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Статті в журналах з теми "Earth's Magnetosheath"
Artemyev, A. V., C. Shi, Y. Lin, Y. Nishimura, C. Gonzalez, J. Verniero, X. Wang, M. Velli, A. Tenerani, and N. Sioulas. "Ion Kinetics of Plasma Flows: Earth's Magnetosheath versus Solar Wind." Astrophysical Journal 939, no. 2 (November 1, 2022): 85. http://dx.doi.org/10.3847/1538-4357/ac96e4.
Повний текст джерелаTurc, Lucile, Vertti Tarvus, Andrew P. Dimmock, Markus Battarbee, Urs Ganse, Andreas Johlander, Maxime Grandin, Yann Pfau-Kempf, Maxime Dubart, and Minna Palmroth. "Asymmetries in the Earth's dayside magnetosheath: results from global hybrid-Vlasov simulations." Annales Geophysicae 38, no. 5 (October 6, 2020): 1045–62. http://dx.doi.org/10.5194/angeo-38-1045-2020.
Повний текст джерелаLongmore, M., S. J. Schwartz, and E. A. Lucek. "Rotation of the magnetic field in Earth's magnetosheath by bulk magnetosheath plasma flow." Annales Geophysicae 24, no. 1 (March 7, 2006): 339–54. http://dx.doi.org/10.5194/angeo-24-339-2006.
Повний текст джерелаSong, P. "Forecasting Earth's magnetopause, magnetosheath, and bow shock." IEEE Transactions on Plasma Science 28, no. 6 (2000): 1966–75. http://dx.doi.org/10.1109/27.902225.
Повний текст джерелаWalsh, B. M., D. G. Sibeck, Y. Wang, and D. H. Fairfield. "Dawn-dusk asymmetries in the Earth's magnetosheath." Journal of Geophysical Research: Space Physics 117, A12 (December 2012): n/a. http://dx.doi.org/10.1029/2012ja018240.
Повний текст джерелаONSAGER, T. G., and M. F. THOMSEN. "The Earth's Foreshock, Bow Shock, and Magnetosheath." Reviews of Geophysics 29, S2 (January 1991): 998–1007. http://dx.doi.org/10.1002/rog.1991.29.s2.998.
Повний текст джерелаGuicking, L., K. H. Glassmeier, H. U. Auster, Y. Narita, and G. Kleindienst. "Low-frequency magnetic field fluctuations in Earth's plasma environment observed by THEMIS." Annales Geophysicae 30, no. 8 (August 27, 2012): 1271–83. http://dx.doi.org/10.5194/angeo-30-1271-2012.
Повний текст джерелаTurc, L., D. Fontaine, P. Savoini, and E. K. J. Kilpua. "Magnetic clouds' structure in the magnetosheath as observed by Cluster and Geotail: four case studies." Annales Geophysicae 32, no. 10 (October 15, 2014): 1247–61. http://dx.doi.org/10.5194/angeo-32-1247-2014.
Повний текст джерелаHou, Chuanpeng, Jiansen He, Die Duan, Xingyu Zhu, Wenya Li, Daniel Verscharen, Terry Liu, and Tieyan Wang. "Efficient Energy Conversion through Vortex Arrays in the Turbulent Magnetosheath." Astrophysical Journal 946, no. 1 (March 1, 2023): 13. http://dx.doi.org/10.3847/1538-4357/acb927.
Повний текст джерелаPaschalidis, N. P., S. M. Krimigis, E. T. Sarris, D. G. Sibeck, R. W. McEntire, S. P. Christon, and L. J. Zanetti. "Ion burst event in the Earth's dayside magnetosheath." Geophysical Research Letters 18, no. 3 (March 1991): 377–80. http://dx.doi.org/10.1029/91gl00140.
Повний текст джерелаДисертації з теми "Earth's Magnetosheath"
Archer, Martin. "Dynamic pressure pulses in Earth's dayside magnetosheath." Thesis, Imperial College London, 2014. http://hdl.handle.net/10044/1/24743.
Повний текст джерелаLongmore, Melissa Mary. "Cluster multi-spacecraft observations at the Earth's foreshock and a survey of Earth's magnetosheath." Thesis, Queen Mary, University of London, 2005. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.425338.
Повний текст джерелаConstantinescu, Ovidiu Dragoş. "Wave sources and structures in the Earth's magnetosheath and adjacent regions." Katlenburg-Lindau : Copernicus, 2007. http://d-nb.info/994457952/34.
