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You searched for subject:(Solar magnetic fields ). Showing records 1 – 30 of 28490 total matches.

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Montana State University

1. Kobelski, Adam Robert. Empirical studies on the initiation of impulsive heating in coronal loops.

Degree: College of Letters & Science, 2014, Montana State University

 The heating of the solar corona is an important topic both for scientists and modern society. One of the most fundamental of structures in the… (more)

Subjects/Keywords: Solar magnetic fields.; Solar flares.

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APA (6th Edition):

Kobelski, A. R. (2014). Empirical studies on the initiation of impulsive heating in coronal loops. (Thesis). Montana State University. Retrieved from https://scholarworks.montana.edu/xmlui/handle/1/8697

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):

Kobelski, Adam Robert. “Empirical studies on the initiation of impulsive heating in coronal loops.” 2014. Thesis, Montana State University. Accessed December 02, 2020. https://scholarworks.montana.edu/xmlui/handle/1/8697.

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

MLA Handbook (7th Edition):

Kobelski, Adam Robert. “Empirical studies on the initiation of impulsive heating in coronal loops.” 2014. Web. 02 Dec 2020.

Vancouver:

Kobelski AR. Empirical studies on the initiation of impulsive heating in coronal loops. [Internet] [Thesis]. Montana State University; 2014. [cited 2020 Dec 02]. Available from: https://scholarworks.montana.edu/xmlui/handle/1/8697.

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

Council of Science Editors:

Kobelski AR. Empirical studies on the initiation of impulsive heating in coronal loops. [Thesis]. Montana State University; 2014. Available from: https://scholarworks.montana.edu/xmlui/handle/1/8697

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


Montana State University

2. 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 02, 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. 02 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 02]. 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 Delaware

3. Tessein, Jeffrey A. Effect of coherent structures on energetic particle intensity in the solar wind.

Degree: PhD, University of Delaware, Department of Physics and Astronomy, 2015, University of Delaware

Solar energetic particles in the solar wind are accelerated in both solar flares and shocks assocated with fast coronal mass ejections. They follow the interplanetary… (more)

Subjects/Keywords: Solar energetic particles.; Solar wind.; Magnetic fields.

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APA (6th Edition):

Tessein, J. A. (2015). Effect of coherent structures on energetic particle intensity in the solar wind. (Doctoral Dissertation). University of Delaware. Retrieved from http://udspace.udel.edu/handle/19716/17614

Chicago Manual of Style (16th Edition):

Tessein, Jeffrey A. “Effect of coherent structures on energetic particle intensity in the solar wind.” 2015. Doctoral Dissertation, University of Delaware. Accessed December 02, 2020. http://udspace.udel.edu/handle/19716/17614.

MLA Handbook (7th Edition):

Tessein, Jeffrey A. “Effect of coherent structures on energetic particle intensity in the solar wind.” 2015. Web. 02 Dec 2020.

Vancouver:

Tessein JA. Effect of coherent structures on energetic particle intensity in the solar wind. [Internet] [Doctoral dissertation]. University of Delaware; 2015. [cited 2020 Dec 02]. Available from: http://udspace.udel.edu/handle/19716/17614.

Council of Science Editors:

Tessein JA. Effect of coherent structures on energetic particle intensity in the solar wind. [Doctoral Dissertation]. University of Delaware; 2015. Available from: http://udspace.udel.edu/handle/19716/17614


University of Cambridge

4. Wood, Toby. The solar tachocline: a self-consistent model of magnetic confinement.

Degree: PhD, 2011, University of Cambridge

 In this dissertation we consider the dynamics of the solar interior, with particular focus on angular momentum balance and magnetic field confinement within the tachocline.… (more)

Subjects/Keywords: Heliophysics; Solar rotation; Magnetic fields; Solar tachocline

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APA (6th Edition):

Wood, T. (2011). The solar tachocline: a self-consistent model of magnetic confinement. (Doctoral Dissertation). University of Cambridge. Retrieved from http://www.dspace.cam.ac.uk/handle/1810/230114https://www.repository.cam.ac.uk/bitstream/1810/230114/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/3/tsw-thesis-final-online.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/5/tsw-thesis-final-online.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/6/tsw-thesis-final-online.pdf.jpg

Chicago Manual of Style (16th Edition):

Wood, Toby. “The solar tachocline: a self-consistent model of magnetic confinement.” 2011. Doctoral Dissertation, University of Cambridge. Accessed December 02, 2020. http://www.dspace.cam.ac.uk/handle/1810/230114https://www.repository.cam.ac.uk/bitstream/1810/230114/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/3/tsw-thesis-final-online.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/5/tsw-thesis-final-online.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/6/tsw-thesis-final-online.pdf.jpg.

MLA Handbook (7th Edition):

Wood, Toby. “The solar tachocline: a self-consistent model of magnetic confinement.” 2011. Web. 02 Dec 2020.

Vancouver:

Wood T. The solar tachocline: a self-consistent model of magnetic confinement. [Internet] [Doctoral dissertation]. University of Cambridge; 2011. [cited 2020 Dec 02]. Available from: http://www.dspace.cam.ac.uk/handle/1810/230114https://www.repository.cam.ac.uk/bitstream/1810/230114/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/3/tsw-thesis-final-online.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/5/tsw-thesis-final-online.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/6/tsw-thesis-final-online.pdf.jpg.

