Relevant bibliographies by topics / Terrestial Magnetism

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

Academic literature on the topic 'Terrestial Magnetism'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 February 2022

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Journal articles on the topic "Terrestial Magnetism"

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Udías, S.J., Agustín. "Athanasius Kircher and Terrestrial Magnetism: The Magnetic Map." Journal of Jesuit Studies 7, no. 2 (January 29, 2020): 166–84. http://dx.doi.org/10.1163/22141332-00702002.

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Athanasius Kircher paid special attention to magnetism, more specifically terrestrial one, in his work Magnes sive de arte magnetica. Other Jesuits of his time, such as Garzoni and Cabeo, also wrote on this subject. Kircher studied in particular magnetic declination and its possible use to determine geographical longitudes. At his time, this was an important subject for long sea journeys. First, he collected a large number of observations of magnetic declination from different sources in three tables and two lists with a total of 518 values, among them forty-three made by Jesuits. Kircher proposed that a magnetic map could be made based on these observations, but he did not do it. From Kircher’s observations a map of magnetic declination has been drawn and it is presented here. Kircher discussed the causes of declination and presented a model for the origin of the magnetic field of the Earth, which differed from that proposed by Gilbert. Kircher finally considered magnetism as a cosmic force with its origin in God.
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ENEBAKK, VIDAR. "Hansteen's magnetometer and the origin of the magnetic crusade." British Journal for the History of Science 47, no. 4 (November 7, 2013): 587–608. http://dx.doi.org/10.1017/s0007087413000903.

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AbstractIn the early nineteenth century, Norwegian mathematician and astronomer Christopher Hansteen (1784–1873) contributed significantly to international collaboration in the study of terrestrial magnetism. In particular, Hansteen was influential in the origin and orientation of the magnetic lobby in Britain, a campaign which resulted in a global network of fixed geomagnetic observatories. In retrospect, however, his contribution was diminished, because his four-pole theory inUntersuchungen der Magnetismus der Erde(1819) was ultimately refuted by Carl Friedrich Gauss inAllgemeine Theorie des Erdmagnetismus(1839). Yet Hansteen's main contribution was practical rather than theoretical. His major impact was related to the circulation of his instruments and techniques. From the mid-1820s, ‘Hansteen's magnetometer’ was distributed all over the British Isles and throughout the international scientific community devoted to studying terrestrial magnetism. Thus in the decades before the magnetic crusade, Hansteen had established an international system of observation, standardization and representation based on measurements with his small and portable magnetometers.
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Gumarova, L., and G. Cornelissen. "Terrestrial and solar magnetism’ influence to diphtheria pandemics." International Journal of Biology and Chemistry 9, no. 2 (2016): 4–10. http://dx.doi.org/10.26577/2218-7979-2016-9-2-4-10.

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McConnell, Anita. "Surveying terrestrial magnetism in time and space." Archives of Natural History 32, no. 2 (October 2005): 346–60. http://dx.doi.org/10.3366/anh.2005.32.2.346.

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Charts marked with the lines of magnetic variation have been published since Halley's Atlantic chart of 1701. It was already known that the location of the magnetic poles shifted over time, and that the north and south poles were not diametrically opposite. As more seafarers penetrated the Southern Ocean, isogons on the charts were extended southwards with greater confidence. At sea variation was measured by comparing compass direction with the Sun's midday shadow. In polar regions, where horizontal force is too weak to attract a compass needle, the location of the pole was sought by observing the inclination of a dip needle swinging in the magnetic meridian, which would hang vertically at the pole. The Fox dip circle, developed in 1834, was the first instrument capable of measuring dip and intensity at sea, and allowed James Clark Ross to predict the location of the South Magnetic Pole. In 1902 Discovery's crew landed an observatory ashore, but a trek on to the plateau failed to reach the magnetic pole. Success came in 1909 during Shackleton's Nimrod expedition, when T. Edgeworth David's party reached the zone of maximum dip. Over the following years data from photographic magnetometers recording declination, vertical and horizontal intensity were routinely made at the various national bases round Antarctica; they contributed to our knowledge of the Earth's internal magnetism and on the solar influences.
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Tachinami, Chihiro, Hiroki Senshu, and Shigeru Ida. "Thermal evolution and magnetism of terrestrial planets." Proceedings of the International Astronomical Union 3, S249 (October 2007): 159–62. http://dx.doi.org/10.1017/s1743921308016542.

