Relevant bibliographies by topics / Planetary magnetic fields

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers

Academic literature on the topic 'Planetary magnetic fields'

Author: Grafiati
Published: 4 June 2021
Last updated: 25 July 2025

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Journal articles on the topic "Planetary magnetic fields"

1

Stevenson, David J. "Planetary magnetic fields." Earth and Planetary Science Letters 208, no. 1-2 (2003): 1–11. http://dx.doi.org/10.1016/s0012-821x(02)01126-3.

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Hamouda, Samir Ahmed, Nada Eaz-Alden Emgau, Rabab Muftah Bohagar, and Aisha Mohammed Eissa. "STUDY OF PLANETARY MAGNETIC FIELDS." International Journal of Research -GRANTHAALAYAH 5, no. 3 (2017): 29–44. http://dx.doi.org/10.29121/granthaalayah.v5.i3.2017.1752.

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Magnetic fields are an important phenomenon in the solar system and beyond. Their causes are complex and have a variety of effects on their surroundings; they have become a critical tool for the exploration of solar system bodies. Magnetic fields play a very important role in the Sun. From sunspots to coronal heating, from solar ares to coronal mass ejections all these apparently diverse phenomena have magnetic fields as their ultimate cause. The study of the terrestrial dynamo is a difficult problem made more so by the inability to construct planetary-scale dynamos for laboratory study. Howev
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Samir, Ahmed Hamouda, Eaz-Alden Emgau Nada, Muftah Bohagar Rabab, and Mohammed Eissa Aisha. "STUDY OF PLANETARY MAGNETIC FIELDS." International Journal of Research -GRANTHAALAYAH 5, no. 3 (2017): 29–44. https://doi.org/10.5281/zenodo.439552.

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Magnetic fields are an important phenomenon in the solar system and beyond. Their causes are complex and have a variety of effects on their surroundings; they have become a critical tool for the exploration of solar system bodies. Magnetic fields play a very important role in the Sun. From sunspots to coronal heating, from solar ares to coronal mass ejections all these apparently diverse phenomena have magnetic fields as their ultimate cause. The study of the terrestrial dynamo is a difficult problem made more so by the inability to construct planetary-scale dynamos for laboratory study. Howev
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Sabin, L., Q. Zhang, A. A. Zijlstra, et al. "Magnetic fields in Proto Planetary Nebulae." Proceedings of the International Astronomical Union 9, S302 (2013): 398–99. http://dx.doi.org/10.1017/s1743921314002592.

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AbstractThe role of magnetic field in late type stars such as proto-planetary and planetary nebulae (PPNe/PNe), is poorly known from an observational point of view. We present submillimetric observations realized with the Submillimeter Array (SMA) which unveil the dust continuum polarization in the envelopes of two well known PPNe: CRL 618 and OH 231.8+4.2. Assuming the current grain alignment theory, we were then able to trace the geometry of the magnetic field.
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Smith, Andy. "Terrestrial, planetary and interplanetary magnetic fields." Astronomy and Geophysics 41, no. 3 (2000): 3.32–3.33. http://dx.doi.org/10.1046/j.1468-4004.2000.00332.x.

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Schubert, G., and K. M. Soderlund. "Planetary magnetic fields: Observations and models." Physics of the Earth and Planetary Interiors 187, no. 3-4 (2011): 92–108. http://dx.doi.org/10.1016/j.pepi.2011.05.013.

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Stevenson, David J. "Planetary Magnetic Fields: Achievements and Prospects." Space Science Reviews 152, no. 1-4 (2009): 651–64. http://dx.doi.org/10.1007/s11214-009-9572-z.

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Jones, Chris A. "Planetary Magnetic Fields and Fluid Dynamos." Annual Review of Fluid Mechanics 43, no. 1 (2011): 583–614. http://dx.doi.org/10.1146/annurev-fluid-122109-160727.

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Greaves, J. S. "Toroidal magnetic fields around planetary nebulae." Astronomy & Astrophysics 392, no. 1 (2002): L1—L4. http://dx.doi.org/10.1051/0004-6361:20021002.

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Schulz, Michael, and George A. Paulikas. "Planetary magnetic fields: A comparative view." Advances in Space Research 10, no. 1 (1990): 55–64. http://dx.doi.org/10.1016/0273-1177(90)90086-f.

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Dissertations / Theses on the topic "Planetary magnetic fields"

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Fu, Roger R. (Roger Rennan). "Magnetic fields in the early solar system." Thesis, Massachusetts Institute of Technology, 2015. http://hdl.handle.net/1721.1/101348.