Повний текст джерелаConstantinescu, Ovidiu Dragoş [Verfasser]. "Wave sources and structures in the Earth's magnetosheath and adjacent regions / von Ovidiu Dragoş Constantinescu." Katlenburg-Lindau : Copernicus GmbH, 2007. http://d-nb.info/994457952/34.
Повний текст джерелаg, Ufot Ekong Ufot. "Analysis of low frequency plasma waves in turbulent magnetosheath : downstream of the Earth's bow shock." Thesis, University of Sussex, 2011. http://sro.sussex.ac.uk/id/eprint/6324/.
Повний текст джерелаWallace, Aletta M. J. (Aletta Margaret Jensen). "Analysis of shock propagation in the magnetosheath." Thesis, Massachusetts Institute of Technology, 2003. http://hdl.handle.net/1721.1/114318.
Повний текст джерелаCataloged from PDF version of thesis.
Includes bibliographical references (pages 25-26).
Four interplanetary shock waves and disturbances are analyzed. Data recorded by multiple spacecraft are compared in order to determine how the speed of these events is modified when they cross Earth's bow shock into the magnetosheath. To accomplish this, it was necessary to find shocks that were seen by spacecraft both in the solar wind and inside the magnetosheath. Using a velocity coplanarity and a Rankine-Hugoniot methods of shock normal analysis, the speeds of these events in the solar wind were calculated. The time of their arrival at a spacecraft in the magnetosheath was determined. The predicted arrival time, assuming a constant shock speed from the spacecraft in the solar wind to the spacecraft in the magnetosheath is then compared to the actual arrival time. The resulting data support the conclusion that there is no change in the speed of the shock as it propagates through the magnetosheath.
by Aletta M. J. Wallace.
S.B. in Planetary Science and Astronomy
Grönlund, Arthur. "Statistical Survey of Earth’s Magnetopause Using MMS Data : Pressure Balance, Total Pressure Contributions and Magnetopause Velocity near the Subsolar Point, Dawn- and Dusk Flanks." Thesis, KTH, Skolan för elektroteknik och datavetenskap (EECS), 2021. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-295200.
Повний текст джерелаMagnetopausen är en viktig struktur i den jordnära rymden, där den ständigt utskickade solvinden från solen möter jordens magnetfält. Detta gränsområde mellan det så kallade magnetosheath på utsidan och magnetosfären på insidan är en diskontinuitet i ständig rörelse fram och tillbaka, upprätthållen av en tryckbalans på båda sidor, på vars yta en mycket viktig process för mass- och energitransport i universum sker kallad magnetisk rekonnektion. För att öka förståelsen för magnetopausen, har denna studie haft som mål att skapa ytterligare statistiskt material gällande diskontinuiteten. Detta inkluderar den totala tryckskillnaden över den, tryckvärden och deras bidrag till det totala trycket i magnetosheath och magnetosfären som gränsar den, samt magnetosfärens hastighet kopplat till tryckskillnaden över den. Detta gjordes genom analys av data från MMS-projektet, specifikt korsningar av magnetopausen i slutet av 2017 och under 2018 vid subsolar point och morgon- /kvällsflankerna. Om än resultaten visar på generellt sätt god överensstämmelse med tidigare studier, noterades en del intressanta resultat. Främst av dessa var en tydlig tendens för högre totalt tryck i magnetosheath jämfört med magnetosfären i alla undersökta regioner, samt ett oväntat skifte av dominerande tryck i magnetosfären från magnetiskt tryck vid subsolar point till termiskt tryck vid flankerna. Fortsatta studier för att bekräfta dessa resultat bör genomföras. Gällande magnetopaushastighet kopplat till tryckskillnad kunde ingen klar koppling ses från resultaten.
Hadid, Lina. "Observations in-situ de la turbulence compressible dans les magnétogaines planétaires et le vent solaire." Thesis, Université Paris-Saclay (ComUE), 2016. http://www.theses.fr/2016SACLS255/document.