Council of Science Editors:

Wood T. The solar tachocline: a self-consistent model of magnetic confinement. [Doctoral Dissertation]. University of Cambridge; 2011. Available from: http://www.dspace.cam.ac.uk/handle/1810/230114https://www.repository.cam.ac.uk/bitstream/1810/230114/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/3/tsw-thesis-final-online.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/5/tsw-thesis-final-online.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/230114/6/tsw-thesis-final-online.pdf.jpg


University of St Andrews

5. Thornton, L. M. Small-scale magnetic feature evolution as observed by Hinode/NFI and SOHO/MDI.

Degree: PhD, 2011, University of St Andrews

 The surface (photosphere) of the Sun is threaded throughout by magnetic fields. Groups of magnetic fields form magnetic features (of a wide range of sizes… (more)

Subjects/Keywords: 520; QB539.M23T5 : Solar magnetic fields : Solar photosphere : Magnetic flux

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APA (6th Edition):

Thornton, L. M. (2011). Small-scale magnetic feature evolution as observed by Hinode/NFI and SOHO/MDI. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/2083

Chicago Manual of Style (16th Edition):

Thornton, L M. “Small-scale magnetic feature evolution as observed by Hinode/NFI and SOHO/MDI.” 2011. Doctoral Dissertation, University of St Andrews. Accessed December 02, 2020. http://hdl.handle.net/10023/2083.

MLA Handbook (7th Edition):

Thornton, L M. “Small-scale magnetic feature evolution as observed by Hinode/NFI and SOHO/MDI.” 2011. Web. 02 Dec 2020.

Vancouver:

Thornton LM. Small-scale magnetic feature evolution as observed by Hinode/NFI and SOHO/MDI. [Internet] [Doctoral dissertation]. University of St Andrews; 2011. [cited 2020 Dec 02]. Available from: http://hdl.handle.net/10023/2083.

Council of Science Editors:

Thornton LM. Small-scale magnetic feature evolution as observed by Hinode/NFI and SOHO/MDI. [Doctoral Dissertation]. University of St Andrews; 2011. Available from: http://hdl.handle.net/10023/2083


University of Exeter

6. 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 02, 2020. http://hdl.handle.net/10871/121154.

MLA Handbook (7th Edition):

Hawkes, G. “Magnetic helicity flow in the Sun and heliosphere.” 2020. Web. 02 Dec 2020.

Vancouver:

Hawkes G. Magnetic helicity flow in the Sun and heliosphere. [Internet] [Doctoral dissertation]. University of Exeter; 2020. [cited 2020 Dec 02]. 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


Montana State University

7. Eckberg, Jon Thomas. Network flux transport: concept and application to solar magnetism.

Degree: MS, College of Letters & Science, 2019, Montana State University

 We have developed a method to efficiently simulate the dynamics of the magnetic flux in the solar network. We call this method Network Flux Transport… (more)

Subjects/Keywords: Solar magnetic fields.; Dynamics.; Simulation methods.

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APA (6th Edition):

Eckberg, J. T. (2019). Network flux transport: concept and application to solar magnetism. (Masters Thesis). Montana State University. Retrieved from https://scholarworks.montana.edu/xmlui/handle/1/15768

Chicago Manual of Style (16th Edition):

Eckberg, Jon Thomas. “Network flux transport: concept and application to solar magnetism.” 2019. Masters Thesis, Montana State University. Accessed December 02, 2020. https://scholarworks.montana.edu/xmlui/handle/1/15768.

MLA Handbook (7th Edition):

Eckberg, Jon Thomas. “Network flux transport: concept and application to solar magnetism.” 2019. Web. 02 Dec 2020.

Vancouver:

Eckberg JT. Network flux transport: concept and application to solar magnetism. [Internet] [Masters thesis]. Montana State University; 2019. [cited 2020 Dec 02]. Available from: https://scholarworks.montana.edu/xmlui/handle/1/15768.

Council of Science Editors:

Eckberg JT. Network flux transport: concept and application to solar magnetism. [Masters Thesis]. Montana State University; 2019. Available from: https://scholarworks.montana.edu/xmlui/handle/1/15768


Montana State University

8. Munoz-Jaramillo, Andres. Towards better constrained models of the solar magnetic cycle.

Degree: PhD, College of Letters & Science, 2010, Montana State University

 The best tools we have for understanding the origin of solar magnetic variability are kinematic dynamo models. During the last decade, this type of models… (more)

Subjects/Keywords: Solar magnetic fields.

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APA (6th Edition):

Munoz-Jaramillo, A. (2010). Towards better constrained models of the solar magnetic cycle. (Doctoral Dissertation). Montana State University. Retrieved from https://scholarworks.montana.edu/xmlui/handle/1/1919

Chicago Manual of Style (16th Edition):

Munoz-Jaramillo, Andres. “Towards better constrained models of the solar magnetic cycle.” 2010. Doctoral Dissertation, Montana State University. Accessed December 02, 2020. https://scholarworks.montana.edu/xmlui/handle/1/1919.

MLA Handbook (7th Edition):

Munoz-Jaramillo, Andres. “Towards better constrained models of the solar magnetic cycle.” 2010. Web. 02 Dec 2020.

