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You searched for subject:(dynamo theory). Showing records 1 – 17 of 17 total matches.

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University of Rochester

1. Park, Kiwan. Theory and simulation of magnetohydrodynamic dynamos and Faraday rotation for plasmas of general composition.

Degree: PhD, 2013, University of Rochester

 Many astrophysical phenomena depend on the underlying dynamics of magnetic fields. The observations of accretion disks and their jets, stellar coronae, and the solar corona… (more)

Subjects/Keywords: Dynamo; Faraday Rotation; MHD; Simulation; Theory; Turbulence

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APA (6th Edition):

Park, K. (2013). Theory and simulation of magnetohydrodynamic dynamos and Faraday rotation for plasmas of general composition. (Doctoral Dissertation). University of Rochester. Retrieved from http://hdl.handle.net/1802/27870

Chicago Manual of Style (16th Edition):

Park, Kiwan. “Theory and simulation of magnetohydrodynamic dynamos and Faraday rotation for plasmas of general composition.” 2013. Doctoral Dissertation, University of Rochester. Accessed November 29, 2020. http://hdl.handle.net/1802/27870.

MLA Handbook (7th Edition):

Park, Kiwan. “Theory and simulation of magnetohydrodynamic dynamos and Faraday rotation for plasmas of general composition.” 2013. Web. 29 Nov 2020.

Vancouver:

Park K. Theory and simulation of magnetohydrodynamic dynamos and Faraday rotation for plasmas of general composition. [Internet] [Doctoral dissertation]. University of Rochester; 2013. [cited 2020 Nov 29]. Available from: http://hdl.handle.net/1802/27870.

Council of Science Editors:

Park K. Theory and simulation of magnetohydrodynamic dynamos and Faraday rotation for plasmas of general composition. [Doctoral Dissertation]. University of Rochester; 2013. Available from: http://hdl.handle.net/1802/27870


University of Colorado

2. Featherstone, Nicholas Andrew. Exploring Convection and Dynamos in the Cores and Envelopes of Stars.

Degree: PhD, Astrophysical & Planetary Sciences, 2011, University of Colorado

  We present theoretical studies in two complementary areas dealing with convection, rotation, and dynamos in A-type stars, and with local helioseismology in the Sun.… (more)

Subjects/Keywords: Convection; Dynamo Theory; Helioseismology; Astrophysics and Astronomy

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APA (6th Edition):

Featherstone, N. A. (2011). Exploring Convection and Dynamos in the Cores and Envelopes of Stars. (Doctoral Dissertation). University of Colorado. Retrieved from https://scholar.colorado.edu/astr_gradetds/5

Chicago Manual of Style (16th Edition):

Featherstone, Nicholas Andrew. “Exploring Convection and Dynamos in the Cores and Envelopes of Stars.” 2011. Doctoral Dissertation, University of Colorado. Accessed November 29, 2020. https://scholar.colorado.edu/astr_gradetds/5.

MLA Handbook (7th Edition):

Featherstone, Nicholas Andrew. “Exploring Convection and Dynamos in the Cores and Envelopes of Stars.” 2011. Web. 29 Nov 2020.

Vancouver:

Featherstone NA. Exploring Convection and Dynamos in the Cores and Envelopes of Stars. [Internet] [Doctoral dissertation]. University of Colorado; 2011. [cited 2020 Nov 29]. Available from: https://scholar.colorado.edu/astr_gradetds/5.

Council of Science Editors:

Featherstone NA. Exploring Convection and Dynamos in the Cores and Envelopes of Stars. [Doctoral Dissertation]. University of Colorado; 2011. Available from: https://scholar.colorado.edu/astr_gradetds/5


University of Cambridge

3. Valeria Shumaylova, Valeria. Scale selection in hydromagnetic dynamos.

Degree: PhD, 2019, University of Cambridge

 One of the extraordinary properties of the Sun is the observed range of motion scales from the convection granules to the cyclic variation of magnetic… (more)

Subjects/Keywords: Dynamo theory; MHD; ABC flow; Mean-field theory

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APA (6th Edition):

Valeria Shumaylova, V. (2019). Scale selection in hydromagnetic dynamos. (Doctoral Dissertation). University of Cambridge. Retrieved from https://www.repository.cam.ac.uk/handle/1810/290138

Chicago Manual of Style (16th Edition):

Valeria Shumaylova, Valeria. “Scale selection in hydromagnetic dynamos.” 2019. Doctoral Dissertation, University of Cambridge. Accessed November 29, 2020. https://www.repository.cam.ac.uk/handle/1810/290138.