Повний текст джерелаAmong the different astrophysical plasmas, the solar wind and the planetary magnetosheathsrepresent the best laboratories for studying the properties of fully developed plasma turbulence.Because of the relatively weak density fluctuations (∼ 10%) in the solar wind, the low frequencyfluctuations are usually described using the incompressible MHD theory. Nevertheless, the effectof the compressibility (in particular in the fast wind) has been a subject of active research withinthe space physics community over the last three decades.My thesis is essentially dedicated to the study of compressible turbulence in different plasma environments,the planetary magnetosheaths (of Saturn and Earth) and the fast and slow solar wind.This was done using in-situ spacecraft data from the Cassini, Cluster and THEMIS/ARTEMISsatellites.I first investigated the properties of MHD and kinetic scale turbulence in the magnetosheathof Saturn using Cassini data at the MHD scales and compared them to known features of thesolar wind turbulence. This work was completed with a more detailed analysis performed in themagnetosheath of Earth using the Cluster data. Then, by applying the recently derived exactlaw of compressible isothermal MHD turbulence to the in-situ observations from THEMIS andCLUSTER spacecrafts, a detailed study regarding the effect of the compressibility on the energycascade (dissipation) rate in the fast and the slow wind is presented. Several new empirical lawsare obtained, which include the power-law scaling of the energy cascade rate as function of theturbulent Mach number. Eventually, an application of this exact model to a more compressiblemedium, the magnetosheath of Earth, using the Cluster data provides the first estimation of theenergy dissipation rate in the magnetosheath, which is found to be up to two orders of magnitudehigher than that observed in the solar wind
Jelínek, Karel. "Dynamika okolozemní rázové vlny a magnetopauzy." Doctoral thesis, 2012. http://www.nusl.cz/ntk/nusl-309848.
Повний текст джерелаКниги з теми "Earth's Magnetosheath"
United States. National Aeronautics and Space Administration., ed. Origins of energetic ions in the earth's magnetosheath. [Washington, DC: National Aeronautics and Space Administration, 1994.
Знайти повний текст джерелаUnited States. National Aeronautics and Space Administration., ed. Origins of energetic ions in the earth's magnetosheath. [Washington, DC: National Aeronautics and Space Administration, 1994.
Знайти повний текст джерелаUnited States. National Aeronautics and Space Administration., ed. Origins of energetic ions in the Earth's magnetosheath: Final report for contract year 1. Palo Alto, Calif: Lockheed Palo Alto Research Laboratory, 1992.
Знайти повний текст джерелаUnited States. National Aeronautics and Space Administration., ed. Origins of energetic ions in the Earth's magnetosheath: Final report for contract year 1. Palo Alto, Calif: Lockheed Palo Alto Research Laboratory, 1992.
Знайти повний текст джерелаL, Grabbe Crockett, and United States. National Aeronautics and Space Administration., eds. Towards an MHD theory for the standoff distance of earth's bow shock. [Washington, DC: National Aeronautics and Space Administration, 1997.
Знайти повний текст джерелаUnited States. National Aeronautics and Space Administration., ed. "Studies of magnetopause structure": Final report for NAGW-1054. [Washington, DC: National Aeronautics and Space Administration, 1991.
Знайти повний текст джерелаUnited States. National Aeronautics and Space Administration., ed. "Studies of magnetopause structure": Final report for NAGW-1054. [Washington, DC: National Aeronautics and Space Administration, 1991.
Знайти повний текст джерелаW, Greenstadt Eugene, Coroniti Ferdinand V, and United States. National Aeronautics and Space Administration., eds. Flank solar wind interaction: Final report July 1991 through June 1994. [Washington, DC]: National Aeronautics and Space Administration, 1994.
Знайти повний текст джерелаW, Greenstadt Eugene, Coroniti Ferdinand V, and United States. National Aeronautics and Space Administration., eds. Flank solar wind interaction: Final report July 1991 through June 1994. [Washington, DC]: National Aeronautics and Space Administration, 1994.
Знайти повний текст джерелаW, Greenstadt Eugene, and United States. National Aeronautics and Space Administration., eds. Flank solar wind interaction: Annual report, June 1991 through July 1992. Redondo Beach, CA: TRW Space and Technology Group, Applied Technology Division, 1992.
Знайти повний текст джерелаЧастини книг з теми "Earth's Magnetosheath"
Dimmock, A. P., K. Nykyri, A. Osmane, H. Karimabadi, and T. I. Pulkkinen. "Dawn-Dusk Asymmetries of the Earth's Dayside Magnetosheath in the Magnetosheath Interplanetary Medium Reference Frame." In Dawn-Dusk Asymmetries in Planetary Plasma Environments, 49–72. Hoboken, NJ, USA: John Wiley & Sons, Inc., 2017. http://dx.doi.org/10.1002/9781119216346.ch5.
