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Author: Grafiati

Published: 10 December 2022

Last updated: 28 January 2023

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1

Volker, Bothmer, Hady Ahmed Abdel, and International Astronomical Union, eds. Solar activity and its magnetic origin: Proceedings of the 233rd symposium of the International Astronomical Union held in Cairo, Egypt, March 31-April 4, 2006. Cambridge: Cambridge University Press, 2006.

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2

A, Balona Luis, Henrichs Huib F, and Medupe Rodney, eds. International Conference on Magnetic Fields in O, B and A Stars: Origin and connection to pulsation, rotation and mass loss : proceedings of a conference held at University of North-West, Mmabatho, South Africa, 27 November - 1 December, 2002. San Francisco, California: Astronomical Society of the Pacific, 2003.

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3

Es'kov, Evgeniy. Biological effects of electromagnetic fields. ru: INFRA-M Academic Publishing LLC., 2021. http://dx.doi.org/10.12737/1229809.

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The monograph, based on the use of literary information and research materials of the author, attempts to systematize the influence of natural and anthropogenic electric fields on biological objects of different levels of complexity. The origin of cosmic and terrestrial magnetism is described and the influence of this factor on the physiological state, viability and development of plant and animal objects is analyzed. The biological effects of magnetic storms are investigated. The mechanisms of generation, perception and use of electric fields in signaling and spatial orientation of animals are analyzed. Much attention is paid to the analysis of specific reactions of animals to electromagnetic fields. The prospects of using electromagnetic fields to control the behavior of animals and direct influence on the growth processes of plant objects are considered. For a wide range of readers interested in the possibilities of controlling animal behavior and influencing plant growth.

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4

Magnetic field(s). Normal, Ill: Dalkey Archive Press, 2002.

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5

Stolle, Claudia, Nils Olsen, Arthur D. Richmond, and Hermann J. Opgenoorth, eds. Earth's Magnetic Field. Dordrecht: Springer Netherlands, 2018. http://dx.doi.org/10.1007/978-94-024-1225-3.

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6

Rajaram, Girija. The earth's magnetic field. New Delhi: Oxford & IBH Pub Co., 1998.

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7

Grönemeyer, D. H. W., and Robert B. Lufkin, eds. Open Field Magnetic Resonance Imaging. Berlin, Heidelberg: Springer Berlin Heidelberg, 2000. http://dx.doi.org/10.1007/978-3-642-59581-3.

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8

Aono, Osamu. Rotation of a magnetic field. Nagoya, Japan: Institute of Plasma Physics, Nagoya University, 1986.

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9

Marshall, Deborah. Magnetic field strength issues in magnetic resonance imaging (MRI). Ottawa: Canadian Coordinating Office for Health Technology Assessment, 1993.

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10

Shao, Yarui. Magnetic flocculation of fine weakly magnetic iron minerals in an applied magnetic field. Birmingham: University of Birmingham, 1997.

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11

Satter, Md Abdus. A theory for dilute magnetic alloys: The origin of magnetic anisotropy. [s.l.]: typescript, 1989.

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12

Iványi, Amália. Magnetic field computation with R-functions. Budapest: Akadémiai Kiadó, 1998.

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13

Ivaányi, Amália. Magnetic field computation with R-functions. Budapest: Akadémiai Kiadó, 1998.

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14

Jacobs, J. A. Reversals of the earth's magnetic field. 2nd ed. Cambridge: Cambridge University Press, 1994.

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15

Labyt, Etienne, Tilmann Sander, and Ronald Wakai, eds. Flexible High Performance Magnetic Field Sensors. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-031-05363-4.

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16

Robitaille, Pierre-Marie, and Lawrence Berliner. Ultra High Field Magnetic Resonance Imaging. Boston, MA: Springer US, 2006. http://dx.doi.org/10.1007/978-0-387-49648-1.

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17

D’haeseleer, William Denis, William Nicholas Guy Hitchon, James D. Callen, and J. Leon Shohet. Flux Coordinates and Magnetic Field Structure. Berlin, Heidelberg: Springer Berlin Heidelberg, 1991. http://dx.doi.org/10.1007/978-3-642-75595-8.

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18

Sulaiman, Ali Haidar. The Near-Saturn Magnetic Field Environment. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-49292-6.

