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Relevant bibliographies by topics / Magnetospheric magnetic field

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Academic literature on the topic 'Magnetospheric magnetic field'

Author: Grafiati

Published: 6 September 2023

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Journal articles on the topic "Magnetospheric magnetic field"

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Pensionerov, Ivan A., Elena S. Belenkaya, Stanley W. H. Cowley, Igor I. Alexeev, Vladimir V. Kalegaev, and David A. Parunakian. "Magnetodisc modelling in Jupiter's magnetosphere using Juno magnetic field data and the paraboloid magnetic field model." Annales Geophysicae 37, no. 1 (2019): 101–9. http://dx.doi.org/10.5194/angeo-37-101-2019.

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Abstract. One of the main features of Jupiter's magnetosphere is its equatorial magnetodisc, which significantly increases the field strength and size of the magnetosphere. Analysis of Juno measurements of the magnetic field during the first 10 orbits covering the dawn to pre-dawn sector of the magnetosphere (∼03:30–06:00 local time) has allowed us to determine optimal parameters of the magnetodisc using the paraboloid magnetospheric magnetic field model, which employs analytic expressions for the magnetospheric current systems. Specifically, within the model we determine the size of the Jovia

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Paty, Carol, Chris S. Arridge, Ian J. Cohen, Gina A. DiBraccio, Robert W. Ebert, and Abigail M. Rymer. "Ice giant magnetospheres." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 378, no. 2187 (2020): 20190480. http://dx.doi.org/10.1098/rsta.2019.0480.

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The ice giant planets provide some of the most interesting natural laboratories for studying the influence of large obliquities, rapid rotation, highly asymmetric magnetic fields and wide-ranging Alfvénic and sonic Mach numbers on magnetospheric processes. The geometries of the solar wind–magnetosphere interaction at the ice giants vary dramatically on diurnal timescales due to the large tilt of the magnetic axis relative to each planet's rotational axis and the apparent off-centred nature of the magnetic field. There is also a seasonal effect on this interaction geometry due to the large obli

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Alexeev, I. I., and E. S. Belenkaya. "Modeling of the Jovian Magnetosphere." Annales Geophysicae 23, no. 3 (2005): 809–26. http://dx.doi.org/10.5194/angeo-23-809-2005.

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Abstract. This paper presents a global model of the Jovian magnetosphere which is valid not only in the equatorial plane and near the planet, as most of the existing models are, but also at high latitudes and in the outer regions of the magnetosphere. The model includes the Jovian dipole, magnetodisc, and tail current system. The tail currents are combined with the magnetopause closure currents. All inner magnetospheric magnetic field sources are screened by the magnetopause currents. It guarantees a zero normal magnetic field component for the inner magnetospheric field at the whole magnetopa

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Kalegaev, Vladimir V., Natalia A. Vlasova, Ilya S. Nazarkov, and Sophia A. Melkova. "Magnetospheric access for solar protons during the January 2005 SEP event." Journal of Space Weather and Space Climate 8 (2018): A55. http://dx.doi.org/10.1051/swsc/2018040.

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The early phase of the extraordinary solar energetic particle 20 January, 2005 event having the highest peak flux of any SEP in the past 50 years of protons with energies > 100 MeV is studied. Solar energetic particles (>16 MeV) entry to the Earth’s magnetosphere on January 20, 2005 under northward interplanetary magnetic field conditions is considered based on multi-satellite data analysis and magnetic field simulation. Solar wind parameters and interplanetary magnetic field data, as well as calculations in terms of the A2000 magnetospheric magnetic field model were used to specify cond

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Krtička, J., Z. Mikulášek, P. Kurfürst, and M. E. Oksala. "Photometric signatures of corotating magnetospheres of hot stars governed by higher-order magnetic multipoles." Astronomy & Astrophysics 659 (March 2022): A37. http://dx.doi.org/10.1051/0004-6361/202141997.