Vancouver:

Munoz-Jaramillo A. Towards better constrained models of the solar magnetic cycle. [Internet] [Doctoral dissertation]. Montana State University; 2010. [cited 2020 Dec 02]. Available from: https://scholarworks.montana.edu/xmlui/handle/1/1919.

Council of Science Editors:

Munoz-Jaramillo A. Towards better constrained models of the solar magnetic cycle. [Doctoral Dissertation]. Montana State University; 2010. Available from: https://scholarworks.montana.edu/xmlui/handle/1/1919


Montana State University

9. 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 02, 2020. https://scholarworks.montana.edu/xmlui/handle/1/2917.

MLA Handbook (7th Edition):

Tarr, Lucas Adrian. “Energetic consequences of flux emergence.” 2013. Web. 02 Dec 2020.

Vancouver:

Tarr LA. Energetic consequences of flux emergence. [Internet] [Doctoral dissertation]. Montana State University; 2013. [cited 2020 Dec 02]. 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


Montana State University

10. Scott, Jason Terrence. Multi-instrument observations of coronal loops.

Degree: PhD, College of Letters & Science, 2012, Montana State University

 This document exhibits results of analysis from data collected with multiple EUV satellites (SOHO, TRACE, STEREO, Hinode, and SDO). The focus is the detailed observation… (more)

Subjects/Keywords: Spectrum analysis; Imaging systems; Solar magnetic fields

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APA (6th Edition):

Scott, J. T. (2012). Multi-instrument observations of coronal loops. (Doctoral Dissertation). Montana State University. Retrieved from https://scholarworks.montana.edu/xmlui/handle/1/2228

Chicago Manual of Style (16th Edition):

Scott, Jason Terrence. “Multi-instrument observations of coronal loops.” 2012. Doctoral Dissertation, Montana State University. Accessed December 02, 2020. https://scholarworks.montana.edu/xmlui/handle/1/2228.

MLA Handbook (7th Edition):

Scott, Jason Terrence. “Multi-instrument observations of coronal loops.” 2012. Web. 02 Dec 2020.

Vancouver:

Scott JT. Multi-instrument observations of coronal loops. [Internet] [Doctoral dissertation]. Montana State University; 2012. [cited 2020 Dec 02]. Available from: https://scholarworks.montana.edu/xmlui/handle/1/2228.

Council of Science Editors:

Scott JT. Multi-instrument observations of coronal loops. [Doctoral Dissertation]. Montana State University; 2012. Available from: https://scholarworks.montana.edu/xmlui/handle/1/2228


Colorado State University

11. Weber, Maria Ann. Dynamic evolution of active-region-scale magnetic flux tubes in the turbulent solar convective envelope, The.

Degree: PhD, Physics, 2014, Colorado State University

 The Sun exhibits cyclic properties of its large-scale magnetic field on the order of ~22 years, with a ~11 year frequency of sunspot occurrence. These… (more)

Subjects/Keywords: convection; flux emergence; solar interior; solar magnetic fields; solar physics; sun

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APA (6th Edition):

Weber, M. A. (2014). Dynamic evolution of active-region-scale magnetic flux tubes in the turbulent solar convective envelope, The. (Doctoral Dissertation). Colorado State University. Retrieved from http://hdl.handle.net/10217/83825

Chicago Manual of Style (16th Edition):

Weber, Maria Ann. “Dynamic evolution of active-region-scale magnetic flux tubes in the turbulent solar convective envelope, The.” 2014. Doctoral Dissertation, Colorado State University. Accessed December 02, 2020. http://hdl.handle.net/10217/83825.

MLA Handbook (7th Edition):

Weber, Maria Ann. “Dynamic evolution of active-region-scale magnetic flux tubes in the turbulent solar convective envelope, The.” 2014. Web. 02 Dec 2020.

Vancouver:

Weber MA. Dynamic evolution of active-region-scale magnetic flux tubes in the turbulent solar convective envelope, The. [Internet] [Doctoral dissertation]. Colorado State University; 2014. [cited 2020 Dec 02]. Available from: http://hdl.handle.net/10217/83825.

Council of Science Editors:

Weber MA. Dynamic evolution of active-region-scale magnetic flux tubes in the turbulent solar convective envelope, The. [Doctoral Dissertation]. Colorado State University; 2014. Available from: http://hdl.handle.net/10217/83825


University of Cambridge

12. Wood, Toby. The solar tachocline : a self-consistent model of magnetic confinement.

Degree: PhD, 2011, University of Cambridge

 In this dissertation we consider the dynamics of the solar interior, with particular focus on angular momentum balance and magnetic field confinement within the tachocline.… (more)

Subjects/Keywords: 520; Heliophysics; Solar rotation; Magnetic fields; Solar tachocline

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APA (6th Edition):

Wood, T. (2011). The solar tachocline : a self-consistent model of magnetic confinement. (Doctoral Dissertation). University of Cambridge. Retrieved from https://doi.org/10.17863/CAM.16099 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.541844

Chicago Manual of Style (16th Edition):

Wood, Toby. “The solar tachocline : a self-consistent model of magnetic confinement.” 2011. Doctoral Dissertation, University of Cambridge. Accessed December 02, 2020. https://doi.org/10.17863/CAM.16099 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.541844.