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19

Erbe, Marlitt. Field Free Line Magnetic Particle Imaging. Wiesbaden: Springer Fachmedien Wiesbaden, 2014. http://dx.doi.org/10.1007/978-3-658-05337-6.

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20

Berger, T. E. On the dynamics of small-scale solar magnetic elements. [Washington, DC: National Aeronautics and Space Administration, 1996.

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21

Berger, T. E. On the dynamics of small-scale solar magnetic elements. [Washington, DC: National Aeronautics and Space Administration, 1996.

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22

Berger, T. E. On the dynamics of small-scale solar magnetic elements. [Washington, DC: National Aeronautics and Space Administration, 1996.

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23

Berger, T. E. On the dynamics of small-scale solar magnetic elements. [Washington, DC: National Aeronautics and Space Administration, 1996.

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24

Burlaga, L. F. Fractal structure of the interplanetary magnetic field. Greenbelt, Md: National Aeronautics and Space Administration, Goddard Space Flight Center, 1985.

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25

Force, Washington (State) Electric Transmission Research Needs Task. Electric and magnetic field reduction: Research needs. [Olympia, Wash.]: The Task Force, 1992.

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26

Looi, Thomas. Magnetic field simulator for microsatellite attitude testing. Ottawa: National Library of Canada, 2002.

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27

Looi, Thomas. Magnetic field simulator for microsatellite attitude testing. [Downsview, Ont.]: University of Toronto, Institute for Aerospace Studies, 2002.

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28

Holmes, John J. Exploitation of A Ship’s Magnetic Field Signatures. Cham: Springer International Publishing, 2006. http://dx.doi.org/10.1007/978-3-031-01693-6.

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29

Holmes, John J. Reduction of a Ship’s Magnetic Field Signatures. Cham: Springer International Publishing, 2008. http://dx.doi.org/10.1007/978-3-031-01708-7.

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30

Klein, Hans-Martin. Clinical Low Field Strength Magnetic Resonance Imaging. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-16516-5.

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31

Soloviev, A., A. Khokhlov, E. Jalkovsky, A. Berezko, A. Lebedev, E. Kharin, I. Shestopalov, et al. The Atlas of the Earth's Magnetic Field. Moscow: Geophysical Center RAS, 2012. http://dx.doi.org/10.2205/2012atlas_mpz.

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32

Soloviev, A., A. Khokhlov, E. Jalkovsky, A. Berezko, A. Lebedev, E. Kharin, I. Shestopalov, et al. The Atlas of the Earth's Magnetic Field. Moscow: Geophysical Center RAS, 2012. http://dx.doi.org/10.2205/2013bs011_atlas_mpz.

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33

Origin and Destiny of the Earth's Magnetic Field. Master Books, 1989.

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34

Nordlund, Å., M. J. Thompson, J. L. Culhane, A. Balogh, and S. K. Solanki. Origin and Dynamics of Solar Magnetism. Springer New York, 2011.

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35

Nordlund, Å., M. J. Thompson, J. L. Culhane, A. Balogh, and S. K. Solanki. Origin and Dynamics of Solar Magnetism. Springer London, Limited, 2009.

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36

J, Thompson M., ed. The origin and dynamics of solar magnetism. [New York?]: Springer, 2009.

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37

Thompson, M. J., J. L. Culhane, and A. Balogh. The Origin and Dynamics of Solar Magnetism. Springer, 2009.

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38

Parker, E. N. Cosmical Magnetic Fields: Their Origin and Their Activity. Oxford University Press, 2019.

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39

Michels, Andreas. Magnetic Small-Angle Neutron Scattering. Oxford University Press, 2021. http://dx.doi.org/10.1093/oso/9780198855170.001.0001.