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Thesis: Ph. D., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, 2015.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references (pages 251-283).<br>The first magnetic fields in the solar system were embedded in the ionized gas of the protoplanetary disk itself. Soon after, newly formed protoplanets may have harbored magnetic core dynamos. Paleomagnetic analysis of ancient samples permits direct constraints on these early solar system magnetic fields. Here I present paleomagnetic studies of several classes of meteorites. Exp
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Sun, Peng, and Peng Sun. "Charged-Particle Transport in Turbulent Magnetic Fields." Diss., The University of Arizona, 2016. http://hdl.handle.net/10150/621573.

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Collisionless turbulence is common in astrophysical magnetic fields and plasmas. The determination of the transport of high-energy charged particles both parallel and perpendicular to the average magnetic field in such a system is of considerable interest. It is recognized that the turbulent magnetic field has important effects on the transport of charged particles and that the properties of different turbulence models may significantly affect the resulting transport properties. A number of different magnetic turbulence models have been proposed in the last several decades. We present here the
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Knapp, Mary (Mary E. ). "Toward detection and characterization of exoplanetary magnetic fields via low frequency radio observation." Thesis, Massachusetts Institute of Technology, 2018. http://hdl.handle.net/1721.1/115642.

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Thesis: Ph. D. in Planetary Sciences, Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, 2018.<br>This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.<br>Cataloged from student-submitted PDF version of thesis.<br>Includes bibliographical references (pages 225-256).<br>Low frequency radio emission from planets is produced by the interaction of energetic charged particles from the planet's ionosphere and/or the solar wind with the planet's magnetic field. Th
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de, Lima Leal Ferreira Marcelo [Verfasser]. "Magnetic Fields and the Formation of Aspherical Planetary Nebulae / Marcelo de Lima Leal Ferreira." Bonn : Universitäts- und Landesbibliothek Bonn, 2015. http://d-nb.info/1077289383/34.

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Rees, Bryan. "A study of planetary nebulae in and towards the Galactic Bulge." Thesis, University of Manchester, 2011. https://www.research.manchester.ac.uk/portal/en/theses/a-study-of-planetary-nebulae-in-and-towards-the-galactic-bulge(ff6c0373-e5a5-491f-b5fb-bda36acac8ba).html.

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A planetary nebula (PN) consists of material, mainly gas, that has been ejected from a star on the asymptotic giant branch of its life cycle. This material emits electromagnetic radiation due to photoionization and recombination, collisional and radiative excitation or free-free radiation. The envelope of material moves outwards from the central star and may take one of a variety of shapes. These shapes are believed to be sculpted by the stellar wind, magnetic fields and interactions with a binary companion. However, within a time scale of as little as 10 000 years the nebula fades from view a
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Schad, Thomas Anthony. "Spectropolarimetry of Fine Magnetized Structures in the Upper Solar Atmosphere." Diss., The University of Arizona, 2013. http://hdl.handle.net/10150/301683.

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One of the earliest indications of magnetic fields acting in the solar atmosphere came at the beginning of the 20th century when George Hale noted a "decided definiteness of structure" in photographs within the Hydrogen Balmer-alpha line core. Fine structure both in the chromosphere and in the corona result from processes that are not well understood but accepted as a consequence of the solar magnetic field. Our knowledge of this field is lacking, and until recently, the assumed relationship between fine thermal structure and the magnetic field remained untested. Here, spectropolarimetric dia
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Guo, Fan. "Effects of Turbulent Magnetic Fields on the Transport and Acceleration of Energetic Charged Particles: Numerical Simulations with Application to Heliospheric Physics." Diss., The University of Arizona, 2012. http://hdl.handle.net/10150/255156.

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Turbulent magnetic fields are ubiquitous in space physics and astrophysics. The influence of magnetic turbulence on the motions of charged particles contains the essential physics of the transport and acceleration of energetic charged particles in the heliosphere, which is to be explored in this thesis. After a brief introduction on the energetic charged particles and magnetic fields in the heliosphere, the rest of this dissertation focuses on three specific topics: 1. the transport of energetic charged particles in the inner heliosphere, 2. the acceleration of ions at collisionless shocks, an
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Yu, Louise. "Recherche de Jupiters chauds autour d'étoiles jeunes." Thesis, Toulouse 3, 2019. http://www.theses.fr/2019TOU30240.

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Les 25 dernières années ont vu la détection d'environ 400 Jupiters chauds (hJs), exoplanètes géantes semblables à Jupiter mais sur des orbites cent fois plus resserrées. Ces planètes étonnantes se seraient formées loin de leur étoile avant de migrer vers elle, cependant les processus physiques à l'origine de ce transfert orbital sont encore peu contraints par les observations. Cette question, essentielle à notre compréhension de la formation des systèmes planétaires, a de profondes répercussions sur l'architecture de ces systèmes, et en particulier sur la probabilité de former des planètes tel
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Dimmock, Andrew. "The study of magnetic and electric field structures at planetary magnetospheres." Thesis, University of Sheffield, 2012. http://etheses.whiterose.ac.uk/2679/.