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Context. The light curves of magnetic, chemically peculiar stars typically show periodic variability due to surface spots that in most cases can be modeled by low-order harmonic expansion. However, high-precision satellite photometry reveals tiny complex features in the light curves of some of these stars that are difficult to explain as caused by a surface phenomenon under reasonable assumptions. These features might originate from light extinction in corotating magnetospheric clouds supported by a complex magnetic field dominated by higher-order multipoles. Aims. We aim to understand the pho

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Jasinski, Jamie M., Neil Murphy, Xianzhe Jia, and James A. Slavin. "Neptune’s Pole-on Magnetosphere: Dayside Reconnection Observations by Voyager 2." Planetary Science Journal 3, no. 4 (2022): 76. http://dx.doi.org/10.3847/psj/ac5967.

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Abstract The “pole-on” configuration occurs when the polar magnetosphere of a planet is directed into the solar wind velocity vector. Such magnetospheric configurations are unique to the ice giant planets. This means that magnetic reconnection, a process that couples a magnetosphere to the solar wind, will be different at the ice giants when they are pole-on compared to other planets. The only available in situ measurements of a pole-on magnetosphere are from the Neptune flyby by Voyager 2, which we analyze in this paper. We show that dayside magnetopause conditions were conducive to magnetic

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Peymirat, C., and D. Fontaine. "A numerical method to compute Euler potentials for non dipolar magnetic fields." Annales Geophysicae 17, no. 3 (1999): 328–37. http://dx.doi.org/10.1007/s00585-999-0328-6.

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Abstract. The magnetospheric magnetic field may be conveniently described by two scalar functions (α, β), known as the Euler potentials. They are not uniquely defined, and they may be difficult to derive for configuration more complex than a simple dipole. We propose here a simple numerical method to compute one possible pair (α, β). In magnetospheric regions of closed field lines, α can be chosen as a function of the tube volume of unit magnetic flux. The method can be applied to a wide class of magnetic fields which describe the magnetospheric domain of closed field lines and the conjugated

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Zaharia, S., C. Z. Cheng, and K. Maezawa. "3-D force-balanced magnetospheric configurations." Annales Geophysicae 22, no. 1 (2004): 251–65. http://dx.doi.org/10.5194/angeo-22-251-2004.

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Abstract. The knowledge of plasma pressure is essential for many physics applications in the magnetosphere, such as computing magnetospheric currents and deriving mag-netosphere-ionosphere coupling. A thorough knowledge of the 3-D pressure distribution has, however, eluded the community, as most in situ pressure observations are either in the ionosphere or the equatorial region of the magnetosphere. With the assumption of pressure isotropy there have been attempts to obtain the pressure at different locations,by either (a) mapping observed data (e.g. in the ionosphere) along the field lines of

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Vaisberg, O. L., L. A. Avanov, T. E. Moore, and V. N. Smirnov. "Ion velocity distributions within the LLBL and their possible implication to multiple reconnections." Annales Geophysicae 22, no. 1 (2004): 213–36. http://dx.doi.org/10.5194/angeo-22-213-2004.

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Abstract. We analyze two LLBL crossings made by the Interball-Tail satellite under a southward or variable magnetosheath magnetic field: one crossing on the flank of the magnetosphere, and another one closer to the subsolar point. Three different types of ion velocity distributions within the LLBL are observed: (a) D-shaped distributions, (b) ion velocity distributions consisting of two counter-streaming components of magnetosheath-type, and (c) distributions with three components, one of which has nearly zero parallel velocity and two counter-streaming components. Only the (a) type fits to th

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Belenkaya, E. S., P. A. Bespalov, S. S. Davydenko, and V. V. Kalegaev. "Magnetic field influence on aurorae and the Jovian plasma disk radial structure." Annales Geophysicae 24, no. 3 (2006): 973–88. http://dx.doi.org/10.5194/angeo-24-973-2006.

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Abstract. The Jovian paraboloid magnetospheric model is applied for the investigation of the planet's auroral emission and plasma disk structure in the middle magnetosphere. Jupiter's auroral emission demonstrates the electrodynamic coupling between the ionosphere and magnetosphere. For comparison of different regions in the ionospheric level and in the magnetosphere, the paraboloid model of the global magnetospheric magnetic field is used. This model provides mapping along highly-conducting magnetic field lines. The paraboloid magnetic field model is also applied for consideration of the stab

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Dissertations / Theses on the topic "Magnetospheric magnetic field"

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Schwarte, Judith. "Modelling the earth's magnetic field of magnetospheric origin from CHAMP data." [S.l. : s.n.], 2004. http://deposit.ddb.de/cgi-bin/dokserv?idn=971057001.