MLA Handbook (7th Edition):

Valeria Shumaylova, Valeria. “Scale selection in hydromagnetic dynamos.” 2019. Web. 29 Nov 2020.

Vancouver:

Valeria Shumaylova V. Scale selection in hydromagnetic dynamos. [Internet] [Doctoral dissertation]. University of Cambridge; 2019. [cited 2020 Nov 29]. Available from: https://www.repository.cam.ac.uk/handle/1810/290138.

Council of Science Editors:

Valeria Shumaylova V. Scale selection in hydromagnetic dynamos. [Doctoral Dissertation]. University of Cambridge; 2019. Available from: https://www.repository.cam.ac.uk/handle/1810/290138


University of Cambridge

4. Valeria Shumaylova, Valeria. Scale selection in hydromagnetic dynamos.

Degree: PhD, 2019, University of Cambridge

 One of the extraordinary properties of the Sun is the observed range of motion scales from the convection granules to the cyclic variation of magnetic… (more)

Subjects/Keywords: Dynamo theory; MHD; ABC flow; Mean-field theory

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APA (6th Edition):

Valeria Shumaylova, V. (2019). Scale selection in hydromagnetic dynamos. (Doctoral Dissertation). University of Cambridge. Retrieved from https://doi.org/10.17863/CAM.37367 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.767874

Chicago Manual of Style (16th Edition):

Valeria Shumaylova, Valeria. “Scale selection in hydromagnetic dynamos.” 2019. Doctoral Dissertation, University of Cambridge. Accessed November 29, 2020. https://doi.org/10.17863/CAM.37367 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.767874.

MLA Handbook (7th Edition):

Valeria Shumaylova, Valeria. “Scale selection in hydromagnetic dynamos.” 2019. Web. 29 Nov 2020.

Vancouver:

Valeria Shumaylova V. Scale selection in hydromagnetic dynamos. [Internet] [Doctoral dissertation]. University of Cambridge; 2019. [cited 2020 Nov 29]. Available from: https://doi.org/10.17863/CAM.37367 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.767874.

Council of Science Editors:

Valeria Shumaylova V. Scale selection in hydromagnetic dynamos. [Doctoral Dissertation]. University of Cambridge; 2019. Available from: https://doi.org/10.17863/CAM.37367 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.767874


Indian Institute of Science

5. Hazra, Gopal. Understanding the Behavior of the Sun's Large Scale Magnetic Field and Its Relation with the Meridional Flow.

Degree: PhD, Faculty of Science, 2018, Indian Institute of Science

 Our Sun is a variable star. The magnetic fields in the Sun play an important role for the existence of a wide variety of phenomena… (more)

Subjects/Keywords: Solar Cycle; Sunspots; Solar Magnetic Field; Dynamo Theory; Flux Transport Dynamo Model; Meridional Circulation; Solar Polar Field; Flux Transport Solar Dynamo; Solar Cycles; Sun’s Polar Magnetic Field; Dynamo Model; 3D Babcock-Leighton Solar Dynamo Model; Astrophysics

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APA (6th Edition):

Hazra, G. (2018). Understanding the Behavior of the Sun's Large Scale Magnetic Field and Its Relation with the Meridional Flow. (Doctoral Dissertation). Indian Institute of Science. Retrieved from http://etd.iisc.ac.in/handle/2005/3791

Chicago Manual of Style (16th Edition):

Hazra, Gopal. “Understanding the Behavior of the Sun's Large Scale Magnetic Field and Its Relation with the Meridional Flow.” 2018. Doctoral Dissertation, Indian Institute of Science. Accessed November 29, 2020. http://etd.iisc.ac.in/handle/2005/3791.

MLA Handbook (7th Edition):

Hazra, Gopal. “Understanding the Behavior of the Sun's Large Scale Magnetic Field and Its Relation with the Meridional Flow.” 2018. Web. 29 Nov 2020.