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This book provides the first extensive treatment of magnetic small-angle neutron scattering (SANS). The theoretical background required to compute magnetic SANS cross sections and correlation functions related to long-wavelength magnetization structures is laid out; and these concepts are scrutinized based on the discussion of experimental neutron data. Regarding prior background knowledge, some familiarity with the basic magnetic interactions and phenomena, as well as scattering theory, is desired. The target audience comprises Ph.D. students and researchers working in the field of magnetism and magnetic materials who wish to make efficient use of the magnetic SANS method. Besides revealing the origins of magnetic SANS (Chapter 1), and furnishing the basics of the magnetic SANS technique (Chapter 2), much of the book is devoted to a comprehensive treatment of the continuum theory of micromagnetics (Chapter 3), as it is relevant for the study of the elastic magnetic SANS cross section. Analytical expressions for the magnetization Fourier components allow one to highlight the essential features of magnetic SANS and to analyze experimental data both in reciprocal (Chapter 4) and real space (Chapter 6). Chapter 5 provides an overview of the magnetic SANS of nanoparticles and so-called complex systems (e.g., ferrofluids, magnetic steels, spin glasses, and amorphous magnets). It is this subfield where major progress is expected to be made in the coming years, mainly via the increased use of numerical micromagnetic simulations (Chapter 7), which is a very promising approach for the understanding of the magnetic SANS from systems exhibiting nanoscale spin inhomogeneity.

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40

(Editor), Volker Bothmer, and Ahmed Abdel Hady (Editor), eds. Solar Activity and its Magnetic Origin (IAU S233) (Proceedings of the International Astronomical Union Symposia and Colloquia). Cambridge University Press, 2006.

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41

ARMITAGE, S. Magnetic Field. Faber & Faber, Limited, 2020.

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42

Nitta, J. Spin generation and manipulation based on spin-orbit interaction in semiconductors. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780198787075.003.0013.

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This chapter focuses on the electron spin degree of freedom in semiconductor spintronics. In particular, the electrostatic control of the spin degree of freedom is an advantageous technology over metal-based spintronics. Spin–orbit interaction (SOI), which gives rise to an effective magnetic field. The essence of SOI is that the moving electrons in an electric field feel an effective magnetic field even without any external magnetic field. Rashba spin–orbit interaction is important since the strength is controlled by the gate voltage on top of the semiconductor’s two-dimensional electron gas. By utilizing the effective magnetic field induced by the SOI, spin generation and manipulation are possible by electrostatic ways. The origin of spin-orbit interactions in semiconductors and the electrical generation and manipulation of spins by electrical means are discussed. Long spin coherence is achieved by special spin helix state where both strengths of Rashba and Dresselhaus SOI are equal.

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43

Kosovichev, Alexander G., Moira Jardine, and Klaus Strassmeier. Solar and Stellar Magnetic Fields: Origins and Manifestations. University of Cambridge ESOL Examinations, 2020.

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44

Kumar, C. S. Nikhil. Magnetic Resonators: Feedback with Magnetic Field and Magnetic Cavity. Springer, 2022.

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45

Balona, Luis. Magnetic Fields in O, B and a Stars - Origin and Connection to Pulsation, Rotation and Mass Loss: Proceedings, International Conference, Mmabatho, South ... Society of the Pacific Conference Series). Astronomical Society of the Pacific, 2003.

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46

ARMITAGE, S. Magnetic Field * Ebook Epub *. Faber & Faber, Limited, 2020.

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47

Gray, William E. Know Your Magnetic Field. Kendall/Hunt Publishing Company, 1993.

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48

Khan, Dilshad Ahmad, Zafar Alam, and Faiz Iqbal. Magnetic Field Assisted Finishing. Taylor & Francis Group, 2021.

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49

Dash, Palmer. Safe Magnetic Field Levels: Effect of Magnetic Field on Human Health. Independently Published, 2022.

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50

Valenzuela, S. O. Introduction. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780198787075.003.0011.

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This chapter begins with a definition of spin Hall effects, which are a group of phenomena that result from spin–orbit interaction. These phenomena link orbital motion to spin direction and act as a spin-dependent magnetic field. In its simplest form, an electrical current gives rise to a transverse spin current that induces spin accumulation at the boundaries of the sample, the direction of the spins being opposite at opposing boundaries. It can be intuitively understood by analogy with the Magnus effect, where a spinning ball in a fluid deviates from its straight path in a direction that depends on the sense of rotation. spin Hall effects can be associated with a variety of spin-orbit mechanisms, which can have intrinsic or extrinsic origin, and depend on the sample geometry, impurity band structure, and carrier density but do not require a magnetic field or any kind of magnetic order to occur.

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