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Topliss, Stephen Mark. "Particle features at the equatorward edge of the cusp." Thesis, University College London (University of London), 2001. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.342233.

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Patra, Swadesh. "The Contribution of Magnetospheric Currents to Ground Magnetic Perturbation during Geomagnetic Storms." DigitalCommons@USU, 2013. https://digitalcommons.usu.edu/etd/1719.

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A geomagnetic storm is triggered in response to a disturbance in the solar wind. The earth's ring current gets energized during a geomagnetic storm, which leads to a decrease in the horizontal component of the geomagnetic field on the earth's surface. The Disturbance Storm Time (Dst) index, which is a measure of the intensity of the ring current, is calculated by taking the average of this decrease in the horizontal intensity across four low latitude magnetometer stations and removing the quiet time secular variations. The rate of decrease of the Dst index is an indicator of the deenergization

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Schwarte, Judith [Verfasser]. "Modelling the earth's magnetic field of magnetospheric origin from CHAMP data / Geoforschungszentrum Potsdam. Von Judith Schwarte." Potsdam : Geoforschungszentrum, 2004. http://d-nb.info/971057001/34.

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Winslow, Reka Moldovan. "Investigation of Mercury's magnetospheric and surface magnetic fields." Thesis, University of British Columbia, 2014. http://hdl.handle.net/2429/50100.

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This thesis is devoted to the study of Mercury’s magnetic field environment, to reveal the nature of the interaction between a weak planetary magnetic field and the interplanetary medium. Due to the lack of orbital spacecraft observations at Mercury prior to the MErcury Surface, Space Environment, GEochemistry, and Ranging (MESSENGER) mission, work in this thesis presents some of the first analysis and interpretation of observations in this unique and dynamic environment. The bow shock and magnetopause define the boundary regions of the planet’s magnetosphere, thereby representing the initial

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Eriksson, Stefan. "Global Magnetospheric Plasma Convection." Doctoral thesis, Stockholm : Tekniska högsk, 2001. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3230.

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Stetler, Fredrik. "Isolated magnetic field structures in the Saturn magnetosphere." Thesis, KTH, Rymd- och plasmafysik, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-214821.

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This report’s primary focus is to use the data gathered by the Cassini satellite and analyzeits magnetic field data around Saturn. By looking for isolated changes in magneticfield values locations of potential plasmoids can be determined and examined. Theseso called plasmoids are pockets of higher density plasma ,associated with an increaseor decrease of the magnetic field strength, inside the magnetosheath, which may be importantfor the interaction between the solar wind plasma and the magnetosphere. Thestudy has been made over 7 years, from the beginning of 2010 to the end of 2016. Duringthi

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Yuen, Rai. "Pulsar Magnetosphere Revisited: Emission Geometry and the Synthesis of the Vacuum-Dipole and the Rotating-Magnetosphere Models." Thesis, The University of Sydney, 2013. http://hdl.handle.net/2123/10011.

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We reconsider the vacuum-dipole model (VDM) and the corotating-magnetosphere model (CMM) for pulsar electrodynamics. Both the VDM and the CMM are fatally flawed as stand-alone models. The former model is used for deriving certain pulsar parameters, such as the surface magnetic field strength and characteristic age, but it lacks the plasma required to emit the observed radiation. The latter model introduces important concepts, such as the Goldreich-Julian charge density and corotation electric field, which form the basis for more detailed models, but it neglects the inductive electric field. Wh

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Bunting, Robert J. "Development and use of a current wedge modelling method for analysis of multiple onset substorms." Thesis, University of York, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.338555.

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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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Books on the topic "Magnetospheric magnetic field"

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United States. National Aeronautics and Space Administration., ed. Magnetospheric substorms and tail dynamics: Final technical report. National Aeronautics and Space Administration, 1998.

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Curtis, S. The Magnetospheric Multiscale Mission--: Resolving fundamental processes in space plasmas : report of the NASA Science and Technology Definition Team for the Magnetospheric Multiscale (MMS) Mission. National Aeronautics and Space Administration, Goddard Space Flight Center, 1999.

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Moore, T. E. The geopause. National Aeronautics and Space Administration, 1995.