Vancouver:

Hazra G. Understanding the Behavior of the Sun's Large Scale Magnetic Field and Its Relation with the Meridional Flow. [Internet] [Doctoral dissertation]. Indian Institute of Science; 2018. [cited 2020 Nov 29]. Available from: http://etd.iisc.ac.in/handle/2005/3791.

Council of Science Editors:

Hazra G. Understanding the Behavior of the Sun's Large Scale Magnetic Field and Its Relation with the Meridional Flow. [Doctoral Dissertation]. Indian Institute of Science; 2018. Available from: http://etd.iisc.ac.in/handle/2005/3791

6. Chen, Long. Optimization of Kinematic Dynamos Using Variational Methods.

Degree: 2018, ETH Zürich

 The Earth possesses a magnetic field that is generated by the fluid motion in a conducting outer core. This system that converts kinetic energy into… (more)

Subjects/Keywords: Dynamo theory; Variational methods; Kinematic dynamo; Optimization; info:eu-repo/classification/ddc/550; info:eu-repo/classification/ddc/530; Earth sciences; Physics

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APA (6th Edition):

Chen, L. (2018). Optimization of Kinematic Dynamos Using Variational Methods. (Doctoral Dissertation). ETH Zürich. Retrieved from http://hdl.handle.net/20.500.11850/227237

Chicago Manual of Style (16th Edition):

Chen, Long. “Optimization of Kinematic Dynamos Using Variational Methods.” 2018. Doctoral Dissertation, ETH Zürich. Accessed November 29, 2020. http://hdl.handle.net/20.500.11850/227237.

MLA Handbook (7th Edition):

Chen, Long. “Optimization of Kinematic Dynamos Using Variational Methods.” 2018. Web. 29 Nov 2020.

Vancouver:

Chen L. Optimization of Kinematic Dynamos Using Variational Methods. [Internet] [Doctoral dissertation]. ETH Zürich; 2018. [cited 2020 Nov 29]. Available from: http://hdl.handle.net/20.500.11850/227237.

Council of Science Editors:

Chen L. Optimization of Kinematic Dynamos Using Variational Methods. [Doctoral Dissertation]. ETH Zürich; 2018. Available from: http://hdl.handle.net/20.500.11850/227237


UCLA

7. Cheng, Jonathan. Characterizing convection in geophysical dynamo systems.

Degree: Geophysics & Space Physics, 2015, UCLA

 The Earth’s magnetic field is produced by a fluid dynamo in the molten iron outer core. This geodynamo is driven by fluid motions induced by… (more)

Subjects/Keywords: Geophysics; Core dynamics; Dynamo theory; Geophysical fluid dynamics; Rotating convection

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APA (6th Edition):

Cheng, J. (2015). Characterizing convection in geophysical dynamo systems. (Thesis). UCLA. Retrieved from http://www.escholarship.org/uc/item/69z5f5gz

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Cheng, Jonathan. “Characterizing convection in geophysical dynamo systems.” 2015. Thesis, UCLA. Accessed November 29, 2020. http://www.escholarship.org/uc/item/69z5f5gz.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Cheng, Jonathan. “Characterizing convection in geophysical dynamo systems.” 2015. Web. 29 Nov 2020.

Vancouver:

Cheng J. Characterizing convection in geophysical dynamo systems. [Internet] [Thesis]. UCLA; 2015. [cited 2020 Nov 29]. Available from: http://www.escholarship.org/uc/item/69z5f5gz.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Cheng J. Characterizing convection in geophysical dynamo systems. [Thesis]. UCLA; 2015. Available from: http://www.escholarship.org/uc/item/69z5f5gz

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

8. Eraso, Gustavo Andres Guerrero. Estudos numéricos do dínamo solar.

Degree: PhD, Astronomia, 2009, University of São Paulo

 O ciclo solar é um dos fenômenos magnéticos mais interessantes do Universo. Embora ele tinha sido descoberto há mais de 150 anos, até agora permanece… (more)

Subjects/Keywords: Ciclo solar; dynamo theory; MHD; MHD; solar cycle; teoría dínamo

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APA (6th Edition):

Eraso, G. A. G. (2009). Estudos numéricos do dínamo solar. (Doctoral Dissertation). University of São Paulo. Retrieved from http://www.teses.usp.br/teses/disponiveis/14/14131/tde-12082009-065953/ ;

Chicago Manual of Style (16th Edition):

Eraso, Gustavo Andres Guerrero. “Estudos numéricos do dínamo solar.” 2009. Doctoral Dissertation, University of São Paulo. Accessed November 29, 2020. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-12082009-065953/ ;.