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AbstractWe evaluate a numerical model on the thermal evolution of terrestrial planets to estimate life-time of planetary intrinsic magnetic field for various mass planets. In this model, we take into account the pressure-dependency of density profile of the planet by using Birch-Murnaghun equation of state, and simulate thermal evolution of the planet by means of mixing length theory. According to our numerical results, the planetary mass must be between 0.1 and 1.4 Earth mass to sustain the intrinsic magnetic field for 4.5Gyr. If existence of intrinsic magnetic field were a key factor to make the planet habitable, the mass range above indicates that super-Earths would not be habitable.
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Gubbins, David. "Terrestrial Magnetism: Historical Perspectives and Future Prospects." Space Science Reviews 155, no. 1-4 (August 2010): 9–27. http://dx.doi.org/10.1007/s11214-010-9675-6.

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Udías, Agustín. "Jesuits and the Natural Sciences in Modern Times, 1814–2014." Brill Research Perspectives in Jesuit Studies 1, no. 3 (May 17, 2019): 1–104. http://dx.doi.org/10.1163/25897454-12340003.

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Abstract After their restoration of 1814, the Jesuits made significant contributions to the natural sciences, especially in the fields of astronomy, meteorology, seismology, terrestrial magnetism, mathematics, and biology. This narrative provides a history of the Jesuit institutions in which these discoveries were made, many of which were established in countries that previously had no scientific institutions whatsoever, thus generating a scientific and educational legacy that endures to this day. The essay also focuses on the teaching and research that took place at Jesuit universities and secondary schools, as well as the order’s creation of a worldwide network of seventy-four astronomical and geophysical observatories where particularly important contributions were made to the fields of terrestrial magnetism, microseisms, tropical hurricanes, and botany.
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Josefowicz, Diane Greco. "Experience, Pedagogy, and the Study of Terrestrial Magnetism." Perspectives on Science 13, no. 4 (December 2005): 452–94. http://dx.doi.org/10.1162/106361405775466108.

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SVENONIUS, ERIC OLAUSSON AND BJÖRN. "The relation between glacial ages and terrestrial magnetism." Boreas 2, no. 3 (January 16, 2008): 109–15. http://dx.doi.org/10.1111/j.1502-3885.1973.tb00250.x.

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OZCEP, FERHAT. "TERRESTRIAL MAGNETISM IN THE OTTOMAN EMPIRE: DOCUMENTS AND MEASUREMENTS." Earth Sciences History 37, no. 1 (January 1, 2018): 1–24. http://dx.doi.org/10.17704/1944-6178-37.1.1.

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ABSTRACT Geophysics, in the modern sense, started with geomagnetic works in the 1600s in the Ottoman Empire. The period between 1600 and 1800 included the measurement of magnetic declination, inclination and magnetic field strength. Before that time, there was only a little information available, such as how to use a compass, for example in the Kitab-i Bahriye (the Book of Navigation) by Piri Reis, one of the most important mariners of the Ottoman Empire. However, this may not mean that magnetic declination was generally understood. The first Turkish scientific book relating to terrestrial magnetism was the book Fuyuzat-i Miknatissiye that was translated in 1731 from German into Turkish by Ibrahim Müteferrika. The subject of that book was earth's magnetism. The magnetic compass was mentioned in several books including Muhammed al Awfi's Jami al- Hikayat (translated into Turkish by Ibn Arabşah); Piri Reis's Kitab-I Bahriye (The Book of ‘Navigation’); Seydi Ali Reis's Risale-i Mirat-I Kainat min Alat-I Irtifa (The Treatise called the Mirror of Universe according to the instrument for measuring Altitude) and Kitab Al-Muhit Fi'Ilm'al-Eflak Va'l Abhur (Book of the Regional Seas and the Science of Astronomy and Navigation). There were two original magnetic declination measurements made by Ottoman Turks in Istanbul in 1727 and 1893. Also, many geomagnetic measurements were carried out during international campaigns between 1600 and 1917 that visited Ottoman territory.
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Dissertations / Theses on the topic "Terrestial Magnetism"

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Farrell, Robert. "Rotating Magnetometry For Terrestrial And Extraterrestrial Subsurface Explorations." ScholarWorks @ UVM, 2018. https://scholarworks.uvm.edu/graddis/945.