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C, Delcourt D., and George C. Marshall Space Flight Center., eds. The geopause. NASA Marshall Space Flight Center, 1995.

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1962-, Ohtani Shin-ichi, and AGU Chapman Conference on Magnetospheric Current Systems (1999 : Kona, Hawaii), eds. Magnetospheric current systems. American Geophysical Union, 2000.

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1943-, Priest E. R., and Summer School on Solar System Plasmas (1984 : Imperial College), eds. Solar system magnetic fields. D. Reidel Pub. Co., 1985.

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L, Horwitz James, Gallagher D. L, and United States. National Aeronautics and Space Administration., eds. Convection of plasmaspheric plasma into the outer magnetosphere and boundary layer region: Initial results. National Aeronautics and Space Administration, 1998.

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The magnetic universe: The elusive traces of an invisible force. Johns Hopkins University Press, 2009.

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United States. National Aeronautics and Space Administration., ed. [Data acquisition and analysis: Solar vector magnetosphere : final report, Aug. - Dec. 1991. University of Alabama in Huntsville, 1992.

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Verő, József. Hullámok a bolygóközi térből, vagy csak a magnetoszférából?: A geomágneses pulzációk eredete : Akadémiai székfoglaló 1996. október. Akadémiai Kiadó, 1999.

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Book chapters on the topic "Magnetospheric magnetic field"

1

Milan, S. E., L. B. N. Clausen, J. C. Coxon, et al. "Overview of Solar Wind–Magnetosphere–Ionosphere–Atmosphere Coupling and the Generation of Magnetospheric Currents." In Earth's Magnetic Field. Springer Netherlands, 2017. http://dx.doi.org/10.1007/978-94-024-1225-3_19.

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Olson, W. P., K. A. Pfitzer, and G. J. Mroz. "Modeling the Magnetospheric Magnetic Field." In Quantitative Modeling of Magnetospheric Processes. American Geophysical Union, 2013. http://dx.doi.org/10.1029/gm021p0077.

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Lühr, Hermann, Chao Xiong, Nils Olsen, and Guan Le. "Near-Earth Magnetic Field Effects of Large-Scale Magnetospheric Currents." In Earth's Magnetic Field. Springer Netherlands, 2017. http://dx.doi.org/10.1007/978-94-024-1225-3_18.

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Finlay, C. C., V. Lesur, E. Thébault, F. Vervelidou, A. Morschhauser, and R. Shore. "Challenges Handling Magnetospheric and Ionospheric Signals in Internal Geomagnetic Field Modelling." In Earth's Magnetic Field. Springer Netherlands, 2017. http://dx.doi.org/10.1007/978-94-024-1225-3_7.

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Koskinen, Hannu E. J., and Emilia K. J. Kilpua. "Radiation Belts and Their Environment." In Astronomy and Astrophysics Library. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-82167-8_1.

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AbstractThe Van Allen radiation belts of high-energy electrons and ions, mostly protons, are embedded in the Earth’s inner magnetosphere where the geomagnetic field is close to that of a magnetic dipole. Understanding of the belts requires a thorough knowledge of the inner magnetosphere and its dynamics, the coupling of the solar wind to the magnetosphere, and wave–particle interactions in different temporal and spatial scales. In this introductory chapter we briefly describe the basic structure of the inner magnetosphere, its different plasma regions and the basics of magnetospheric activity.

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Nagai, Tsugunobu. "An Empirical Model of Substorm-Related Magnetic Field Variations at Synchronous Orbit." In Magnetospheric Substorms. American Geophysical Union, 2013. http://dx.doi.org/10.1029/gm064p0091.

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Olsen, Nils, and Claudia Stolle. "Magnetic Signatures of Ionospheric and Magnetospheric Current Systems During Geomagnetic Quiet Conditions—An Overview." In Earth's Magnetic Field. Springer Netherlands, 2017. http://dx.doi.org/10.1007/978-94-024-1225-3_2.

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Mcpherron, Robert L. "The Synchronous Orbit Magnetic Field Data Set." In Quantitative Modeling of Magnetospheric Processes. American Geophysical Union, 2013. http://dx.doi.org/10.1029/gm021p0035.