MLA Handbook (7th Edition):

Wood, Toby. “The solar tachocline : a self-consistent model of magnetic confinement.” 2011. Web. 02 Dec 2020.

Vancouver:

Wood T. The solar tachocline : a self-consistent model of magnetic confinement. [Internet] [Doctoral dissertation]. University of Cambridge; 2011. [cited 2020 Dec 02]. Available from: https://doi.org/10.17863/CAM.16099 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.541844.

Council of Science Editors:

Wood T. The solar tachocline : a self-consistent model of magnetic confinement. [Doctoral Dissertation]. University of Cambridge; 2011. Available from: https://doi.org/10.17863/CAM.16099 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.541844


Montana State University

13. Rust, Thomas Ludwell. Explosive events in the quiet Sun: extreme ultraviolet imaging spectroscopy instrumentation and observations.

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

 Explosive event is the name given to slit spectrograph observations of high spectroscopic velocities in solar transition region spectral lines. Explosive events show much variety… (more)

Subjects/Keywords: Optical spectroscopy.; Ultraviolet radiation.; Magnetic reconnection.; Solar magnetic fields.

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APA (6th Edition):

Rust, T. L. (2017). Explosive events in the quiet Sun: extreme ultraviolet imaging spectroscopy instrumentation and observations. (Thesis). Montana State University. Retrieved from https://scholarworks.montana.edu/xmlui/handle/1/13485

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):

Rust, Thomas Ludwell. “Explosive events in the quiet Sun: extreme ultraviolet imaging spectroscopy instrumentation and observations.” 2017. Thesis, Montana State University. Accessed December 02, 2020. https://scholarworks.montana.edu/xmlui/handle/1/13485.

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

MLA Handbook (7th Edition):

Rust, Thomas Ludwell. “Explosive events in the quiet Sun: extreme ultraviolet imaging spectroscopy instrumentation and observations.” 2017. Web. 02 Dec 2020.

Vancouver:

Rust TL. Explosive events in the quiet Sun: extreme ultraviolet imaging spectroscopy instrumentation and observations. [Internet] [Thesis]. Montana State University; 2017. [cited 2020 Dec 02]. Available from: https://scholarworks.montana.edu/xmlui/handle/1/13485.

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

Council of Science Editors:

Rust TL. Explosive events in the quiet Sun: extreme ultraviolet imaging spectroscopy instrumentation and observations. [Thesis]. Montana State University; 2017. Available from: https://scholarworks.montana.edu/xmlui/handle/1/13485

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


University of Manchester

14. Bareford, Michael. The Heating of the Solar Corona by Kink Instabilities.

Degree: 2012, University of Manchester

 The million-degree temperature of the solar corona might be due to the combined effectof barely distinguishable energy releases, called nanoflares, that occur throughoutthe solar atmosphere.… (more)

Subjects/Keywords: Solar Corona; Magnetic Fields; Magnetohydrodynamics; Instabilities; Magnetic Reconnection; Plasmas

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APA (6th Edition):

Bareford, M. (2012). The Heating of the Solar Corona by Kink Instabilities. (Doctoral Dissertation). University of Manchester. Retrieved from http://www.manchester.ac.uk/escholar/uk-ac-man-scw:155144

Chicago Manual of Style (16th Edition):

Bareford, Michael. “The Heating of the Solar Corona by Kink Instabilities.” 2012. Doctoral Dissertation, University of Manchester. Accessed December 02, 2020. http://www.manchester.ac.uk/escholar/uk-ac-man-scw:155144.

MLA Handbook (7th Edition):

Bareford, Michael. “The Heating of the Solar Corona by Kink Instabilities.” 2012. Web. 02 Dec 2020.

Vancouver:

Bareford M. The Heating of the Solar Corona by Kink Instabilities. [Internet] [Doctoral dissertation]. University of Manchester; 2012. [cited 2020 Dec 02]. Available from: http://www.manchester.ac.uk/escholar/uk-ac-man-scw:155144.

Council of Science Editors:

Bareford M. The Heating of the Solar Corona by Kink Instabilities. [Doctoral Dissertation]. University of Manchester; 2012. Available from: http://www.manchester.ac.uk/escholar/uk-ac-man-scw:155144


University of Manchester

15. Bareford, Michael. The heating of the solar corona by kink instabilities.

Degree: PhD, 2012, University of Manchester

 The million-degree temperature of the solar corona might be due to the combined effect of barely distinguishable energy releases, called nanoflares, that occur throughout the… (more)

Subjects/Keywords: 520; Solar Corona; Magnetic Fields; Magnetohydrodynamics; Instabilities; Magnetic Reconnection; Plasmas

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APA (6th Edition):

Bareford, M. (2012). The heating of the solar corona by kink instabilities. (Doctoral Dissertation). University of Manchester. Retrieved from https://www.research.manchester.ac.uk/portal/en/theses/the-heating-of-the-solar-corona-by-kink-instabilities(b61532f0-e02c-4a03-a751-450d6ce7ad59).html ; http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.549649

Chicago Manual of Style (16th Edition):

Bareford, Michael. “The heating of the solar corona by kink instabilities.” 2012. Doctoral Dissertation, University of Manchester. Accessed December 02, 2020. https://www.research.manchester.ac.uk/portal/en/theses/the-heating-of-the-solar-corona-by-kink-instabilities(b61532f0-e02c-4a03-a751-450d6ce7ad59).html ; http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.549649.