Повний текст джерелаNewell, Patrick T., and Ching-I. Meng. "Magnetosheath injections deep inside the closed LLBL: A review of observations." In Earth's Low-Latitude Boundary Layer, 149–56. Washington, D. C.: American Geophysical Union, 2003. http://dx.doi.org/10.1029/133gm15.
Повний текст джерелаDenton, Richard E., Brian J. Anderson, Stephen A. Fuselier, S. Peter Gary, and Mary K. Hudson. "Ion Anisotropy-driven waves in the Earth's magnetosheath and plasma depletion layer." In Solar System Plasmas in Space and Time, 111–19. Washington, D. C.: American Geophysical Union, 1994. http://dx.doi.org/10.1029/gm084p0111.
Повний текст джерелаYamauchi, M., R. Lundin, O. Norberg, I. Sandahl, L. Eliasson, and D. Winningham. "Signatures of direct magnetosheath plasma injections onto closed field-line regions based on observations at mid- and low-altitudes." In Earth's Low-Latitude Boundary Layer, 179–88. Washington, D. C.: American Geophysical Union, 2003. http://dx.doi.org/10.1029/133gm18.
Повний текст джерелаØieroset, Marit, David L. Mitchell, Tai D. Phan, Robert P. Lin, Dana H. Crider, and Mario H. Acuña. "The Magnetic Field Pile-Up and Density Depletion in the Martian Magnetosheath: A Comparison with the Plasma Depletion Layer Upstream of the Earth’s Magnetopause." In Mars’ Magnetism and Its Interaction with the Solar Wind, 185–202. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-0-306-48604-3_4.
Повний текст джерелаGÉNOT, V., E. BUDNIK, C. JACQUEY, I. DANDOURAS, and E. LUCEK. "MIRROR MODES OBSERVED WITH CLUSTER IN THE EARTH'S MAGNETOSHEATH: STATISTICAL STUDY AND IMF/SOLAR WIND DEPENDENCE." In Advances in Geosciences, 263–83. World Scientific Publishing Company, 2009. http://dx.doi.org/10.1142/9789812836205_0019.
Повний текст джерелаТези доповідей конференцій з теми "Earth's Magnetosheath"
Robertson, Ina P., Thomas E. Cravens, Michael R. Collier, David G. Sibeck, Kip D. Kuntz, and Steven L. Snowden. "Solar wind charge exchange and Earth's magnetosheath." In SOLAR WIND 13: Proceedings of the Thirteenth International Solar Wind Conference. AIP, 2013. http://dx.doi.org/10.1063/1.4811077.
Повний текст джерелаTawfik, A., M. A. Amer, O. M. Shalabiea, and M. S. El-Nawawy. "The Periodicity of the Alfven Mode Waves in the Earth’s Magnetosheath." In MODERN TRENDS IN PHYSICS RESEARCH: Second International Conference on Modern Trends in Physics Research MTPR-06. AIP, 2007. http://dx.doi.org/10.1063/1.2711133.
Повний текст джерелаLewis, H. R., X. Li, J. LaBelle, T. D. Phan, and R. A. Treumann. "Characteristics of the ion pressure tensor in the earth’s magnetosheath: AMPTE/IRM observations." In International conference on plasma physics ICPP 1994. AIP, 1995. http://dx.doi.org/10.1063/1.49000.
Повний текст джерелаBreneman, A. W., C. A. Cattell, K. Kersten, A. Paradise, S. Schreiner, P. J. Kellogg, K. Goetz, and L. B. Wilson. "STEREO and wind observations of intense electron cyclotron harmonic waves at the earths bow shock and inside the magnetosheath." In 2014 XXXIth URSI General Assembly and Scientific Symposium (URSI GASS). IEEE, 2014. http://dx.doi.org/10.1109/ursigass.2014.6929903.
Повний текст джерелаЗвіти організацій з теми "Earth's Magnetosheath"
Chang, S. W., J. D. Scudder, J. F. Fennell, R. Friedel, and R. P. Lepping. Energetic Magnetosheath Ions Connected to the Earth's Bow Shock: Possible Source of CEPs. Fort Belvoir, VA: Defense Technical Information Center, December 2001. http://dx.doi.org/10.21236/ada399602.
Повний текст джерелаBranduardi-Raymont, Graziella, and et al. SMILE Definition Study Report. ESA SCI, December 2018. http://dx.doi.org/10.5270/esa.smile.definition_study_report-2018-12.
Повний текст джерела