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You searched for subject:(Sun Corona Magnetic fields Mathematical models). Showing records 1 – 30 of 60067 total matches.

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University of St Andrews

1. Johnston, Craig David. Modelling chromospheric evaporation in response to coronal heating.

Degree: PhD, 2018, University of St Andrews

 This thesis presents a new computationally efficient method for modelling the response of the solar corona to the release of energy. During impulsive heating events,… (more)

Subjects/Keywords: 523.7; Sun: corona; Sun: magnetic fields; Magnetohydrodynamics (MHD); Coronal heating; Chromospheric evaporation; QB529.J7; Sun – Corona – Mathematical models; Solar chromosphere

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APA (6th Edition):

Johnston, C. D. (2018). Modelling chromospheric evaporation in response to coronal heating. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/14630

Chicago Manual of Style (16th Edition):

Johnston, Craig David. “Modelling chromospheric evaporation in response to coronal heating.” 2018. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/14630.

MLA Handbook (7th Edition):

Johnston, Craig David. “Modelling chromospheric evaporation in response to coronal heating.” 2018. Web. 03 Dec 2020.

Vancouver:

Johnston CD. Modelling chromospheric evaporation in response to coronal heating. [Internet] [Doctoral dissertation]. University of St Andrews; 2018. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/14630.

Council of Science Editors:

Johnston CD. Modelling chromospheric evaporation in response to coronal heating. [Doctoral Dissertation]. University of St Andrews; 2018. Available from: http://hdl.handle.net/10023/14630

2. Williams, Benjamin Matthew. The dynamic topology of the solar corona : mapping the Sun's three dimensional magnetic skeleton.

Degree: PhD, 2018, University of St Andrews

 Observations of the surface of the Sun reveal multi-scaled, mixed magnetic features that carpet the entire solar surface. Not surprisingly, the global magnetic fields extrapolated… (more)

Subjects/Keywords: 523.7; Magnetic fields; Magnetic reconnection; Magnetic topology; Sun; Magnetohydrodynamics; Numerical methods; Magnetic null points; QB529.M23W55; Sun – Corona – Magnetic fields – Mathematical models; Solar magnetic fields

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APA (6th Edition):

Williams, B. M. (2018). The dynamic topology of the solar corona : mapping the Sun's three dimensional magnetic skeleton. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/14637

Chicago Manual of Style (16th Edition):

Williams, Benjamin Matthew. “The dynamic topology of the solar corona : mapping the Sun's three dimensional magnetic skeleton.” 2018. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/14637.

MLA Handbook (7th Edition):

Williams, Benjamin Matthew. “The dynamic topology of the solar corona : mapping the Sun's three dimensional magnetic skeleton.” 2018. Web. 03 Dec 2020.

Vancouver:

Williams BM. The dynamic topology of the solar corona : mapping the Sun's three dimensional magnetic skeleton. [Internet] [Doctoral dissertation]. University of St Andrews; 2018. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/14637.

Council of Science Editors:

Williams BM. The dynamic topology of the solar corona : mapping the Sun's three dimensional magnetic skeleton. [Doctoral Dissertation]. University of St Andrews; 2018. Available from: http://hdl.handle.net/10023/14637


University of St Andrews

3. Bocquet, Francois-Xavier. Investigations of current build up in topologically simple magnetic fields.

Degree: PhD, 2005, University of St Andrews

 The solar corona is a highly conductive plasma which is dominated by the coronal magnetic field. Observations show that important solar phenomena like flares or… (more)

Subjects/Keywords: 523.7; QB529.B7; Sun – Corona – Magnetic fields; Sun – Corona – Magnetic fields – Mathematical models

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APA (6th Edition):

Bocquet, F. (2005). Investigations of current build up in topologically simple magnetic fields. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/11291

Chicago Manual of Style (16th Edition):

Bocquet, Francois-Xavier. “Investigations of current build up in topologically simple magnetic fields.” 2005. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/11291.

MLA Handbook (7th Edition):

Bocquet, Francois-Xavier. “Investigations of current build up in topologically simple magnetic fields.” 2005. Web. 03 Dec 2020.

Vancouver:

Bocquet F. Investigations of current build up in topologically simple magnetic fields. [Internet] [Doctoral dissertation]. University of St Andrews; 2005. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/11291.

Council of Science Editors:

Bocquet F. Investigations of current build up in topologically simple magnetic fields. [Doctoral Dissertation]. University of St Andrews; 2005. Available from: http://hdl.handle.net/10023/11291


University of St Andrews

4. Carcedo, Laura. Theory and observations of the magnetic field in the solar corona.

Degree: PhD, 2005, University of St Andrews

 Although the solar corona is one of the most studied areas in solar physics, its activity, such as flares, prominence eruptions and CMEs, is far… (more)

Subjects/Keywords: 523.7; QB529.C2; Sun – Corona – Magnetic fields; Sun – Corona – Magnetic fields – Mathematical models

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APA (6th Edition):

Carcedo, L. (2005). Theory and observations of the magnetic field in the solar corona. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/12948

Chicago Manual of Style (16th Edition):

Carcedo, Laura. “Theory and observations of the magnetic field in the solar corona.” 2005. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/12948.

MLA Handbook (7th Edition):

Carcedo, Laura. “Theory and observations of the magnetic field in the solar corona.” 2005. Web. 03 Dec 2020.

