Systematic analysis of inertial wave patterns in spherical shell
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Systematic analysis of inertial wave patterns in spherical shell (2015)
DE PB NW RPISBN: 9783639844139 bzw. 3639844130, in Deutsch, AV Akademikerverlag Jun 2015, Taschenbuch, neu, Nachdruck.
Von Händler/Antiquariat, AHA-BUCH GmbH [51283250], Einbeck, Germany.
This item is printed on demand - Print on Demand Titel. Neuware - Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere's equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory. 76 pp. Englisch.
This item is printed on demand - Print on Demand Titel. Neuware - Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere's equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory. 76 pp. Englisch.
2
Systematic analysis of inertial wave patterns in spherical shell
DE PB NWISBN: 9783639844139 bzw. 3639844130, in Deutsch, Av Akademikerverlag, Taschenbuch, neu.
Lieferung aus: Deutschland, Versandkostenfrei.
buecher.de GmbH & Co. KG, [1].
Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere's equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory.2015. 76 S. 220 mmVersandfertig in 3-5 Tagen, Softcover.
buecher.de GmbH & Co. KG, [1].
Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere's equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory.2015. 76 S. 220 mmVersandfertig in 3-5 Tagen, Softcover.
3
Systematic analysis of inertial wave patterns in spherical shell
DE NWISBN: 9783639844139 bzw. 3639844130, in Deutsch, VDM Verlag Dr. Müller, Saarbrücken, Deutschland, neu.
Lieferung aus: Deutschland, zzgl. Versandkosten.
Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere's equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory.
Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere's equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory.
4
Systematic analysis of inertial wave patterns in spherical shell
~EN NW ABISBN: 9783639844139 bzw. 3639844130, vermutlich in Englisch, VDM Verlag Dr. Müller, Saarbrücken, Deutschland, neu, Hörbuch.
Lieferung aus: Deutschland, Lieferzeit: 5 Tage.
Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere's equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory.
Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere's equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory.
5
Systematic analysis of inertial wave patterns in spherical shell - Fluid Mechanics
~EN PB NWISBN: 9783639844139 bzw. 3639844130, vermutlich in Englisch, AV Akademikerverlag, Taschenbuch, neu.
Lieferung aus: Deutschland, Versandkostenfrei.
Systematic analysis of inertial wave patterns in spherical shell: Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere`s equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory. Englisch, Taschenbuch.
Systematic analysis of inertial wave patterns in spherical shell: Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere`s equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory. Englisch, Taschenbuch.
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Systematic analysis of inertial wave patterns in spherical shell (2015)
EN PB USISBN: 9783639844139 bzw. 3639844130, in Englisch, 76 Seiten, AV Akademikerverlag, Taschenbuch, gebraucht.
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Von Händler/Antiquariat, super_star_seller.
Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere's equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory. Paperback, Label: AV Akademikerverlag, AV Akademikerverlag, Produktgruppe: Book, Publiziert: 2015-05-26, Studio: AV Akademikerverlag.
Von Händler/Antiquariat, super_star_seller.
Inertial waves for an incompressible fluid inside a spherical shell are investigated. Inertial waves have an important role for the motion in the liquid outer core of the earth, the atmosphere and the oceans. Different inertial modes are excited as the modulation frequency is varied. The inertial waves propagating from inner sphere have inclined characteristics throughout the shell and are reflected back from the outer sphere. For larger forcing amplitudes and smaller libration frequencies, the inertial waves become unstable and can be stated as turbulent. The angle of propagation of waves with respect to axis of rotation is dependent on libration frequency. A layer is present at the tangent of inner sphere's equator and parallel to the axis of rotation called as Stewartson layer and its thickness and properties are dependent on libration frequency and amplitude. Zonal flow becomes unstable for larger amplitudes. Good agreement is found when the experimental results are compared with theory. Paperback, Label: AV Akademikerverlag, AV Akademikerverlag, Produktgruppe: Book, Publiziert: 2015-05-26, Studio: AV Akademikerverlag.
7
Systematic analysis of inertial wave patterns in spherical shell
~EN PB NWISBN: 3639844130 bzw. 9783639844139, vermutlich in Englisch, AV Akademikerverlag, Taschenbuch, neu.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
8
Systematic analysis of inertial wave patterns in spherical shell: Fluid Mechanics (2015)
EN PB NWISBN: 9783639844139 bzw. 3639844130, in Englisch, 76 Seiten, Av Akademikerverlag, Taschenbuch, neu.
Lieferung aus: Deutschland, Versandfertig in 6 - 10 Werktagen.
Von Händler/Antiquariat, aha Buch.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
Von Händler/Antiquariat, aha Buch.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen
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