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Signaling and sensing with rotating magnet sources have both Terrestrial and Extraterrestrial applications. The dual spinning magnet unit presented in this paper is a simple, lightweight solution to help understand soil densities and locate water and ice pockets, for example, on Mars. Traditional magnetic telemetry systems that use energy-inefficient large induction coils and antennas as sources and receivers are not practical for extraterrestrial and remote field sensing applications. The recent proliferation of strong rare-earth permanent magnets and high-sensitivity magnetometers enables alternative magnetic telemetry system concepts with significantly more compact formats and lower energy consumption. There are also terrestrial applications, for example, subterranean objects such as underground infrastructure and unexploded ordnances (UXO) that are often unmapped and difficult to find on Earth. Current ground penetrating radar units are expensive, large, and heavy. The research presented explores the viability and possibility to develop a unit that will induce an oscillating magnetic field with controllable shape to reliably locate buried ferromagnetic and non-ferromagnetic objects while remaining lightweight and cost effective. A Dual Rotating Magnet (DRM) design is presented. Experiments and numerical simulations assess the system for terrestrial and extraterrestrial detection of: 1) differences in soil densities, 2) water and ice pockets at shallow depths in the subsurface, and 3) subterranean ferromagnetic and non-ferromagnetic objects of interest.
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陳伯舫 and Pak-fong Chan. "Numerical investigations of the terrestrial conductivity anomaly undervarious geophysical conditions." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1988. http://hub.hku.hk/bib/B31231494.

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Goodman, Matthew. "From 'magnetic fever' to 'magnetical insanity' : historical geographies of British terrestrial magnetic research, 1833-1857." Thesis, University of Glasgow, 2018. http://theses.gla.ac.uk/30829/.

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This thesis explores British-led efforts to observe and map the earth’s magnetic field between 1833 and 1857. In doing so, the thesis examines how magnetic instruments, magnetic observers and magnetic instructions were mobilised in and across multiple geographies, from the Canadian Arctic, to the island of St Helena, to Van Diemen’s Land in the southern hemisphere and at many sites in between. Interest in terrestrial magnetic research burgeoned and was crystallised during the early nineteenth century in Britain and abroad and resulted in the creation of systems of physical observatories and the organisation of magnetic surveys. This work addresses what it meant to coordinate such a network by scrutinising what is popularly known as “the magnetic crusade”, but which was more commonly referred to at the time as the British magnetic scheme. There were several individuals involved in the formation of this scheme but this thesis focuses on two in particular: Edward Sabine and Humphrey Lloyd. In the correspondence of these two figures, we can follow the process by which terrestrial magnetic research was disciplined, its participants educated, its observational data organised and its instruments developed, deployed and used at different stations across the globe. This work seeks to extend and at times complicate our understanding of what it meant to coordinate a big Victorian scientific pursuit and explores among other things the management of instruments in different geographic contexts; the experience of scientific servicemen in the observatory and during surveying efforts; the space in which magnetic data were handled and the processes employed in reducing these data. In all, this thesis aims to recover the several different practices of place that attended the organisation of what was considered in the first half of the nineteenth century to be the greatest scientific endeavour yet pursued.
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Chan, Pak-fong. "Numerical investigations of the terrestrial conductivity anomaly under various geophysical conditions /." [Hong Kong : University of Hong Kong], 1988. http://sunzi.lib.hku.hk/hkuto/record.jsp?B12428577.