Vancouver:

Carcedo L. Theory and observations of the magnetic field in the solar corona. [Internet] [Doctoral dissertation]. University of St Andrews; 2005. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/12948.

Council of Science Editors:

Carcedo L. Theory and observations of the magnetic field in the solar corona. [Doctoral Dissertation]. University of St Andrews; 2005. Available from: http://hdl.handle.net/10023/12948


University of St Andrews

5. O'Hara, Jennifer. Numerical simulations of footpoint driven coronal heating.

Degree: PhD, 2016, University of St Andrews

Magnetic field permeates the solar atmosphere and plays a crucial role in the dynamics, energetics and structures observed. In particular, magnetic flux tubes provide the… (more)

Subjects/Keywords: 523.7; Magnetohydrodynamics; Sun – Corona; Magnetic fields

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APA (6th Edition):

O'Hara, J. (2016). Numerical simulations of footpoint driven coronal heating. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/8871

Chicago Manual of Style (16th Edition):

O'Hara, Jennifer. “Numerical simulations of footpoint driven coronal heating.” 2016. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/8871.

MLA Handbook (7th Edition):

O'Hara, Jennifer. “Numerical simulations of footpoint driven coronal heating.” 2016. Web. 03 Dec 2020.

Vancouver:

O'Hara J. Numerical simulations of footpoint driven coronal heating. [Internet] [Doctoral dissertation]. University of St Andrews; 2016. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/8871.

Council of Science Editors:

O'Hara J. Numerical simulations of footpoint driven coronal heating. [Doctoral Dissertation]. University of St Andrews; 2016. Available from: http://hdl.handle.net/10023/8871


Montana State University

6. Tarr, Lucas Adrian. Energetic consequences of flux emergence.

Degree: PhD, College of Letters & Science, 2013, Montana State University

 When magnetic field in the solar convection zone buoyantly rises to pierce the visible solar surface (photosphere), the atmosphere (corona) above this surface must respond… (more)

Subjects/Keywords: Cosmic magnetic fields.; Solar energy.; Sun Corona.

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APA (6th Edition):

Tarr, L. A. (2013). Energetic consequences of flux emergence. (Doctoral Dissertation). Montana State University. Retrieved from https://scholarworks.montana.edu/xmlui/handle/1/2917

Chicago Manual of Style (16th Edition):

Tarr, Lucas Adrian. “Energetic consequences of flux emergence.” 2013. Doctoral Dissertation, Montana State University. Accessed December 03, 2020. https://scholarworks.montana.edu/xmlui/handle/1/2917.

MLA Handbook (7th Edition):

Tarr, Lucas Adrian. “Energetic consequences of flux emergence.” 2013. Web. 03 Dec 2020.

Vancouver:

Tarr LA. Energetic consequences of flux emergence. [Internet] [Doctoral dissertation]. Montana State University; 2013. [cited 2020 Dec 03]. Available from: https://scholarworks.montana.edu/xmlui/handle/1/2917.

Council of Science Editors:

Tarr LA. Energetic consequences of flux emergence. [Doctoral Dissertation]. Montana State University; 2013. Available from: https://scholarworks.montana.edu/xmlui/handle/1/2917


University of St Andrews

7. Fuentes Fernández, Jorge. MHD evolution of magnetic null points to static equilibria.

Degree: PhD, 2011, University of St Andrews

 In magnetised plasmas, magnetic reconnection is the process of magnetic field merging and recombination through which considerable amounts of magnetic energy may be converted into… (more)

Subjects/Keywords: 537; Sun; Magnetic fields; Reconnection; QB539.M23F8; Magnetic reconnection – Mathematical models; Solar magnetic fields – Mathematical models; Magnetohydrodynamics

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APA (6th Edition):

Fuentes Fernández, J. (2011). MHD evolution of magnetic null points to static equilibria. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/1897

Chicago Manual of Style (16th Edition):

Fuentes Fernández, Jorge. “MHD evolution of magnetic null points to static equilibria.” 2011. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/1897.

MLA Handbook (7th Edition):

Fuentes Fernández, Jorge. “MHD evolution of magnetic null points to static equilibria.” 2011. Web. 03 Dec 2020.

Vancouver:

Fuentes Fernández J. MHD evolution of magnetic null points to static equilibria. [Internet] [Doctoral dissertation]. University of St Andrews; 2011. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/1897.

Council of Science Editors:

Fuentes Fernández J. MHD evolution of magnetic null points to static equilibria. [Doctoral Dissertation]. University of St Andrews; 2011. Available from: http://hdl.handle.net/10023/1897


University of St Andrews

8. 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 (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 December 03, 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. 03 Dec 2020.

Vancouver:

Wilmot-Smith A. The origin and dynamic interaction of solar magnetic fields. [Internet] [Doctoral dissertation]. University of St Andrews; 2008. [cited 2020 Dec 03]. 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


University of St Andrews

9. Yeates, Anthony Robinson. Development and application of a global magnetic field evolution model for the solar corona.

Degree: PhD, 2009, University of St Andrews

Magnetic fields are fundamental to the structure and dynamics of the Sun’s corona. Observations show them to be locally complex, with highly sheared and twisted… (more)

Subjects/Keywords: 520; Sun; Magnetohydrodynamics; Solar filaments; Solar prominences; Coronal mass ejections; Magnetic field; QB529.Y4; Sun – Corona – Magnetic fields – Mathematical models

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APA (6th Edition):

Yeates, A. R. (2009). Development and application of a global magnetic field evolution model for the solar corona. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/734

Chicago Manual of Style (16th Edition):

Yeates, Anthony Robinson. “Development and application of a global magnetic field evolution model for the solar corona.” 2009. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/734.

