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You searched for subject:(Stellar Convection). Showing records 1 – 6 of 6 total matches.

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University of Colorado

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

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

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

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

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

APA (6th Edition):

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

Chicago Manual of Style (16th Edition):

Augustson, Kyle C. “Convection and Dynamo Action in Massive Stars.” 2013. Doctoral Dissertation, University of Colorado. Accessed January 17, 2021. https://scholar.colorado.edu/astr_gradetds/26.

MLA Handbook (7th Edition):

Augustson, Kyle C. “Convection and Dynamo Action in Massive Stars.” 2013. Web. 17 Jan 2021.

Vancouver:

Augustson KC. Convection and Dynamo Action in Massive Stars. [Internet] [Doctoral dissertation]. University of Colorado; 2013. [cited 2021 Jan 17]. Available from: https://scholar.colorado.edu/astr_gradetds/26.

Council of Science Editors:

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


Uppsala University

2. Bernadich, Miquel Colom i. Measuring the Characteristic Sizes of Convection Structures in AGB Stars with Fourier Decomposition Analyses : the Stellar Intensity Analyzer (SIA) Pipeline.

Degree: Theoretical Astrophysics, 2020, Uppsala University

  Context. Theoretical studies predict that the length scale of convection in stellar atmospheres isproportional to the pressure scale height, which implies that giant and… (more)

Subjects/Keywords: Asymptotic Giant Branch; AGB; red giants; stars; stellar convection; Fourier analysis; convection cells; Astronomy, Astrophysics and Cosmology; Astronomi, astrofysik och kosmologi

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APA (6th Edition):

Bernadich, M. C. i. (2020). Measuring the Characteristic Sizes of Convection Structures in AGB Stars with Fourier Decomposition Analyses : the Stellar Intensity Analyzer (SIA) Pipeline. (Thesis). Uppsala University. Retrieved from http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-414041

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):

Bernadich, Miquel Colom i. “Measuring the Characteristic Sizes of Convection Structures in AGB Stars with Fourier Decomposition Analyses : the Stellar Intensity Analyzer (SIA) Pipeline.” 2020. Thesis, Uppsala University. Accessed January 17, 2021. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-414041.

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

MLA Handbook (7th Edition):

Bernadich, Miquel Colom i. “Measuring the Characteristic Sizes of Convection Structures in AGB Stars with Fourier Decomposition Analyses : the Stellar Intensity Analyzer (SIA) Pipeline.” 2020. Web. 17 Jan 2021.

Vancouver:

Bernadich MCi. Measuring the Characteristic Sizes of Convection Structures in AGB Stars with Fourier Decomposition Analyses : the Stellar Intensity Analyzer (SIA) Pipeline. [Internet] [Thesis]. Uppsala University; 2020. [cited 2021 Jan 17]. Available from: http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-414041.

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

Council of Science Editors:

Bernadich MCi. Measuring the Characteristic Sizes of Convection Structures in AGB Stars with Fourier Decomposition Analyses : the Stellar Intensity Analyzer (SIA) Pipeline. [Thesis]. Uppsala University; 2020. Available from: http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-414041

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

3. Brown, Justin. The Effects of Small-Scale Mixing Processes on Supernova Progenitors.

Degree: Astronomy & Astrophysics, 2016, University of California – Santa Cruz

 Minor mixing processes—any fluid processes that mix material or transport heat other than convection or other large-scale flows—play a critical role in stellar evolution. These… (more)

Subjects/Keywords: Astronomy; Astrophysics; Applied mathematics; computational fluid dynamics; massive stars; overshooting convection; semiconvection; stellar evolution; thermohaline convection

…use stellar models with as accurate a treatment of semi-convection as possible. 1.3 1.3.1… …known as thermohaline convection) occurs in regions of stellar and planetary interiors… …combination of neutrinos and helium burning. Stellar winds of all models have been included… …in red. Convection is given by dense, black hashing; overshoot by sparse, gray hashing… …semi-convection by red crosshatching; and thermohaline convection by blue dots. The overshoot… 

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APA (6th Edition):

Brown, J. (2016). The Effects of Small-Scale Mixing Processes on Supernova Progenitors. (Thesis). University of California – Santa Cruz. Retrieved from http://www.escholarship.org/uc/item/7xf9x6vk

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):

Brown, Justin. “The Effects of Small-Scale Mixing Processes on Supernova Progenitors.” 2016. Thesis, University of California – Santa Cruz. Accessed January 17, 2021. http://www.escholarship.org/uc/item/7xf9x6vk.

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

MLA Handbook (7th Edition):

Brown, Justin. “The Effects of Small-Scale Mixing Processes on Supernova Progenitors.” 2016. Web. 17 Jan 2021.

Vancouver:

Brown J. The Effects of Small-Scale Mixing Processes on Supernova Progenitors. [Internet] [Thesis]. University of California – Santa Cruz; 2016. [cited 2021 Jan 17]. Available from: http://www.escholarship.org/uc/item/7xf9x6vk.