MLA Handbook (7th Edition):

Bareford, Michael. “The heating of the solar corona by kink instabilities.” 2012. Web. 02 Dec 2020.

Vancouver:

Bareford M. The heating of the solar corona by kink instabilities. [Internet] [Doctoral dissertation]. University of Manchester; 2012. [cited 2020 Dec 02]. Available from: https://www.research.manchester.ac.uk/portal/en/theses/the-heating-of-the-solar-corona-by-kink-instabilities(b61532f0-e02c-4a03-a751-450d6ce7ad59).html ; http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.549649.

Council of Science Editors:

Bareford M. The heating of the solar corona by kink instabilities. [Doctoral Dissertation]. University of Manchester; 2012. Available from: https://www.research.manchester.ac.uk/portal/en/theses/the-heating-of-the-solar-corona-by-kink-instabilities(b61532f0-e02c-4a03-a751-450d6ce7ad59).html ; http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.549649


New Jersey Institute of Technology

16. Park, Sung-Hong. Study of magnetic helicity in solar active regions and its relationship with solar eruptions.

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

  It is generally believed that eruptive phenomena in the solar atmosphere such as solar flares and coronal mass ejections (CMEs) occur in solar active… (more)

Subjects/Keywords: The sun; Magnetic helicity; Solar active regions; Magnetic fields; Solar eruptions; Flare forecasting; Other Physics

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APA (6th Edition):

Park, S. (2010). Study of magnetic helicity in solar active regions and its relationship with solar eruptions. (Doctoral Dissertation). New Jersey Institute of Technology. Retrieved from https://digitalcommons.njit.edu/dissertations/226

Chicago Manual of Style (16th Edition):

Park, Sung-Hong. “Study of magnetic helicity in solar active regions and its relationship with solar eruptions.” 2010. Doctoral Dissertation, New Jersey Institute of Technology. Accessed December 02, 2020. https://digitalcommons.njit.edu/dissertations/226.

MLA Handbook (7th Edition):

Park, Sung-Hong. “Study of magnetic helicity in solar active regions and its relationship with solar eruptions.” 2010. Web. 02 Dec 2020.

Vancouver:

Park S. Study of magnetic helicity in solar active regions and its relationship with solar eruptions. [Internet] [Doctoral dissertation]. New Jersey Institute of Technology; 2010. [cited 2020 Dec 02]. Available from: https://digitalcommons.njit.edu/dissertations/226.

Council of Science Editors:

Park S. Study of magnetic helicity in solar active regions and its relationship with solar eruptions. [Doctoral Dissertation]. New Jersey Institute of Technology; 2010. Available from: https://digitalcommons.njit.edu/dissertations/226


University of St Andrews

17. 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 02, 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. 02 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 02]. 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

18. 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 02, 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. 02 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 02]. 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

19. 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 02, 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. 02 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 02]. 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

20. Mathew,S K. Study of solar magnetic and velocity fields; -.

Degree: Science, 2014, Gujarat University

Available newline

-

Advisors/Committee Members: Ashok,N M.

Subjects/Keywords: magnetic; solar; Study; velocity fields

Page 1

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APA (6th Edition):

K, M. (2014). Study of solar magnetic and velocity fields; -. (Thesis). Gujarat University. Retrieved from http://shodhganga.inflibnet.ac.in/handle/10603/30504

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):

K, Mathew,S. “Study of solar magnetic and velocity fields; -.” 2014. Thesis, Gujarat University. Accessed December 02, 2020. http://shodhganga.inflibnet.ac.in/handle/10603/30504.

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

MLA Handbook (7th Edition):

K, Mathew,S. “Study of solar magnetic and velocity fields; -.” 2014. Web. 02 Dec 2020.

Vancouver:

K M. Study of solar magnetic and velocity fields; -. [Internet] [Thesis]. Gujarat University; 2014. [cited 2020 Dec 02]. Available from: http://shodhganga.inflibnet.ac.in/handle/10603/30504.

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

Council of Science Editors:

K M. Study of solar magnetic and velocity fields; -. [Thesis]. Gujarat University; 2014. Available from: http://shodhganga.inflibnet.ac.in/handle/10603/30504

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


Montana State University

21. Welsch, Brian Thomas. Magnetic helicity transport in the quiet Sun.

Degree: PhD, College of Letters & Science, 2002, Montana State University

Subjects/Keywords: Magnetic fields.; Solar photosphere.

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APA (6th Edition):

Welsch, B. T. (2002). Magnetic helicity transport in the quiet Sun. (Doctoral Dissertation). Montana State University. Retrieved from https://scholarworks.montana.edu/xmlui/handle/1/8197

Chicago Manual of Style (16th Edition):

Welsch, Brian Thomas. “Magnetic helicity transport in the quiet Sun.” 2002. Doctoral Dissertation, Montana State University. Accessed December 02, 2020. https://scholarworks.montana.edu/xmlui/handle/1/8197.

MLA Handbook (7th Edition):

Welsch, Brian Thomas. “Magnetic helicity transport in the quiet Sun.” 2002. Web. 02 Dec 2020.