MLA Handbook (7th Edition):

Yeates, Anthony Robinson. “Development and application of a global magnetic field evolution model for the solar corona.” 2009. Web. 03 Dec 2020.

Vancouver:

Yeates AR. Development and application of a global magnetic field evolution model for the solar corona. [Internet] [Doctoral dissertation]. University of St Andrews; 2009. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/734.

Council of Science Editors:

Yeates AR. Development and application of a global magnetic field evolution model for the solar corona. [Doctoral Dissertation]. University of St Andrews; 2009. Available from: http://hdl.handle.net/10023/734


University of St Andrews

10. Bowness, Ruth. Current sheets in the solar corona : formation, fragmentation and heating.

Degree: PhD, 2011, University of St Andrews

 In this thesis we investigate current sheets in the solar corona. The well known 1D model for the tearing mode instability is presented, before progressing… (more)

Subjects/Keywords: 520; MHD; Current sheets; Tearing mode instability; Magnetic reconnection; QB529.B78; Sun – Corona – Mathematical models; Magnetohydrodynamics; Magnetic reconnection

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APA (6th Edition):

Bowness, R. (2011). Current sheets in the solar corona : formation, fragmentation and heating. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/2081

Chicago Manual of Style (16th Edition):

Bowness, Ruth. “Current sheets in the solar corona : formation, fragmentation and heating.” 2011. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/2081.

MLA Handbook (7th Edition):

Bowness, Ruth. “Current sheets in the solar corona : formation, fragmentation and heating.” 2011. Web. 03 Dec 2020.

Vancouver:

Bowness R. Current sheets in the solar corona : formation, fragmentation and heating. [Internet] [Doctoral dissertation]. University of St Andrews; 2011. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/2081.

Council of Science Editors:

Bowness R. Current sheets in the solar corona : formation, fragmentation and heating. [Doctoral Dissertation]. University of St Andrews; 2011. Available from: http://hdl.handle.net/10023/2081


Boston University

11. Savcheva-Tasseva, Antonia Stefanova. The evolution of solar sigmoidal active regions.

Degree: PhD, Astronomy, 2013, Boston University

 The formation, evolution and eruption of solar active regions is a main theme in solar physics. Ultimately the goal is predicting when, where and how… (more)

Subjects/Keywords: Astronomy; Astrophysics; Magnetic fields; Corona; CME; Sigmoid; Sun; X-rays

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APA (6th Edition):

Savcheva-Tasseva, A. S. (2013). The evolution of solar sigmoidal active regions. (Doctoral Dissertation). Boston University. Retrieved from http://hdl.handle.net/2144/34334

Chicago Manual of Style (16th Edition):

Savcheva-Tasseva, Antonia Stefanova. “The evolution of solar sigmoidal active regions.” 2013. Doctoral Dissertation, Boston University. Accessed December 03, 2020. http://hdl.handle.net/2144/34334.

MLA Handbook (7th Edition):

Savcheva-Tasseva, Antonia Stefanova. “The evolution of solar sigmoidal active regions.” 2013. Web. 03 Dec 2020.

Vancouver:

Savcheva-Tasseva AS. The evolution of solar sigmoidal active regions. [Internet] [Doctoral dissertation]. Boston University; 2013. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/2144/34334.

Council of Science Editors:

Savcheva-Tasseva AS. The evolution of solar sigmoidal active regions. [Doctoral Dissertation]. Boston University; 2013. Available from: http://hdl.handle.net/2144/34334

12. Edwards, Sarah J. On the topology of global coronal magnetic fields.

Degree: PhD, 2014, University of St Andrews

 This thesis considers the magnetic topology of the global solar corona. To understand the magnetic topology we use the magnetic skeleton which provides us with… (more)

Subjects/Keywords: 523.7; Solar physics; Magnetic fields; Magnetic topology; QB539.M23E3; Sun – Corona – Mathematical fields; Sun – Corona – Mathematical fields – Mathematical fields

models Many models have been used to describe the global magnetic field of the Sun based on… …Structures in Global Magnetic Fields i… …chromosphere, transition region and corona. The solar atmosphere and 1 2 its magnetic field is the… …maximum the polarity of the dipole magnetic field of the Sun changes [e.g., Hathaway, 2010… …x5D;. For the Sun to go through a complete magnetic polarity change, and return to the… 

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APA (6th Edition):

Edwards, S. J. (2014). On the topology of global coronal magnetic fields. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/5896

Chicago Manual of Style (16th Edition):

Edwards, Sarah J. “On the topology of global coronal magnetic fields.” 2014. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/5896.

MLA Handbook (7th Edition):

Edwards, Sarah J. “On the topology of global coronal magnetic fields.” 2014. Web. 03 Dec 2020.

Vancouver:

Edwards SJ. On the topology of global coronal magnetic fields. [Internet] [Doctoral dissertation]. University of St Andrews; 2014. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/5896.