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Aveiro, Henrique Carlotto. "Electric and magnetic field signatures of gravity waves and 2-day planetary waves in the equatorial E-region." Instituto Nacional de Pesquisas Espaciais, 2009. http://urlib.net/sid.inpe.br/mtc-m18@80/2008/12.16.11.31.

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Observações do eletrojato equatorial (EEJ) utilizando radares VHF mostram ecos retro-espalhados em dois tipos de irregularidades de densidade eletrônica, explicadas pelas instabilidades de dois-feixes modificada (ecos Tipo I) e deriva de gradiente (ecos Tipo II). Das velocidades das irregularidades Tipo II obtidas de dados de radar, inferimos os campos elétricos verticais (E_z). A análise harmônica de tais campos mostra a presença de campos elétricos induzidos por ondas de gravidade (GW) no EEJ. Calculamos a razão entre os campos elétricos relacionados a GW e o campo elétrico vertical total. E
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Books on the topic "Planetary magnetic fields"

1

Summer Study Program in Geophysical Fluid Dynamics (1988 Woods Hole Oceanographic Institution). Order and disorder in planetary dynamos. Woods Hole Oceanographic Institution, 1988.

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Space Environment Center (U.S.), ed. Wang and Sheeley medium-range planetary A index forecast verification statistics. U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Center, 1996.

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Space Environment Center (U.S.), ed. Wang and Sheeley medium-range planetary A index forecast verification statistics. U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Center, 1996.

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Space Environment Center (U.S.), ed. Wang and Sheeley medium-range planetary A index forecast verification statistics. U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Center, 1996.

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Space Environment Center (U.S.), ed. Wang and Sheeley medium-range planetary A index forecast verification statistics. U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Center, 1996.

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Space Environment Center (U.S.), ed. Wang and Sheeley medium-range planetary A index forecast verification statistics. U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Center, 1996.

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Evans, D. R. Non-dipolar magnetic field models and patterns of radio emission: Uranus and Neptune compared : final report. National Aeronautics and Space Administration, 1994.

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United States. National Aeronautics and Space Administration., ed. Non-dipolar magnetic field models and patterns of radio emission: Uranus and Neptune compared : final report. National Aeronautics and Space Administration, 1994.

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United States. National Aeronautics and Space Administration., ed. Non-dipolar magnetic field models and patterns of radio emission: Uranus and Neptune compared : final report. National Aeronautics and Space Administration, 1994.

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L, Kaufmann Richard, and United States. National Aeronautics and Space Administration., eds. Force balance and substorm effects in the magnetotail. National Aeronautics and Space Administration, 1997.

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Book chapters on the topic "Planetary magnetic fields"

1

Bagenal, Frances. "Planetary Magnetospheres." In Solar System Magnetic Fields. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5482-3_9.

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Stevenson, David J. "Planetary Magnetic Fields: Achievements and Prospects." In Planetary Magnetism. Springer New York, 2009. http://dx.doi.org/10.1007/978-1-4419-5901-0_20.

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Langlais, Benoit, Vincent Lesur, Michael E. Purucker, Jack E. P. Connerney, and Mioara Mandea. "Crustal Magnetic Fields of Terrestrial Planets." In Planetary Magnetism. Springer New York, 2009. http://dx.doi.org/10.1007/978-1-4419-5901-0_7.

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Russell, C. T., and M. K. Dougherty. "Magnetic Fields of the Outer Planets." In Planetary Magnetism. Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-5901-0_8.

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Saur, Joachim, Fritz M. Neubauer, and Karl-Heinz Glassmeier. "Induced Magnetic Fields in Solar System Bodies." In Planetary Magnetism. Springer New York, 2009. http://dx.doi.org/10.1007/978-1-4419-5901-0_12.

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Gurzadyan, Grigor A. "Magnetic Fields in Planetary Nebulae." In Astronomy and Astrophysics Library. Springer Berlin Heidelberg, 1997. http://dx.doi.org/10.1007/978-3-662-03448-4_17.

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Jia, Xianzhe, Margaret G. Kivelson, Krishan K. Khurana, and Raymond J. Walker. "Magnetic Fields of the Satellites of Jupiter and Saturn." In Planetary Magnetism. Springer New York, 2009. http://dx.doi.org/10.1007/978-1-4419-5901-0_9.

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Driscoll, Peter E. "Planetary Interiors, Magnetic Fields, and Habitability." In Handbook of Exoplanets. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-30648-3_76-1.

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Driscoll, Peter E. "Planetary Interiors, Magnetic Fields, and Habitability." In Handbook of Exoplanets. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-55333-7_76.

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Roberge, Wayne G., and Glenn E. Ciolek. "Magnetic Fields and Planetary Systems Formation." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_986-4.