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

Council of Science Editors:

Brown J. The Effects of Small-Scale Mixing Processes on Supernova Progenitors. [Thesis]. University of California – Santa Cruz; 2016. Available from: http://www.escholarship.org/uc/item/7xf9x6vk

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


University of Vienna

4. Happenhofer, Natalie. Simulation of low Mach number fluids.

Degree: 2010, University of Vienna

In dieser Arbeit werden die Navier-Stokes Gleichungen für kompressible Fluide mittels eines von N. Kwatra et al. vorgeschlagenen Verfahren gelöst. Dieses Verfahren filtert effektiv Schallwellen,… (more)

Subjects/Keywords: 31.76 Numerische Mathematik; 31.45 Partielle Differentialgleichungen; 31.80 Angewandte Mathematik; 39.22 Astrophysik; Hyperbolisches Differentialgleichungssystem / Navier-Stokes Gleichungen / konservative numerische Verfahren / ENO-Verfahren / stellare Konvektion / doppelt-diffusive Konvektion; hyperbolic system of differential equations / Navier-Stokes equations / conservative numerical scheme / essentially-non-oscillatory scheme / fractional step method / stellar convection / double-diffusive convection

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

APA (6th Edition):

Happenhofer, N. (2010). Simulation of low Mach number fluids. (Thesis). University of Vienna. Retrieved from http://othes.univie.ac.at/10551/

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):

Happenhofer, Natalie. “Simulation of low Mach number fluids.” 2010. Thesis, University of Vienna. Accessed January 17, 2021. http://othes.univie.ac.at/10551/.

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

MLA Handbook (7th Edition):

Happenhofer, Natalie. “Simulation of low Mach number fluids.” 2010. Web. 17 Jan 2021.

Vancouver:

Happenhofer N. Simulation of low Mach number fluids. [Internet] [Thesis]. University of Vienna; 2010. [cited 2021 Jan 17]. Available from: http://othes.univie.ac.at/10551/.

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

Council of Science Editors:

Happenhofer N. Simulation of low Mach number fluids. [Thesis]. University of Vienna; 2010. Available from: http://othes.univie.ac.at/10551/

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


ETH Zürich

5. Ploner, Stefan R.O. Dynamics of the solar convection zone and atmosphere.

Degree: 1999, ETH Zürich

Subjects/Keywords: SONNENATMOSPHÄRE (ASTRONOMIE); KONVEKTION IN STERNEN (ASTRONOMIE); SOLAR ATMOSPHERE (ASTRONOMY); STELLAR CONVECTION (ASTRONOMY); info:eu-repo/classification/ddc/520; Astronomy, cartography

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APA (6th Edition):

Ploner, S. R. O. (1999). Dynamics of the solar convection zone and atmosphere. (Doctoral Dissertation). ETH Zürich. Retrieved from http://hdl.handle.net/20.500.11850/144118

Chicago Manual of Style (16th Edition):

Ploner, Stefan R O. “Dynamics of the solar convection zone and atmosphere.” 1999. Doctoral Dissertation, ETH Zürich. Accessed January 17, 2021. http://hdl.handle.net/20.500.11850/144118.

MLA Handbook (7th Edition):

Ploner, Stefan R O. “Dynamics of the solar convection zone and atmosphere.” 1999. Web. 17 Jan 2021.

Vancouver:

Ploner SRO. Dynamics of the solar convection zone and atmosphere. [Internet] [Doctoral dissertation]. ETH Zürich; 1999. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/20.500.11850/144118.

Council of Science Editors:

Ploner SRO. Dynamics of the solar convection zone and atmosphere. [Doctoral Dissertation]. ETH Zürich; 1999. Available from: http://hdl.handle.net/20.500.11850/144118

6. Sainsbury-Martinez, Felix. Flows, instabilities, and magnetism in stars and planets.

Degree: PhD, 2017, University of Exeter

 Flows, instabilities, and magnetism play significant roles in the internal and atmospheric dynamics of objects ranging from the smallest exoplanets to the largest stars. These… (more)

Subjects/Keywords: 530; Astrophysics; MHD; Instabilities; Fluid Dynamics; Stellar Physics; Exoplanets; Exoplanet Transits; Radial Velocities; Solar Corona; Solar Chromosphere; Convection; HD

convection. . . . . 6 1.2 Internal Structure of Stars Against Mass… …with streamfunction contours, and velocity streams for a ‘toybox’ Rayleigh-Bénard convection… …and velocity streams for a modified, and restricted, Rayleigh-Bénard convection model. 2.3… …to investigate the internal structure of a star via oscillation modes within the stellar… …of providing us, with a wealth of stellar data, over long periods, and with high signal to… 

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

APA (6th Edition):

Sainsbury-Martinez, F. (2017). Flows, instabilities, and magnetism in stars and planets. (Doctoral Dissertation). University of Exeter. Retrieved from http://hdl.handle.net/10871/32072

Chicago Manual of Style (16th Edition):

Sainsbury-Martinez, Felix. “Flows, instabilities, and magnetism in stars and planets.” 2017. Doctoral Dissertation, University of Exeter. Accessed January 17, 2021. http://hdl.handle.net/10871/32072.

MLA Handbook (7th Edition):

Sainsbury-Martinez, Felix. “Flows, instabilities, and magnetism in stars and planets.” 2017. Web. 17 Jan 2021.

Vancouver:

Sainsbury-Martinez F. Flows, instabilities, and magnetism in stars and planets. [Internet] [Doctoral dissertation]. University of Exeter; 2017. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/10871/32072.

Council of Science Editors:

Sainsbury-Martinez F. Flows, instabilities, and magnetism in stars and planets. [Doctoral Dissertation]. University of Exeter; 2017. Available from: http://hdl.handle.net/10871/32072

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