Council of Science Editors:

Edwards SJ. On the topology of global coronal magnetic fields. [Doctoral Dissertation]. University of St Andrews; 2014. Available from: http://hdl.handle.net/10023/5896


University of St Andrews

13. MacTaggart, David. Theoretical magnetic flux emergence.

Degree: PhD, 2011, University of St Andrews

Magnetic flux emergence is the subject of how magnetic fields from the solar interior can rise and expand into the atmosphere to produce active regions.… (more)

Subjects/Keywords: 520; Magnetohydrodynamics; Flux emergence; Numerical MHD; Magnetic eruptions; QB539.M23M82; Solar magnetic fields – Mathematical models; Magnetic flux; Magnetohydrodynamics; Sun – Active regions

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APA (6th Edition):

MacTaggart, D. (2011). Theoretical magnetic flux emergence. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/1692

Chicago Manual of Style (16th Edition):

MacTaggart, David. “Theoretical magnetic flux emergence.” 2011. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/1692.

MLA Handbook (7th Edition):

MacTaggart, David. “Theoretical magnetic flux emergence.” 2011. Web. 03 Dec 2020.

Vancouver:

MacTaggart D. Theoretical magnetic flux emergence. [Internet] [Doctoral dissertation]. University of St Andrews; 2011. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/1692.

Council of Science Editors:

MacTaggart D. Theoretical magnetic flux emergence. [Doctoral Dissertation]. University of St Andrews; 2011. Available from: http://hdl.handle.net/10023/1692


University of St Andrews

14. Macnamara, Cicely K. The period ratio P₁/2P₂ in coronal waves.

Degree: PhD, 2011, University of St Andrews

 Increasing observational evidence of wave modes brings us to a closer understanding of the solar corona. Coronal seismology allows us to combine wave observations and… (more)

Subjects/Keywords: 520; Solar physics; Solar waves; QB529.M62; Sun – Loop prominences – Mathematical models; Sun – Corona

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APA (6th Edition):

Macnamara, C. K. (2011). The period ratio P₁/2P₂ in coronal waves. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/2101

Chicago Manual of Style (16th Edition):

Macnamara, Cicely K. “The period ratio P₁/2P₂ in coronal waves.” 2011. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/2101.

MLA Handbook (7th Edition):

Macnamara, Cicely K. “The period ratio P₁/2P₂ in coronal waves.” 2011. Web. 03 Dec 2020.

Vancouver:

Macnamara CK. The period ratio P₁/2P₂ in coronal waves. [Internet] [Doctoral dissertation]. University of St Andrews; 2011. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/2101.

Council of Science Editors:

Macnamara CK. The period ratio P₁/2P₂ in coronal waves. [Doctoral Dissertation]. University of St Andrews; 2011. Available from: http://hdl.handle.net/10023/2101

15. Howson, Thomas Alexander. Three dimensional MHD simulations of the dynamics and energetics of coronal flux tubes.

Degree: PhD, 2019, University of St Andrews

 In this thesis we present the results of three-dimensional MHD simulations of the evolution of magnetic flux tubes within the solar atmosphere. We consider the… (more)

Subjects/Keywords: Magnetohydrodynamics (MHD); Coronal waves; Coronal heating; QB539.M23H7; Sun – Corona – Magnetic fields – Mathematical models; Magnetohydrodynamics – Mathematical models

…in regions of open magnetic field. Since the solar corona is highly inhomogeneous in nature… …energy that heats the corona is the Sun’s magnetic field (e.g. Klimchuk, 2006)… …2011; Pagano and De Moortel, 2017) or magnetic energy slowly accumulates in the corona… …and velocity fields and may lead to heating through magnetic reconnection (see Yamada… …things mathematical has been invaluable, particularly when my mind won’t stop thinking about my… 

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APA (6th Edition):

Howson, T. A. (2019). Three dimensional MHD simulations of the dynamics and energetics of coronal flux tubes. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/17512

Chicago Manual of Style (16th Edition):

Howson, Thomas Alexander. “Three dimensional MHD simulations of the dynamics and energetics of coronal flux tubes.” 2019. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/17512.

MLA Handbook (7th Edition):

Howson, Thomas Alexander. “Three dimensional MHD simulations of the dynamics and energetics of coronal flux tubes.” 2019. Web. 03 Dec 2020.

Vancouver:

Howson TA. Three dimensional MHD simulations of the dynamics and energetics of coronal flux tubes. [Internet] [Doctoral dissertation]. University of St Andrews; 2019. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/17512.

Council of Science Editors:

Howson TA. Three dimensional MHD simulations of the dynamics and energetics of coronal flux tubes. [Doctoral Dissertation]. University of St Andrews; 2019. Available from: http://hdl.handle.net/10023/17512


New Jersey Institute of Technology

16. Chen, Xin. Magnetic reconnection in small and large scales on the sun.

Degree: PhD, Physics, 2016, New Jersey Institute of Technology

  Almost all solar activities observed are related to the solar magnetic field, especially the topological restructuring of magnetic fields, the so-called magnetic reconnection in… (more)

Subjects/Keywords: Sun activity; Sun mafnetic fields; Sun chromosphere; Sun corona; Sunflares; Other Physics

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APA (6th Edition):

Chen, X. (2016). Magnetic reconnection in small and large scales on the sun. (Doctoral Dissertation). New Jersey Institute of Technology. Retrieved from https://digitalcommons.njit.edu/dissertations/66

Chicago Manual of Style (16th Edition):

Chen, Xin. “Magnetic reconnection in small and large scales on the sun.” 2016. Doctoral Dissertation, New Jersey Institute of Technology. Accessed December 03, 2020. https://digitalcommons.njit.edu/dissertations/66.

MLA Handbook (7th Edition):

Chen, Xin. “Magnetic reconnection in small and large scales on the sun.” 2016. Web. 03 Dec 2020.