Vancouver:

Welsch BT. Magnetic helicity transport in the quiet Sun. [Internet] [Doctoral dissertation]. Montana State University; 2002. [cited 2020 Dec 02]. Available from: https://scholarworks.montana.edu/xmlui/handle/1/8197.

Council of Science Editors:

Welsch BT. Magnetic helicity transport in the quiet Sun. [Doctoral Dissertation]. Montana State University; 2002. Available from: https://scholarworks.montana.edu/xmlui/handle/1/8197


University of St Andrews

22. Restante, Anna Lisa. The investigation of quasi-separatrix layers in solar magnetic fields.

Degree: PhD, 2011, University of St Andrews

 The structure of the magnetic field is often an important factor in many energetic processes in the solar corona. To determine the topology of the… (more)

Subjects/Keywords: 520; Solar physics : Quasi-separatrix layers (QSLs) : Magnetic field topology : Reconnection : QB539.M23R4 : Solar magnetic fields – Mathematical models : Magnetic reconnection : Force-free magnetic fields

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APA (6th Edition):

Restante, A. L. (2011). The investigation of quasi-separatrix layers in solar magnetic fields. (Doctoral Dissertation). University of St Andrews. Retrieved from http://hdl.handle.net/10023/2106

Chicago Manual of Style (16th Edition):

Restante, Anna Lisa. “The investigation of quasi-separatrix layers in solar magnetic fields.” 2011. Doctoral Dissertation, University of St Andrews. Accessed December 02, 2020. http://hdl.handle.net/10023/2106.

MLA Handbook (7th Edition):

Restante, Anna Lisa. “The investigation of quasi-separatrix layers in solar magnetic fields.” 2011. Web. 02 Dec 2020.

Vancouver:

Restante AL. The investigation of quasi-separatrix layers in solar magnetic fields. [Internet] [Doctoral dissertation]. University of St Andrews; 2011. [cited 2020 Dec 02]. Available from: http://hdl.handle.net/10023/2106.

Council of Science Editors:

Restante AL. The investigation of quasi-separatrix layers in solar magnetic fields. [Doctoral Dissertation]. University of St Andrews; 2011. Available from: http://hdl.handle.net/10023/2106


University of Hawaii – Manoa

23. Leka, Kimberly Dawn. Are solar emerging flux regions carrying electric current?.

Degree: PhD, 2009, University of Hawaii – Manoa

Microfiche.

xii, 158 leaves, bound ill. 29 cm

Subjects/Keywords: Solar flares; Sunspots; Solar magnetic fields

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APA (6th Edition):

Leka, K. D. (2009). Are solar emerging flux regions carrying electric current?. (Doctoral Dissertation). University of Hawaii – Manoa. Retrieved from http://hdl.handle.net/10125/9353

Chicago Manual of Style (16th Edition):

Leka, Kimberly Dawn. “Are solar emerging flux regions carrying electric current?.” 2009. Doctoral Dissertation, University of Hawaii – Manoa. Accessed December 02, 2020. http://hdl.handle.net/10125/9353.

MLA Handbook (7th Edition):

Leka, Kimberly Dawn. “Are solar emerging flux regions carrying electric current?.” 2009. Web. 02 Dec 2020.

Vancouver:

Leka KD. Are solar emerging flux regions carrying electric current?. [Internet] [Doctoral dissertation]. University of Hawaii – Manoa; 2009. [cited 2020 Dec 02]. Available from: http://hdl.handle.net/10125/9353.

Council of Science Editors:

Leka KD. Are solar emerging flux regions carrying electric current?. [Doctoral Dissertation]. University of Hawaii – Manoa; 2009. Available from: http://hdl.handle.net/10125/9353

24. Cardoso, Elisa Augusto dos Santos. Modelo padrão de dínamo: impacto da densidade solar.

Degree: 2018, Universidade de Évora

 Segundo a Teoria de Dínamo Solar, o campo magnético no Sol é transportado e organizado através da circulação meridional. A circulação meridional nos modelos de… (more)

Subjects/Keywords: Física solar; Campo magnético; Modelo solar; Dínamo solar; Hélio-sismologia; Manchas solares; Solar physics; Magnetic fields; Solar models; Solar dynamo; Helioseismology; Sunspots

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APA (6th Edition):

Cardoso, E. A. d. S. (2018). Modelo padrão de dínamo: impacto da densidade solar. (Thesis). Universidade de Évora. Retrieved from https://www.rcaap.pt/detail.jsp?id=oai:dspace.uevora.pt:10174/23157

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):

Cardoso, Elisa Augusto dos Santos. “Modelo padrão de dínamo: impacto da densidade solar.” 2018. Thesis, Universidade de Évora. Accessed December 02, 2020. https://www.rcaap.pt/detail.jsp?id=oai:dspace.uevora.pt:10174/23157.

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

MLA Handbook (7th Edition):

Cardoso, Elisa Augusto dos Santos. “Modelo padrão de dínamo: impacto da densidade solar.” 2018. Web. 02 Dec 2020.

Vancouver:

Cardoso EAdS. Modelo padrão de dínamo: impacto da densidade solar. [Internet] [Thesis]. Universidade de Évora; 2018. [cited 2020 Dec 02]. Available from: https://www.rcaap.pt/detail.jsp?id=oai:dspace.uevora.pt:10174/23157.