MLA Handbook (7th Edition):

Eraso, Gustavo Andres Guerrero. “Estudos numéricos do dínamo solar.” 2009. Web. 29 Nov 2020.

Vancouver:

Eraso GAG. Estudos numéricos do dínamo solar. [Internet] [Doctoral dissertation]. University of São Paulo; 2009. [cited 2020 Nov 29]. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-12082009-065953/ ;.

Council of Science Editors:

Eraso GAG. Estudos numéricos do dínamo solar. [Doctoral Dissertation]. University of São Paulo; 2009. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-12082009-065953/ ;


McMaster University

9. Jackel, Benjamin. Magnetic Dynamos: How Do They Even Work?.

Degree: PhD, 2015, McMaster University

The origin of cosmic magnetic fields is a important area of astrophysics. The process by which they are created falls under the heading of dynamo(more)

Subjects/Keywords: Accretion Disk; Magnetic Dynamo; magnetohydrodynamics; Mean Field Theory

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APA (6th Edition):

Jackel, B. (2015). Magnetic Dynamos: How Do They Even Work?. (Doctoral Dissertation). McMaster University. Retrieved from http://hdl.handle.net/11375/18299

Chicago Manual of Style (16th Edition):

Jackel, Benjamin. “Magnetic Dynamos: How Do They Even Work?.” 2015. Doctoral Dissertation, McMaster University. Accessed November 29, 2020. http://hdl.handle.net/11375/18299.

MLA Handbook (7th Edition):

Jackel, Benjamin. “Magnetic Dynamos: How Do They Even Work?.” 2015. Web. 29 Nov 2020.

Vancouver:

Jackel B. Magnetic Dynamos: How Do They Even Work?. [Internet] [Doctoral dissertation]. McMaster University; 2015. [cited 2020 Nov 29]. Available from: http://hdl.handle.net/11375/18299.

Council of Science Editors:

Jackel B. Magnetic Dynamos: How Do They Even Work?. [Doctoral Dissertation]. McMaster University; 2015. Available from: http://hdl.handle.net/11375/18299


University of Cambridge

10. Donnelly, Cara. Shearing waves and the MRI dynamo in stratified accretion discs.

Degree: PhD, 2014, University of Cambridge

 Accretion discs efficiently transport angular momentum by a wide variety of as yet imperfectly understood mechanisms, with profound implications for the disc lifetime and planet… (more)

Subjects/Keywords: Protoplanetary disks; Angular momentum; Theory of Wave-motion; Shear flow; Dynamo theory (Cosmic physics)

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APA (6th Edition):

Donnelly, C. (2014). Shearing waves and the MRI dynamo in stratified accretion discs. (Doctoral Dissertation). University of Cambridge. Retrieved from https://www.repository.cam.ac.uk/handle/1810/246452https://www.repository.cam.ac.uk/bitstream/1810/246452/3/thesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/246452/4/thesis.pdf.jpg

Chicago Manual of Style (16th Edition):

Donnelly, Cara. “Shearing waves and the MRI dynamo in stratified accretion discs.” 2014. Doctoral Dissertation, University of Cambridge. Accessed November 29, 2020. https://www.repository.cam.ac.uk/handle/1810/246452https://www.repository.cam.ac.uk/bitstream/1810/246452/3/thesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/246452/4/thesis.pdf.jpg.

MLA Handbook (7th Edition):

Donnelly, Cara. “Shearing waves and the MRI dynamo in stratified accretion discs.” 2014. Web. 29 Nov 2020.

Vancouver:

Donnelly C. Shearing waves and the MRI dynamo in stratified accretion discs. [Internet] [Doctoral dissertation]. University of Cambridge; 2014. [cited 2020 Nov 29]. Available from: https://www.repository.cam.ac.uk/handle/1810/246452https://www.repository.cam.ac.uk/bitstream/1810/246452/3/thesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/246452/4/thesis.pdf.jpg.