Vancouver:

Chen X. Magnetic reconnection in small and large scales on the sun. [Internet] [Doctoral dissertation]. New Jersey Institute of Technology; 2016. [cited 2020 Dec 03]. Available from: https://digitalcommons.njit.edu/dissertations/66.

Council of Science Editors:

Chen X. Magnetic reconnection in small and large scales on the sun. [Doctoral Dissertation]. New Jersey Institute of Technology; 2016. Available from: https://digitalcommons.njit.edu/dissertations/66


University of St Andrews

17. Maclean, Rhona Claire. Topological structure of the magnetic solar corona.

Degree: PhD, 2007, University of St Andrews

 The solar corona is a highly complex and active plasma environment, containing many exotic phenomena such as solar flares, coronal mass ejections, prominences, coronal loops,… (more)

Subjects/Keywords: 520; Solar magnetic fields; Sun – Corona; QB529.M6

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APA (6th Edition):

Maclean, R. C. (2007). Topological structure of the magnetic solar corona. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/151

Chicago Manual of Style (16th Edition):

Maclean, Rhona Claire. “Topological structure of the magnetic solar corona.” 2007. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/151.

MLA Handbook (7th Edition):

Maclean, Rhona Claire. “Topological structure of the magnetic solar corona.” 2007. Web. 03 Dec 2020.

Vancouver:

Maclean RC. Topological structure of the magnetic solar corona. [Internet] [Doctoral dissertation]. University of St Andrews; 2007. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/151.

Council of Science Editors:

Maclean RC. Topological structure of the magnetic solar corona. [Doctoral Dissertation]. University of St Andrews; 2007. Available from: http://hdl.handle.net/10023/151


New Jersey Institute of Technology

18. Yang, Xu. Investigation of small-scale energy release and transfer processes in the solar atmosphere with high-resolution observations in infrared.

Degree: PhD, Physics, 2019, New Jersey Institute of Technology

  Solar spectrum in the infrared (IR) contains abundant information of solar activities, however, it has not spectral lines in the solar IR spectrum provide… (more)

Subjects/Keywords: Sun: chromosphere; Sun: corona; Sun: granulation; Sun: magnetic field; Sun: photosphere; Sun: sunspot; Astrophysics and Astronomy

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APA (6th Edition):

Yang, X. (2019). Investigation of small-scale energy release and transfer processes in the solar atmosphere with high-resolution observations in infrared. (Doctoral Dissertation). New Jersey Institute of Technology. Retrieved from https://digitalcommons.njit.edu/dissertations/1438

Chicago Manual of Style (16th Edition):

Yang, Xu. “Investigation of small-scale energy release and transfer processes in the solar atmosphere with high-resolution observations in infrared.” 2019. Doctoral Dissertation, New Jersey Institute of Technology. Accessed December 03, 2020. https://digitalcommons.njit.edu/dissertations/1438.

MLA Handbook (7th Edition):

Yang, Xu. “Investigation of small-scale energy release and transfer processes in the solar atmosphere with high-resolution observations in infrared.” 2019. Web. 03 Dec 2020.

Vancouver:

Yang X. Investigation of small-scale energy release and transfer processes in the solar atmosphere with high-resolution observations in infrared. [Internet] [Doctoral dissertation]. New Jersey Institute of Technology; 2019. [cited 2020 Dec 03]. Available from: https://digitalcommons.njit.edu/dissertations/1438.

Council of Science Editors:

Yang X. Investigation of small-scale energy release and transfer processes in the solar atmosphere with high-resolution observations in infrared. [Doctoral Dissertation]. New Jersey Institute of Technology; 2019. Available from: https://digitalcommons.njit.edu/dissertations/1438


University of St Andrews

19. Wood, Paul D. Elements of solar activity : particle acceleration and filament formation.

Degree: PhD, 2005, University of St Andrews

 This thesis studies the acceleration of particles to super-thermal energies in explosive solar events as well as the magnetic changes in connectivity that may be… (more)

Subjects/Keywords: 523.7; QB526.P7W7; Sun – Prominences; Solar magnetic fields – Mathematical models; Solar flares

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APA (6th Edition):

Wood, P. D. (2005). Elements of solar activity : particle acceleration and filament formation. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/11309

Chicago Manual of Style (16th Edition):

Wood, Paul D. “Elements of solar activity : particle acceleration and filament formation.” 2005. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/11309.

MLA Handbook (7th Edition):

Wood, Paul D. “Elements of solar activity : particle acceleration and filament formation.” 2005. Web. 03 Dec 2020.

Vancouver:

Wood PD. Elements of solar activity : particle acceleration and filament formation. [Internet] [Doctoral dissertation]. University of St Andrews; 2005. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/11309.

Council of Science Editors:

Wood PD. Elements of solar activity : particle acceleration and filament formation. [Doctoral Dissertation]. University of St Andrews; 2005. Available from: http://hdl.handle.net/10023/11309


University of St Andrews

20. McEwan, Michael P. Effect of structuring on coronal loop oscillations.

Degree: PhD, 2007, University of St Andrews

 In this Thesis the theoretical understanding of oscillations in coronal structures is developed. In particular, coronal loops are modelled as magnetic slabs of plasma. The… (more)

Subjects/Keywords: 530.44; Corona; Oscillations; Coronal seismology; Sun; QB529.M48; Sun – Corona; Sun – Loop prominences; Magnetohydrodynamic waves – Mathematical models; Oscillations – Mathematical models

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APA (6th Edition):

McEwan, M. P. (2007). Effect of structuring on coronal loop oscillations. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/265

Chicago Manual of Style (16th Edition):

McEwan, Michael P. “Effect of structuring on coronal loop oscillations.” 2007. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/265.