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

Council of Science Editors:

Cardoso EAdS. Modelo padrão de dínamo: impacto da densidade solar. [Thesis]. Universidade de Évora; 2018. Available from: https://www.rcaap.pt/detail.jsp?id=oai:dspace.uevora.pt:10174/23157

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


University of St Andrews

25. 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 02, 2020. http://hdl.handle.net/10023/1692.

MLA Handbook (7th Edition):

MacTaggart, David. “Theoretical magnetic flux emergence.” 2011. Web. 02 Dec 2020.

Vancouver:

MacTaggart D. Theoretical magnetic flux emergence. [Internet] [Doctoral dissertation]. University of St Andrews; 2011. [cited 2020 Dec 02]. 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


Montana State University

26. Welsch, Brian Thomas. Statistical properties of separators in model active regions.

Degree: MS, College of Letters & Science, 1998, Montana State University

Subjects/Keywords: Solar activity; Magnetic separators.; Magnetic reconnection.; Statistics.; Magnetic fields.

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APA (6th Edition):

Welsch, B. T. (1998). Statistical properties of separators in model active regions. (Masters Thesis). Montana State University. Retrieved from https://scholarworks.montana.edu/xmlui/handle/1/7695

Chicago Manual of Style (16th Edition):

Welsch, Brian Thomas. “Statistical properties of separators in model active regions.” 1998. Masters Thesis, Montana State University. Accessed December 02, 2020. https://scholarworks.montana.edu/xmlui/handle/1/7695.

MLA Handbook (7th Edition):

Welsch, Brian Thomas. “Statistical properties of separators in model active regions.” 1998. Web. 02 Dec 2020.

Vancouver:

Welsch BT. Statistical properties of separators in model active regions. [Internet] [Masters thesis]. Montana State University; 1998. [cited 2020 Dec 02]. Available from: https://scholarworks.montana.edu/xmlui/handle/1/7695.

Council of Science Editors:

Welsch BT. Statistical properties of separators in model active regions. [Masters Thesis]. Montana State University; 1998. Available from: https://scholarworks.montana.edu/xmlui/handle/1/7695


Rhodes University

27. Lotz, Stefanus Ignatius. Empirical modelling of the solar wind influence on Pc3 pulsation activity.

Degree: Faculty of Science, Physics and Electronics, 2012, Rhodes University

 Geomagnetic pulsations are ultra-low frequency (ULF) oscillations of the geomagnetic field that have been observed in the magnetosphere and on the Earth since the 1800’s.… (more)

Subjects/Keywords: Solar wind  – Research; Solar activity  – Research; Stellar oscillations  – Research; Magnetospheric radio wave propagation; Interplanetary magnetic fields

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APA (6th Edition):

Lotz, S. I. (2012). Empirical modelling of the solar wind influence on Pc3 pulsation activity. (Thesis). Rhodes University. Retrieved from http://hdl.handle.net/10962/d1005249

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):

Lotz, Stefanus Ignatius. “Empirical modelling of the solar wind influence on Pc3 pulsation activity.” 2012. Thesis, Rhodes University. Accessed December 02, 2020. http://hdl.handle.net/10962/d1005249.

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

MLA Handbook (7th Edition):

Lotz, Stefanus Ignatius. “Empirical modelling of the solar wind influence on Pc3 pulsation activity.” 2012. Web. 02 Dec 2020.

Vancouver:

Lotz SI. Empirical modelling of the solar wind influence on Pc3 pulsation activity. [Internet] [Thesis]. Rhodes University; 2012. [cited 2020 Dec 02]. Available from: http://hdl.handle.net/10962/d1005249.

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

Council of Science Editors:

Lotz SI. Empirical modelling of the solar wind influence on Pc3 pulsation activity. [Thesis]. Rhodes University; 2012. Available from: http://hdl.handle.net/10962/d1005249

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

28. Tereza Satiko Nishida Pinto. Aplicação de campos magnéticos livres de força na explosão solar de 13 de dezembro de 2006.

Degree: 2010, Instituto Nacional de Pesquisas Espaciais

Solar flares can be understood as electromagnetic fenomena occuring at the solar atmosphere. Energy release occurs when magnetic reconnection takes place, followed by particle acceleration,… (more)

Subjects/Keywords: solar flare; force free magnetic fields; inhomogeneous magnetic fields; gyrosynchrotron emission; microwave emission; emissão em microondas; explosões solares; campos magnéticos livres de força; campos magnéticos inomogêneos; emissão girossincrotrônica

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APA (6th Edition):

Pinto, T. S. N. (2010). Aplicação de campos magnéticos livres de força na explosão solar de 13 de dezembro de 2006. (Thesis). Instituto Nacional de Pesquisas Espaciais. Retrieved from http://urlib.net/sid.inpe.br/[email protected]/2010/02.12.17.57

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):

Pinto, Tereza Satiko Nishida. “Aplicação de campos magnéticos livres de força na explosão solar de 13 de dezembro de 2006.” 2010. Thesis, Instituto Nacional de Pesquisas Espaciais. Accessed December 02, 2020. http://urlib.net/sid.inpe.br/[email protected]/2010/02.12.17.57.