Council of Science Editors:

Donnelly C. Shearing waves and the MRI dynamo in stratified accretion discs. [Doctoral Dissertation]. University of Cambridge; 2014. Available from: https://www.repository.cam.ac.uk/handle/1810/246452https://www.repository.cam.ac.uk/bitstream/1810/246452/3/thesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/246452/4/thesis.pdf.jpg


McMaster University

11. Cridland, Alex J. Direct Numerical Simulations of Magnetic Helicity Conserving Astrophysical Dynamos.

Degree: MSc, 2013, McMaster University

Here we present direct numerical simulations of a shearing box which models the MHD turbulence in astrophysical systems with cylindrical geometries. The purpose of… (more)

Subjects/Keywords: Astrophysics; Magnetohydrodynamics; MHD; dynamo theory; direct numerical simulation; Physical Processes; Physical Processes

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APA (6th Edition):

Cridland, A. J. (2013). Direct Numerical Simulations of Magnetic Helicity Conserving Astrophysical Dynamos. (Masters Thesis). McMaster University. Retrieved from http://hdl.handle.net/11375/13636

Chicago Manual of Style (16th Edition):

Cridland, Alex J. “Direct Numerical Simulations of Magnetic Helicity Conserving Astrophysical Dynamos.” 2013. Masters Thesis, McMaster University. Accessed November 29, 2020. http://hdl.handle.net/11375/13636.

MLA Handbook (7th Edition):

Cridland, Alex J. “Direct Numerical Simulations of Magnetic Helicity Conserving Astrophysical Dynamos.” 2013. Web. 29 Nov 2020.

Vancouver:

Cridland AJ. Direct Numerical Simulations of Magnetic Helicity Conserving Astrophysical Dynamos. [Internet] [Masters thesis]. McMaster University; 2013. [cited 2020 Nov 29]. Available from: http://hdl.handle.net/11375/13636.

Council of Science Editors:

Cridland AJ. Direct Numerical Simulations of Magnetic Helicity Conserving Astrophysical Dynamos. [Masters Thesis]. McMaster University; 2013. Available from: http://hdl.handle.net/11375/13636


University of Colorado

12. Augustson, Kyle C. Convection and Dynamo Action in Massive Stars.

Degree: PhD, Astrophysical & Planetary Sciences, 2013, University of Colorado

  Contact between numerical simulations and observations of stellar magnetism is sought, with an emphasis on those stars that are the most readily observed and… (more)

Subjects/Keywords: Dynamo Theory; Fluid Dynamics; Stellar Convection; Stellar Magnetism; Astrophysics and Astronomy; Physical Processes; Stars, Interstellar Medium and the Galaxy

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APA (6th Edition):

Augustson, K. C. (2013). Convection and Dynamo Action in Massive Stars. (Doctoral Dissertation). University of Colorado. Retrieved from https://scholar.colorado.edu/astr_gradetds/26

Chicago Manual of Style (16th Edition):

Augustson, Kyle C. “Convection and Dynamo Action in Massive Stars.” 2013. Doctoral Dissertation, University of Colorado. Accessed November 29, 2020. https://scholar.colorado.edu/astr_gradetds/26.

MLA Handbook (7th Edition):

Augustson, Kyle C. “Convection and Dynamo Action in Massive Stars.” 2013. Web. 29 Nov 2020.

Vancouver:

Augustson KC. Convection and Dynamo Action in Massive Stars. [Internet] [Doctoral dissertation]. University of Colorado; 2013. [cited 2020 Nov 29]. Available from: https://scholar.colorado.edu/astr_gradetds/26.

Council of Science Editors:

Augustson KC. Convection and Dynamo Action in Massive Stars. [Doctoral Dissertation]. University of Colorado; 2013. Available from: https://scholar.colorado.edu/astr_gradetds/26


University of Exeter

13. Zhan, Xiaoya. A study of convection and dynamo in rotating fluid systems.

Degree: PhD, 2010, University of Exeter

 Convection in a Boussinesq fluid confined by a annular channel fast rotating about a vertical axis and uniformly heated from below, is one of our… (more)

Subjects/Keywords: 620.106; convection; dynamo theory; spherical geometry; channel

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APA (6th Edition):

Zhan, X. (2010). A study of convection and dynamo in rotating fluid systems. (Doctoral Dissertation). University of Exeter. Retrieved from https://ore.exeter.ac.uk/repository/handle/10036/100074 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.517199

Chicago Manual of Style (16th Edition):

Zhan, Xiaoya. “A study of convection and dynamo in rotating fluid systems.” 2010. Doctoral Dissertation, University of Exeter. Accessed November 29, 2020. https://ore.exeter.ac.uk/repository/handle/10036/100074 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.517199.