MLA Handbook (7th Edition):

McEwan, Michael P. “Effect of structuring on coronal loop oscillations.” 2007. Web. 03 Dec 2020.

Vancouver:

McEwan MP. Effect of structuring on coronal loop oscillations. [Internet] [Doctoral dissertation]. University of St Andrews; 2007. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/265.

Council of Science Editors:

McEwan MP. Effect of structuring on coronal loop oscillations. [Doctoral Dissertation]. University of St Andrews; 2007. Available from: http://hdl.handle.net/10023/265

21. Sturrock, Zoe. Numerical simulations of sunspot rotation driven by magnetic flux emergence.

Degree: PhD, 2017, University of St Andrews

Magnetic flux continually emerges from the Sun, rising through the solar interior, emerging at the photosphere in the form of sunspots and expanding into the… (more)

Subjects/Keywords: 523.7; Magnetohydrodynamics; Sun; Magnetic fields; QB525.S88; Sunspots – Mathematical models; Solar magnetic fields

…contributions of vertical flows that advect twisted magnetic fields up into the corona and by… …magnetic flux on the Sun. In this chapter, we provide any necessary background and a motivation… …Flux tubes are the building blocks of magnetic field on the Sun, and as such we consider… …magnetic flux tubes through layers of the Sun, namely magnetic buoyancy, is introduced in Section… …particles within the plasma can create electric and magnetic fields. In reality, a local charge… 

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APA (6th Edition):

Sturrock, Z. (2017). Numerical simulations of sunspot rotation driven by magnetic flux emergence. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/10129

Chicago Manual of Style (16th Edition):

Sturrock, Zoe. “Numerical simulations of sunspot rotation driven by magnetic flux emergence.” 2017. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/10129.

MLA Handbook (7th Edition):

Sturrock, Zoe. “Numerical simulations of sunspot rotation driven by magnetic flux emergence.” 2017. Web. 03 Dec 2020.

Vancouver:

Sturrock Z. Numerical simulations of sunspot rotation driven by magnetic flux emergence. [Internet] [Doctoral dissertation]. University of St Andrews; 2017. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/10129.

Council of Science Editors:

Sturrock Z. Numerical simulations of sunspot rotation driven by magnetic flux emergence. [Doctoral Dissertation]. University of St Andrews; 2017. Available from: http://hdl.handle.net/10023/10129


University of St Andrews

22. Mellor, Christopher. Magnetic annihilation, null collapse and coronal heating.

Degree: PhD, 2004, University of St Andrews

 The problem of how the Sun's corona is heated is of central importance to solar physics research. In this thesis we model three main areas.… (more)

Subjects/Keywords: 523.7; QB529.M4; Magnetohydrodynamics; Solar magnetic fields; Sun – Corona; Plasma (Ionized gases)

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APA (6th Edition):

Mellor, C. (2004). Magnetic annihilation, null collapse and coronal heating. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/12946

Chicago Manual of Style (16th Edition):

Mellor, Christopher. “Magnetic annihilation, null collapse and coronal heating.” 2004. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/12946.

MLA Handbook (7th Edition):

Mellor, Christopher. “Magnetic annihilation, null collapse and coronal heating.” 2004. Web. 03 Dec 2020.

Vancouver:

Mellor C. Magnetic annihilation, null collapse and coronal heating. [Internet] [Doctoral dissertation]. University of St Andrews; 2004. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/12946.

Council of Science Editors:

Mellor C. Magnetic annihilation, null collapse and coronal heating. [Doctoral Dissertation]. University of St Andrews; 2004. Available from: http://hdl.handle.net/10023/12946


New Jersey Institute of Technology

23. Tan, Changyi. Relationship between photospheric magnetic fields and coronal activities.

Degree: PhD, Federated Physics Department, 2010, New Jersey Institute of Technology

  Coronal emission comes in two forms, a steady component where the corona is heated to million degrees and a much hotter transient component of… (more)

Subjects/Keywords: Sun; Magnetic fields; Flares; X-rays; Corona; Sunspot; Other Physics

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APA (6th Edition):

Tan, C. (2010). Relationship between photospheric magnetic fields and coronal activities. (Doctoral Dissertation). New Jersey Institute of Technology. Retrieved from https://digitalcommons.njit.edu/dissertations/200

Chicago Manual of Style (16th Edition):

Tan, Changyi. “Relationship between photospheric magnetic fields and coronal activities.” 2010. Doctoral Dissertation, New Jersey Institute of Technology. Accessed December 03, 2020. https://digitalcommons.njit.edu/dissertations/200.

MLA Handbook (7th Edition):

Tan, Changyi. “Relationship between photospheric magnetic fields and coronal activities.” 2010. Web. 03 Dec 2020.

Vancouver:

Tan C. Relationship between photospheric magnetic fields and coronal activities. [Internet] [Doctoral dissertation]. New Jersey Institute of Technology; 2010. [cited 2020 Dec 03]. Available from: https://digitalcommons.njit.edu/dissertations/200.

