma heating. It particularly focuses on the nature and role of the fluctuations populating this frequency range, and discusses several model predictions and recent observational findings in this context. eBook.
This book provides an overview of solar wind turbulence from both the theoretical and observational perspective. It argues that the interplanetary medium offers the best opportunity to directly study turbulent fluctuations in collisionless plasmas. In fact, during expansion, the solar wind evolves towards a state characterized by large-amplitude fluctuations in all observed parameters, which resembles, at least at large scales, the well-known hydrodynamic turbulence. This text starts with historical references to past observations and experiments on turbulent flows. It then introduces the Navier-Stokes equations for a magnetized plasma whose low-frequency turbulence evolution is described within the framework of the MHD approximation. It also considers the scaling of plasma and magnetic field fluctuations and the study of nonlinear energy cascades within the same framework. It reports observations of turbulence in the ecliptic and at high latitude, treating Alfvénic and compressive fluctuations separately in order to explain the transport of mass, momentum and energy during the expansion. Further, existing models are compared with direct observations in the heliosphere. The problem of self-similar and anomalous fluctuations in the solar wind is then addressed using tools provided by dynamical system theory and discussed on the basis of available models and observations. The book highlights observations of Yaglom’s law in solar wind turbulence, which is one of the most important findings in fully developed turbulence and directly related to the long-lasting and still unsolved problem of solar wind plasma heating. Lastly, it includes a short chapter dedicated to the kinetic range of fluctuations, which has recently been receiving more attention from the space plasma community, since this is inherently related to turbulent energy dissipation and consequent plasma heating. It particularly focuses on the nature and role of the fluctuations populating this frequency range, and discusses several model predictions and recent observational findings in this context. eBook.
6
Turbulence in the Solar Wind
DE PB NWISBN: 9783319434407 bzw. 3319434403, in Deutsch, Springer International Publishing, Taschenbuch, neu.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
7
Turbulence in the Solar Wind (2016)
EN NW EB DLISBN: 9783319434407 bzw. 3319434403, in Englisch, Springer, Springer, Springer, neu, E-Book, elektronischer Download.
Lieferung aus: Frankreich, in-stock.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
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