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Conference papers on the topic "Planetary magnetic fields"

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Asimopolos, Laurentiu, Natalia-Silvia Asimopolos, Vijdea Anca-Marina, Dinu Luminita, and Adrian-Aristide Asimopolos. "ANALYSIS OF GEOMAGNETIC DATABASES IMPACTING SPACE WEATHER." In SGEM International Multidisciplinary Scientific GeoConference 24. STEF92 Technology, 2024. https://doi.org/10.5593/sgem2024/6.1/s28.63.

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Through the complex analysis of the geomagnetic database of the Surlari Geomagnetic Observatory for over 80 years, corroborated with the data of other planetary observatories from the INTERMAGNET network, we have extracted the geomagnetic information that is correlated with the specific physical parameters of space weather domain. Space weather refers to the conditions and phenomena occurring in outer space that can influence the near-Earth space environment. This concept includes a variety of events and conditions that occur outside the Earth's atmosphere and can affect various aspects of spa
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García-Segura, Guillermo. "The Structuring of Planetary Nebulae." In MAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures. AIP, 2005. http://dx.doi.org/10.1063/1.2077187.

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Soker, Noam. "Can We Ignore Magnetic Fields in Studies of PN Formation, Shaping and Interaction with the ISM?" In PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools. AIP, 2005. http://dx.doi.org/10.1063/1.2146238.

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Crawford, David A. "Simulations of Magnetic Fields Produced by Asteroid Impact: Possible Implications for Planetary Paleomagnetism." In 2019 15th Hypervelocity Impact Symposium. American Society of Mechanical Engineers, 2019. http://dx.doi.org/10.1115/hvis2019-032.

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Abstract The origin and evolution of the Moon's magnetic field has been a major question in lunar science ever since Luna 1 made the first magnetic measurements in the vicinity of the Moon in 1959. Orbital measurements show that the magnetic field at the surface of the Moon has local scale lengths on the order of 1-100 km. While this could suggest a correlation with impact craters, most lunar magnetic anomalies don’t appear to correlate with known geologic structures, including impacts [1]. However, the magnetic field produced by impact events are spatially and temporally complex. Add in the c
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Ramakrishnan, Gowtham Raj. "Analytical Calculation to Optimize Magnetic Planetary Gear Topology to Avoid Auto Slip during Various Torque Requirements for Passenger Car Application." In Symposium on International Automotive Technology. SAE International, 2024. http://dx.doi.org/10.4271/2024-26-0041.

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&lt;div class="section abstract"&gt;&lt;div class="htmlview paragraph"&gt;The automotive industry has recently started implementing magnetic gears, in different types, as an alternative design for transmission systems. One such design being the Magnetic planetary gear permanent magnet (MPG-PM) machine. The current methodology and the relevant formulae help to design the magnetic planetary gear system, which does not have design considerations for permanent magnet machines and the influence of magnetic fields. The influence of design characteristics of PM machine, Magnetic field and its materia
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Junge, A., A. Przyklenk, H. U. Auster, D. Heyner, L. A. D'Arcio, and K. Kempkens. "On-ground measurements of time-varying magnetic fields on board BepiColombo's mercury planetary orbiter spacecraft from a solar array drive mechansim." In 2016 ESA Workshop on Aerospace EMC (Aerospace EMC). IEEE, 2016. http://dx.doi.org/10.1109/aeroemc.2016.7504543.

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Kim, Changsung Sean, Jongpa Hong, Jihye Shim, et al. "Numerical and Experimental Study on Metal Organic Vapor Phase Epitaxy of InGaN/GaN Multi Quantum Wells." In ASME/JSME 2007 5th Joint Fluids Engineering Conference. ASMEDC, 2007. http://dx.doi.org/10.1115/fedsm2007-37115.

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A numerical and experimental study has been performed to characterize the metal organic vapor phase epitaxy (MOVPE) growth of InGaN/GaN multi-quantum wells (MQW). One of the major objectives of the present study is to predict the optimal operating conditions that would be suitable for the fabrication of GaN-based light-emitting diodes (LED) using three different reactors, vertical, horizontal and planetary. Computational fluids dynamic (CFD) simulations considering gas phase chemical reactions and surface chemistry were carried out and compared with experimental measurements. Through a lot of
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Yasnov, L. V. "Coronal Magnetic Field Structure in Solar Active Regions." In Planetary Radio Emissions VII. Austrian Academy of Sciences Press, 2011. http://dx.doi.org/10.1553/pre7s455.

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Huggins, P. J. "Signatures of the Magnetic Field Structure in PNe." In PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools. AIP, 2005. http://dx.doi.org/10.1063/1.2146237.

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"Generation of Auroral Kilometric Radiation in a dipole magnetic field: 3-D approach." In Planetary Radio Emissions VIII. Austrian Academy of Sciences Press, 2018. http://dx.doi.org/10.1553/pre8s261.

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