Council of Science Editors:

Tan C. Relationship between photospheric magnetic fields and coronal activities. [Doctoral Dissertation]. New Jersey Institute of Technology; 2010. Available from: https://digitalcommons.njit.edu/dissertations/200


University of St Andrews

24. Cook, Graeme Robert. Magnetic flux transport simulations : applications to solar and stellar magnetic fields.

Degree: PhD, 2011, University of St Andrews

Magnetic fields play a key role in a wide variety of phenomena found on the Sun. One such phenomena is the Coronal Mass Ejection (CME)… (more)

Subjects/Keywords: 520; Solar; Magnetic flux transport; Applied mathematics; Coronal mass ejections; Stellar magnetic fields; QB539.M23C7; Solar magnetic fields – Mathematical models; Coronal mass ejections; Stars – Magnetic fields – Mathematical models

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APA (6th Edition):

Cook, G. R. (2011). Magnetic flux transport simulations : applications to solar and stellar magnetic fields. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/2072

Chicago Manual of Style (16th Edition):

Cook, Graeme Robert. “Magnetic flux transport simulations : applications to solar and stellar magnetic fields.” 2011. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/2072.

MLA Handbook (7th Edition):

Cook, Graeme Robert. “Magnetic flux transport simulations : applications to solar and stellar magnetic fields.” 2011. Web. 03 Dec 2020.

Vancouver:

Cook GR. Magnetic flux transport simulations : applications to solar and stellar magnetic fields. [Internet] [Doctoral dissertation]. University of St Andrews; 2011. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/2072.

Council of Science Editors:

Cook GR. Magnetic flux transport simulations : applications to solar and stellar magnetic fields. [Doctoral Dissertation]. University of St Andrews; 2011. Available from: http://hdl.handle.net/10023/2072

25. Roberts, Merrill. The Interior Structure, Dynamics, and Heliospheric Impact of Reconnection-Driven Solar Coronal Hole Jets.

Degree: 2018, The Catholic University of America

From bright loop structures and polar plumes to solar flares and coronal mass ejections(CMEs), our Sun has shown itself to be a highly dynamic star… (more)

Subjects/Keywords: Corona; Coronal Holes; Magnetic Reconnection; Magnetohydrodynamics; Parker Solar Probe (PSP); Sun

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APA (6th Edition):

Roberts, M. (2018). The Interior Structure, Dynamics, and Heliospheric Impact of Reconnection-Driven Solar Coronal Hole Jets. (Thesis). The Catholic University of America. Retrieved from http://hdl.handle.net/1961/cuislandora:72136

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):

Roberts, Merrill. “The Interior Structure, Dynamics, and Heliospheric Impact of Reconnection-Driven Solar Coronal Hole Jets.” 2018. Thesis, The Catholic University of America. Accessed December 03, 2020. http://hdl.handle.net/1961/cuislandora:72136.

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

MLA Handbook (7th Edition):

Roberts, Merrill. “The Interior Structure, Dynamics, and Heliospheric Impact of Reconnection-Driven Solar Coronal Hole Jets.” 2018. Web. 03 Dec 2020.

Vancouver:

Roberts M. The Interior Structure, Dynamics, and Heliospheric Impact of Reconnection-Driven Solar Coronal Hole Jets. [Internet] [Thesis]. The Catholic University of America; 2018. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/1961/cuislandora:72136.

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

Council of Science Editors:

Roberts M. The Interior Structure, Dynamics, and Heliospheric Impact of Reconnection-Driven Solar Coronal Hole Jets. [Thesis]. The Catholic University of America; 2018. Available from: http://hdl.handle.net/1961/cuislandora:72136

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


University of Sydney

26. Gilchrist, Stuart. Data-driven numerical modelling of the solar coronal magnetic field .

Degree: 2013, University of Sydney

 The aim of this thesis is the development of numerical models for determining the coronal magnetic field from observations of the magnetic field at the… (more)

Subjects/Keywords: Sun; Corona; Magnetic field; Grad-Rubin; Force-free equations

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APA (6th Edition):

Gilchrist, S. (2013). Data-driven numerical modelling of the solar coronal magnetic field . (Thesis). University of Sydney. Retrieved from http://hdl.handle.net/2123/10217

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):

Gilchrist, Stuart. “Data-driven numerical modelling of the solar coronal magnetic field .” 2013. Thesis, University of Sydney. Accessed December 03, 2020. http://hdl.handle.net/2123/10217.

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

MLA Handbook (7th Edition):

Gilchrist, Stuart. “Data-driven numerical modelling of the solar coronal magnetic field .” 2013. Web. 03 Dec 2020.

Vancouver:

Gilchrist S. Data-driven numerical modelling of the solar coronal magnetic field . [Internet] [Thesis]. University of Sydney; 2013. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/2123/10217.

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

Council of Science Editors:

Gilchrist S. Data-driven numerical modelling of the solar coronal magnetic field . [Thesis]. University of Sydney; 2013. Available from: http://hdl.handle.net/2123/10217

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


Montana State University

27. Egeland, Ricky Alan. Long-term variability of the sun in the context of solar-analog stars.

Degree: College of Letters & Science, 2017, Montana State University

 The Sun is the best observed object in astrophysics, but despite this distinction the nature of its well-ordered generation of magnetic field in 11-year activity… (more)

Subjects/Keywords: Sun.; Solar magnetic fields.; Solar cycle.