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

MLA Handbook (7th Edition):

Pinto, Tereza Satiko Nishida. “Aplicação de campos magnéticos livres de força na explosão solar de 13 de dezembro de 2006.” 2010. Web. 02 Dec 2020.

Vancouver:

Pinto TSN. Aplicação de campos magnéticos livres de força na explosão solar de 13 de dezembro de 2006. [Internet] [Thesis]. Instituto Nacional de Pesquisas Espaciais; 2010. [cited 2020 Dec 02]. Available from: http://urlib.net/sid.inpe.br/[email protected]/2010/02.12.17.57.

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

Council of Science Editors:

Pinto TSN. Aplicação de campos magnéticos livres de força na explosão solar de 13 de dezembro de 2006. [Thesis]. Instituto Nacional de Pesquisas Espaciais; 2010. Available from: http://urlib.net/sid.inpe.br/[email protected]/2010/02.12.17.57

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

29. Edmondson, Justin K. Theory of Three-Dimensional Interchange Reconnection and the Dynamic Evolution of the Global Solar Coronal Magnetic Field Structure: A Mechanism for the Origin and Generation of the Slow Solar Wind.

Degree: PhD, Applied Physics, 2009, University of Michigan

 To understand the evolution of the solar corona and the generation of the solar wind, it is necessary to understand the structure and dynamics of… (more)

Subjects/Keywords: Solar Corona; Magnetic Reconnection; Solar Magnetic Fields; Science

…stored in strong magnetic fields of active regions. A typical solar flare can release energies… …INTERCHANGE RECONNECTION AND THE DYNAMIC EVOLUTION OF THE GLOBAL SOLAR CORONAL MAGNETIC FIELD… …the global coronal magnetic field as a generation mechanism for the slow solar wind. xiii… …processes of the coronal magnetic field central to all solar activity. Observationally, the solar… …The average large-scale solar magnetic field exhibits a dipolar structure separated by an… 

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APA (6th Edition):

Edmondson, J. K. (2009). Theory of Three-Dimensional Interchange Reconnection and the Dynamic Evolution of the Global Solar Coronal Magnetic Field Structure: A Mechanism for the Origin and Generation of the Slow Solar Wind. (Doctoral Dissertation). University of Michigan. Retrieved from http://hdl.handle.net/2027.42/64690

Chicago Manual of Style (16th Edition):

Edmondson, Justin K. “Theory of Three-Dimensional Interchange Reconnection and the Dynamic Evolution of the Global Solar Coronal Magnetic Field Structure: A Mechanism for the Origin and Generation of the Slow Solar Wind.” 2009. Doctoral Dissertation, University of Michigan. Accessed December 02, 2020. http://hdl.handle.net/2027.42/64690.

MLA Handbook (7th Edition):

Edmondson, Justin K. “Theory of Three-Dimensional Interchange Reconnection and the Dynamic Evolution of the Global Solar Coronal Magnetic Field Structure: A Mechanism for the Origin and Generation of the Slow Solar Wind.” 2009. Web. 02 Dec 2020.

Vancouver:

Edmondson JK. Theory of Three-Dimensional Interchange Reconnection and the Dynamic Evolution of the Global Solar Coronal Magnetic Field Structure: A Mechanism for the Origin and Generation of the Slow Solar Wind. [Internet] [Doctoral dissertation]. University of Michigan; 2009. [cited 2020 Dec 02]. Available from: http://hdl.handle.net/2027.42/64690.

Council of Science Editors:

Edmondson JK. Theory of Three-Dimensional Interchange Reconnection and the Dynamic Evolution of the Global Solar Coronal Magnetic Field Structure: A Mechanism for the Origin and Generation of the Slow Solar Wind. [Doctoral Dissertation]. University of Michigan; 2009. Available from: http://hdl.handle.net/2027.42/64690


University of Hawaii – Manoa

30. Armstrong, James D, 1970. Structure and energy transport of the solar convection zone.

Degree: PhD, 2009, University of Hawaii – Manoa

Also available by subscription via World Wide Web

xvi, 139 leaves, bound ill. 29 cm

Subjects/Keywords: Solar radiation; Solar radiation  – Mathematical models; Solar magnetic fields; Sunspots

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APA (6th Edition):

Armstrong, James D, 1. (2009). Structure and energy transport of the solar convection zone. (Doctoral Dissertation). University of Hawaii – Manoa. Retrieved from http://hdl.handle.net/10125/12102

Chicago Manual of Style (16th Edition):

Armstrong, James D, 1970. “Structure and energy transport of the solar convection zone.” 2009. Doctoral Dissertation, University of Hawaii – Manoa. Accessed December 02, 2020. http://hdl.handle.net/10125/12102.

MLA Handbook (7th Edition):

Armstrong, James D, 1970. “Structure and energy transport of the solar convection zone.” 2009. Web. 02 Dec 2020.

Vancouver:

Armstrong, James D 1. Structure and energy transport of the solar convection zone. [Internet] [Doctoral dissertation]. University of Hawaii – Manoa; 2009. [cited 2020 Dec 02]. Available from: http://hdl.handle.net/10125/12102.

Council of Science Editors:

Armstrong, James D 1. Structure and energy transport of the solar convection zone. [Doctoral Dissertation]. University of Hawaii – Manoa; 2009. Available from: http://hdl.handle.net/10125/12102

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