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Jacquey, Christian. "Substorm associated tail current changes inferred from lobe magnetic field observations." In Magnetospheric Current Systems. American Geophysical Union, 2000. http://dx.doi.org/10.1029/gm118p0275.

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Horbury, T. S., A. Balogh, M. W. Dunlop, et al. "Cluster magnetic field observations of magnetospheric boundaries." In Earth's Low-Latitude Boundary Layer. American Geophysical Union, 2003. http://dx.doi.org/10.1029/133gm06.

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Conference papers on the topic "Magnetospheric magnetic field"

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Vellante, M., M. Piersanti, B. Heilig, J. Reda, and A. Del Corpo. "Magnetospheric plasma density inferred from field line resonances: Effects of using different magnetic field models." In 2014 XXXIth URSI General Assembly and Scientific Symposium (URSI GASS). IEEE, 2014. http://dx.doi.org/10.1109/ursigass.2014.6929941.

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Chamati, Maria. "CHARACTERISTICS OF Pc5 PULSATIONS ACTIVITY AT MID LATITUDES DURING DECEMBER 2019." In 22nd SGEM International Multidisciplinary Scientific GeoConference 2022. STEF92 Technology, 2022. http://dx.doi.org/10.5593/sgem2022/1.1/s05.059.

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Magnetospheric pulsations and the mechanisms underlying their generation are topics under active studies. The Pc5 (f =1.7�6.7 mHz) geomagnetic continuous pulsations, recorded at mid latitudes (L =1.6) during December 2019, with a low level of geomagnetic activity, are analyzed and discussed in this paper. The data sets of the series on geomagnetic field variations recorded at Panagjuriste Geomagnetic Observatory in Bulgaria are analyzed. The spectral characteristics of the pulsations were determined by Continuous Wavelet Analysis (CWT). It is demonstrated that Pc5 pulsation activity appears wi

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Chamati, Maria, and Borislav Andonov. "Pc5 PULSATIONS OBSERVED DURING THE GEOMAGNETIC STORM ON 12 MAY 2021." In 22nd SGEM International Multidisciplinary Scientific GeoConference 2022. STEF92 Technology, 2022. http://dx.doi.org/10.5593/sgem2022/1.1/s05.063.

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The study of ultra-low frequency (ULF) waves and geomagnetic pulsations plays an important role in better understanding the mechanisms of their generation and spread in the magnetosphere and on the ground. The magnetospheric ULF waves, which provide useful information about the conditions in the solar wind and in the magnetosphere, can be detected on the ground by different types of magnetometers and recorded as geomagnetic pulsations � continuous and irregular. This paper aims to study the characteristics of Pc5 geomagnetic continuous pulsations recorded at mid latitudes during the strong geo

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Melrose, Don. "Oscillating pair creation in pulsar magnetospheres." In MAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures. AIP, 2005. http://dx.doi.org/10.1063/1.2077191.

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Mao, Yao-Ting, David Auslander, David Pankow, and John Sample. "Estimating Angular Velocity, Attitude Orientation With Controller Design for Three Units CubeSat." In ASME 2014 Dynamic Systems and Control Conference. American Society of Mechanical Engineers, 2014. http://dx.doi.org/10.1115/dscc2014-5895.

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CINEMA (CubeSat for Ions, Neutrals, Electrons and MAgneticfields) will image energetic neutral atoms (ENAs) in the magnetosphere, and make measurements of electrons, ions, and magnetic fields at high latitudes. To satisfy the mission requirements, the three unit cubesat was designed. The spin axis needs to be in the ecliptic normal and the spin rate needs to be 4 rpm. The only power source for CINEMA is the solar panels. External torques are generated by an orthogonal pair of coils acting with the earths magnetic field. This paper provides the control strategy, given the limited power and avai

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Asimopolos, Laurentiu, Natalia-Silvia Asimopolos, and Adrian-Aristide Asimopolos. "COMPARATIVE AND SPECTRAL STUDIES BETWEEN GEOMAGNETIC SERIES RECORDED IN INTERMAGNET OBSERVATORIES." In 22nd SGEM International Multidisciplinary Scientific GeoConference 2022. STEF92 Technology, 2022. http://dx.doi.org/10.5593/sgem2022/6.1/s28.36.