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APA (6th Edition):

Egeland, R. A. (2017). Long-term variability of the sun in the context of solar-analog stars. (Thesis). Montana State University. Retrieved from https://scholarworks.montana.edu/xmlui/handle/1/12774

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):

Egeland, Ricky Alan. “Long-term variability of the sun in the context of solar-analog stars.” 2017. Thesis, Montana State University. Accessed December 03, 2020. https://scholarworks.montana.edu/xmlui/handle/1/12774.

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

MLA Handbook (7th Edition):

Egeland, Ricky Alan. “Long-term variability of the sun in the context of solar-analog stars.” 2017. Web. 03 Dec 2020.

Vancouver:

Egeland RA. Long-term variability of the sun in the context of solar-analog stars. [Internet] [Thesis]. Montana State University; 2017. [cited 2020 Dec 03]. Available from: https://scholarworks.montana.edu/xmlui/handle/1/12774.

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

Council of Science Editors:

Egeland RA. Long-term variability of the sun in the context of solar-analog stars. [Thesis]. Montana State University; 2017. Available from: https://scholarworks.montana.edu/xmlui/handle/1/12774

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


University of Exeter

28. Hawkes, G. Magnetic helicity flow in the Sun and heliosphere.

Degree: PhD, 2020, University of Exeter

Magnetic helicity, the measure of entanglement within a magnetic field, has the capability to further our knowledge of the magnetic fields which are ubiquitous across… (more)

Subjects/Keywords: magnetic fields; helicity; sun; solar physics

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APA (6th Edition):

Hawkes, G. (2020). Magnetic helicity flow in the Sun and heliosphere. (Doctoral Dissertation). University of Exeter. Retrieved from http://hdl.handle.net/10871/121154

Chicago Manual of Style (16th Edition):

Hawkes, G. “Magnetic helicity flow in the Sun and heliosphere.” 2020. Doctoral Dissertation, University of Exeter. Accessed December 03, 2020. http://hdl.handle.net/10871/121154.

MLA Handbook (7th Edition):

Hawkes, G. “Magnetic helicity flow in the Sun and heliosphere.” 2020. Web. 03 Dec 2020.

Vancouver:

Hawkes G. Magnetic helicity flow in the Sun and heliosphere. [Internet] [Doctoral dissertation]. University of Exeter; 2020. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10871/121154.

Council of Science Editors:

Hawkes G. Magnetic helicity flow in the Sun and heliosphere. [Doctoral Dissertation]. University of Exeter; 2020. Available from: http://hdl.handle.net/10871/121154


University of St Andrews

29. Murray, Michelle J. Solar flux emergence : a three-dimensional numerical study.

Degree: PhD, 2008, University of St Andrews

 Flux is continually emerging on the Sun, making its way from the solar interior up into the atmosphere. Emergence occurs on small-scales in the quiet… (more)

Subjects/Keywords: 520; Sun; Flux emergence; Numerical; Simulation; QB539.M23M8; Solar magnetic fields – Mathematical models; Magnetic flux

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APA (6th Edition):

Murray, M. J. (2008). Solar flux emergence : a three-dimensional numerical study. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/441

Chicago Manual of Style (16th Edition):

Murray, Michelle J. “Solar flux emergence : a three-dimensional numerical study.” 2008. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/441.

MLA Handbook (7th Edition):

Murray, Michelle J. “Solar flux emergence : a three-dimensional numerical study.” 2008. Web. 03 Dec 2020.

Vancouver:

Murray MJ. Solar flux emergence : a three-dimensional numerical study. [Internet] [Doctoral dissertation]. University of St Andrews; 2008. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/441.

Council of Science Editors:

Murray MJ. Solar flux emergence : a three-dimensional numerical study. [Doctoral Dissertation]. University of St Andrews; 2008. Available from: http://hdl.handle.net/10023/441


University of St Andrews

30. McDougall-Bagnall, A. M. Dee. MHD mode conversion of fast and slow magnetoacoustic waves in the solar corona.

Degree: PhD, 2010, University of St Andrews

 There are three main wave types present in the Sun’s atmosphere: Alfvén waves and fast and slow magnetoacoustic waves. Alfvén waves are purely magnetic and… (more)

Subjects/Keywords: 520; Sun; Magnetohydrodynamics; Waves; Mode conversion; Corona; QB529.M3; Sun – Corona; Magnetohydrodynamic waves – Mathematical models

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APA (6th Edition):

McDougall-Bagnall, A. M. D. (2010). MHD mode conversion of fast and slow magnetoacoustic waves in the solar corona. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/1361

Chicago Manual of Style (16th Edition):

McDougall-Bagnall, A M Dee. “MHD mode conversion of fast and slow magnetoacoustic waves in the solar corona.” 2010. Doctoral Dissertation, University of St Andrews. Accessed December 03, 2020. http://hdl.handle.net/10023/1361.

MLA Handbook (7th Edition):

McDougall-Bagnall, A M Dee. “MHD mode conversion of fast and slow magnetoacoustic waves in the solar corona.” 2010. Web. 03 Dec 2020.

Vancouver:

McDougall-Bagnall AMD. MHD mode conversion of fast and slow magnetoacoustic waves in the solar corona. [Internet] [Doctoral dissertation]. University of St Andrews; 2010. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10023/1361.

Council of Science Editors:

McDougall-Bagnall AMD. MHD mode conversion of fast and slow magnetoacoustic waves in the solar corona. [Doctoral Dissertation]. University of St Andrews; 2010. Available from: http://hdl.handle.net/10023/1361

[1] [2] [3] [4] [5] … [2003]

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