MLA Handbook (7th Edition):

Zhan, Xiaoya. “A study of convection and dynamo in rotating fluid systems.” 2010. Web. 29 Nov 2020.

Vancouver:

Zhan X. A study of convection and dynamo in rotating fluid systems. [Internet] [Doctoral dissertation]. University of Exeter; 2010. [cited 2020 Nov 29]. Available from: https://ore.exeter.ac.uk/repository/handle/10036/100074 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.517199.

Council of Science Editors:

Zhan X. A study of convection and dynamo in rotating fluid systems. [Doctoral Dissertation]. University of Exeter; 2010. Available from: https://ore.exeter.ac.uk/repository/handle/10036/100074 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.517199


University of Arizona

14. BOYER, DARRYL WILLIAM. MAGNETOHYDRODYNAMIC DYNAMOS IN THE PRESENCE OF FOSSIL MAGNETIC FIELDS.

Degree: 1982, University of Arizona

 A fossil magnetic field embedded in the radiative core of the Sun has been thought possible for some time now. However, such a fossil magnetic… (more)

Subjects/Keywords: Solar magnetic fields.; Magnetohydrodynamics.; Dynamo theory (Cosmic physics); Astrophysics.

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APA (6th Edition):

BOYER, D. W. (1982). MAGNETOHYDRODYNAMIC DYNAMOS IN THE PRESENCE OF FOSSIL MAGNETIC FIELDS. (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/185249

Chicago Manual of Style (16th Edition):

BOYER, DARRYL WILLIAM. “MAGNETOHYDRODYNAMIC DYNAMOS IN THE PRESENCE OF FOSSIL MAGNETIC FIELDS. ” 1982. Doctoral Dissertation, University of Arizona. Accessed November 29, 2020. http://hdl.handle.net/10150/185249.

MLA Handbook (7th Edition):

BOYER, DARRYL WILLIAM. “MAGNETOHYDRODYNAMIC DYNAMOS IN THE PRESENCE OF FOSSIL MAGNETIC FIELDS. ” 1982. Web. 29 Nov 2020.

Vancouver:

BOYER DW. MAGNETOHYDRODYNAMIC DYNAMOS IN THE PRESENCE OF FOSSIL MAGNETIC FIELDS. [Internet] [Doctoral dissertation]. University of Arizona; 1982. [cited 2020 Nov 29]. Available from: http://hdl.handle.net/10150/185249.

Council of Science Editors:

BOYER DW. MAGNETOHYDRODYNAMIC DYNAMOS IN THE PRESENCE OF FOSSIL MAGNETIC FIELDS. [Doctoral Dissertation]. University of Arizona; 1982. Available from: http://hdl.handle.net/10150/185249


Indian Institute of Science

15. Chatterjee, Piyali. Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability.

Degree: PhD, Faculty of Science, 2010, Indian Institute of Science

 The Sun, by the virtue of its proximity to Earth, serves as an excellent astrophysical laboratory for testing our theoretical ideas. The Sun displays a… (more)

Subjects/Keywords: Solar Magnetic Field; Magnetism (Astrophysics); Helioseismology; Solar Dynamo Models; Solar Oscillations; Helicity; Solar Dynamo Theory; Stochastic Fluctuations; Mean Field Dynamo Model; Magnetic Flux Tube; Poloidal Field Accretion; Dynamo Model SURYA; Astrophysics

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APA (6th Edition):

Chatterjee, P. (2010). Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability. (Doctoral Dissertation). Indian Institute of Science. Retrieved from http://etd.iisc.ac.in/handle/2005/657

Chicago Manual of Style (16th Edition):

Chatterjee, Piyali. “Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability.” 2010. Doctoral Dissertation, Indian Institute of Science. Accessed November 29, 2020. http://etd.iisc.ac.in/handle/2005/657.