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The main objectives of this study are: analysis of the associated spectrum of the geomagnetic field, time of occurrence of geomagnetic storms and comparisons between recordings made at various geomagnetic observatories in the INTERMAGNET network, in terms of frequency intensity identified and correlations during geomagnetic disturbances. A geomagnetic storm is a temporary disturbance of the Earth's magnetosphere caused by ejections of solar corona mass, coronal holes or solar flares. The data used in this paper are recorded from the Surlari Observatory, and additional information for the chara

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Ma, Qianli, Wen Li, and Xiao-Jia Zhang. "Modeling Electron Scattering and Acceleration by Whistler Mode Chorus Waves in Jupiter's Magnetosphere: Effects of Magnetic Field Model, Total Electron Density, and Electron Injections." In 2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS). IEEE, 2021. http://dx.doi.org/10.23919/ursigass51995.2021.9560536.

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Reports on the topic "Magnetospheric magnetic field"

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Branduardi-Raymont, Graziella, and et al. SMILE Definition Study Report. ESA SCI, 2018. http://dx.doi.org/10.5270/esa.smile.definition_study_report-2018-12.

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The SMILE definition study report describes a novel self-standing mission dedicated to observing solar wind-magnetosphere coupling via simultaneous in situ solar wind/magnetosheath plasma and magnetic field measurements, X-Ray images of the magnetosheath and magnetic cusps, and UV images of global auroral distributions defining system-level consequences. The Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) will complement all solar, solar wind and in situ magnetospheric observations, including both space- and ground-based observatories, to enable the first-ever observations of the ful

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BARKHATOV, NIKOLAY, and SERGEY REVUNOV. A software-computational neural network tool for predicting the electromagnetic state of the polar magnetosphere, taking into account the process that simulates its slow loading by the kinetic energy of the solar wind. SIB-Expertise, 2021. http://dx.doi.org/10.12731/er0519.07122021.

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The auroral activity indices AU, AL, AE, introduced into geophysics at the beginning of the space era, although they have certain drawbacks, are still widely used to monitor geomagnetic activity at high latitudes. The AU index reflects the intensity of the eastern electric jet, while the AL index is determined by the intensity of the western electric jet. There are many regression relationships linking the indices of magnetic activity with a wide range of phenomena observed in the Earth's magnetosphere and atmosphere. These relationships determine the importance of monitoring and predicting ge

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Huang, Tian-Sen, Philippe Le-Sager, and Yuri V. Petrov. Proposal Coupling of Earth's Magnetosphere and Ionosphere in a Realistic Magnetic Field. Defense Technical Information Center, 2000. http://dx.doi.org/10.21236/ada387201.

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Van Allen, James A. Energetic Particles and Magnetic Fields in the Earth's Magnetosphere and Interplanetary Space. Defense Technical Information Center, 1997. http://dx.doi.org/10.21236/ada628212.

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Lee, L. C., and S. I. Akasofu. [A study of the magnetic field annihilation process in the magnetosphere and some geotechnical applications]. Office of Scientific and Technical Information (OSTI), 1993. http://dx.doi.org/10.2172/6873123.

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Lee, L. C., and S. L. Akasofu. [A study of the magnetic field annihilation process in the magnetosphere and some geotechnical applications]. Office of Scientific and Technical Information (OSTI), 1993. http://dx.doi.org/10.2172/6610443.

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Lee, L. C., and S. L. Akasofu. [A study of the magnetic field annihilation process in the magnetosphere and some geotechnical applications]. Progress report. Office of Scientific and Technical Information (OSTI), 1993. http://dx.doi.org/10.2172/10147941.

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Lee, L. C., and S. I. Akasofu. [A study of the magnetic field annihilation process in the magnetosphere and some geotechnical applications]. Progress report. Office of Scientific and Technical Information (OSTI), 1993. http://dx.doi.org/10.2172/10147946.

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[A study of the magnetic field annihilation process in the magnetosphere and some geotechnical applications]. Office of Scientific and Technical Information (OSTI), 1993. http://dx.doi.org/10.2172/6584414.

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[A study of the magnetic field annihilation process in the magnetosphere and some geotechnical applications]. Office of Scientific and Technical Information (OSTI), 1993. http://dx.doi.org/10.2172/6610452.

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