MLA Handbook (7th Edition):

Chatterjee, Piyali. “Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability.” 2010. Web. 29 Nov 2020.

Vancouver:

Chatterjee P. Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability. [Internet] [Doctoral dissertation]. Indian Institute of Science; 2010. [cited 2020 Nov 29]. Available from: http://etd.iisc.ac.in/handle/2005/657.

Council of Science Editors:

Chatterjee P. Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability. [Doctoral Dissertation]. Indian Institute of Science; 2010. Available from: http://etd.iisc.ac.in/handle/2005/657

16. Donnelly, Cara. Shearing waves and the MRI dynamo in stratified accretion discs.

Degree: PhD, 2014, University of Cambridge

 Accretion discs efficiently transport angular momentum by a wide variety of as yet imperfectly understood mechanisms, with profound implications for the disc lifetime and planet… (more)

Subjects/Keywords: 523.01; Protoplanetary disks; Angular momentum; Theory of Wave-motion; Shear flow; Dynamo theory (Cosmic physics)

…magnetic buoyancy 1.8.2 Dynamo theory . . . . . . . . . . 1.9 Thesis outline… …nothing which is the outcome of work done in collaboration. Shearing Waves and the MRI Dynamo… …of the MRI have shown that the dynamo changes character on addition of vertical… …spatial and a novel temporal averaging to reveal the essential structure of the dynamo. We find… …azimuthal wavenumber, and that the critical Alfv´en speed below which the dynamo can operate… 

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Donnelly, C. (2014). Shearing waves and the MRI dynamo in stratified accretion discs. (Doctoral Dissertation). University of Cambridge. Retrieved from https://doi.org/10.17863/CAM.16134 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.633480

Chicago Manual of Style (16th Edition):

Donnelly, Cara. “Shearing waves and the MRI dynamo in stratified accretion discs.” 2014. Doctoral Dissertation, University of Cambridge. Accessed November 29, 2020. https://doi.org/10.17863/CAM.16134 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.633480.

MLA Handbook (7th Edition):

Donnelly, Cara. “Shearing waves and the MRI dynamo in stratified accretion discs.” 2014. Web. 29 Nov 2020.

Vancouver:

Donnelly C. Shearing waves and the MRI dynamo in stratified accretion discs. [Internet] [Doctoral dissertation]. University of Cambridge; 2014. [cited 2020 Nov 29]. Available from: https://doi.org/10.17863/CAM.16134 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.633480.

Council of Science Editors:

Donnelly C. Shearing waves and the MRI dynamo in stratified accretion discs. [Doctoral Dissertation]. University of Cambridge; 2014. Available from: https://doi.org/10.17863/CAM.16134 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.633480


University of St Andrews

17. Wilmot-Smith, Antonia. The origin and dynamic interaction of solar magnetic fields.

Degree: PhD, 2008, University of St Andrews

 The dynamics of the solar corona are dominated by the magnetic field which creates its structure. The magnetic field in most of the corona is… (more)

Subjects/Keywords: 520; MHD; Magnetic reconnection; QB539.M23W5; Solar magnetic fields; Sun – Corona – Magnetic fields – Mathematical models; Magnetic reconnection; Dynamo theory (Cosmic physics)

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Wilmot-Smith, A. (2008). The origin and dynamic interaction of solar magnetic fields. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/417

Chicago Manual of Style (16th Edition):

Wilmot-Smith, Antonia. “The origin and dynamic interaction of solar magnetic fields.” 2008. Doctoral Dissertation, University of St Andrews. Accessed November 29, 2020. http://hdl.handle.net/10023/417.

MLA Handbook (7th Edition):

Wilmot-Smith, Antonia. “The origin and dynamic interaction of solar magnetic fields.” 2008. Web. 29 Nov 2020.

Vancouver:

Wilmot-Smith A. The origin and dynamic interaction of solar magnetic fields. [Internet] [Doctoral dissertation]. University of St Andrews; 2008. [cited 2020 Nov 29]. Available from: http://hdl.handle.net/10023/417.

Council of Science Editors:

Wilmot-Smith A. The origin and dynamic interaction of solar magnetic fields. [Doctoral Dissertation]. University of St Andrews; 2008. Available from: http://hdl.handle.net/10023/417

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