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Nordström, Pontus. "Ground based observations of Pi2 pulsation in the terrestrial magnetic field." Thesis, KTH, Rymd- och plasmafysik, 2007. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-91913.

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In this thesis ground-based observations of the terrestrial magnetic field have been used to studythe characteristics of a special type of magnetospheric pulsation called Pi2. The magnetic fielddata used was observed by the SANAE pulsation magnetometer, located at Antarctica. Severalcharacteristics of the pulsations have been examined for 137 events. For all the events aninjection of energetic particles could be seen simultaneously in the magnetosphere, which is anindication of a substorm onset. The particle injection was confirmed by data from theLANL/SOPA electron flux satellites, located in geosynchronous orbits at 6.6 RE height. Themain frequency of the events was concentrated in the lower part of the defined Pi2 range (7-25mHz) with a mean of 11.3 mHz. The polarisation parameters and the rate of damping wereexamined for 20 clear events. The damping increment had typical values of 0.05-2.Thepolarisation azimuth was directed in the North-East/South-West direction for most of the eventsand the sense of polarisation showed a transition from counter clockwise before 0200 local timeto clockwise afterward.
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Lee, Daniel Thomas. "Three-dimensional topology of the magnetic field in the solar corona." Thesis, University of Central Lancashire, 2018. http://clok.uclan.ac.uk/25371/.

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This thesis investigates the topology of the magnetic field in the solar corona, due to a variety of source configurations and types. To fully understand the complex behaviour of the Sun's magnetic field, it is important to have a complete description of the features present in its structure. The magnetic topologies due to network source configurations are investigated using both the point source description and the continuous source description. A series of case studies involving an emerging bipole in a hexagonal arrangement to simulate a supergranular cell are studied. This has a particular focus on the behaviour of coronal nulls located in the topology, and a particular case may form the underpinning of a model for polar plumes. A new topological feature, called a null-like point, is defined by relaxing the definition of a magnetic null point. Separatix-like surfaces, originating from null-like points, allow quasi-separatrix layers to be found in magnetic topologies due to continuously distributed sources. The squashing factor, Q, is mapped across the source configuration, highlighting the locations of the quasi-separatrix layers. Finally, an algorithm is developed which automatically detects and classifies magnetic events local to X-ray bright points (XBPs). Significant peaks are identified in the gradients of flux curves (positive, negative and absolute flux) local to XBP footpoints, allowing instances of flux emergence and cancellation to be identified and linked to the onset and demise of the XBPs studied. The algorithm correctly classifies 90% of all emergence and cancellation events related to the studied XBPs.
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Atkin, Andrew James. "Drivers of scientific success; an analysis of terrestrial magnetism on the Discovery Antarctic expedition, 1901-04." Thesis, University of Canterbury. Gateway Antarctica, 2013. http://hdl.handle.net/10092/8107.

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The turn of the twentieth century was an era of intense exploratory and scientific activity on and around the Antarctic continent. A few campaigns specialised in either territorial discovery or scientific inquiry, but most combined exploration and science in a comfortable alliance that produced results in both arenas. In recent years the scientific achievements of the Discovery expedition (1901-04) have been the subject of renewed analysis, but it is never clear what criteria, if any, are being applied to support statements about scientific success. This research is founded on a case study focused on the magnetic science program of the Discovery expedition commencing with preparations, performance of magnetic observing at sea and ashore, post-expedition management of the products of research, and finally, arrangements for publication. The case study forms the basis for firstly, identifying the indicators of scientific success and secondly, an analysis of the relative contributions of the drivers promoting quality scientific outcomes during the era of Antarctic scientific exploration between 1898 and 1914. The principal elements contributing to superior outcomes are identified as the human elements of preparation, leadership, scientific practice, skill, knowledge development and finally post-expedition management of data or collections gathered during fieldwork. No single element guarantees scientific success; it is a product of a combination of factors, but failure in just one facet can undermine outcomes fatally. The effectiveness of the relationship between these factors determines the degree of success or failure of a program. Achieving the potential of a research program relies on elements coming together in a timely and synergistic manner in combination with a measure of luck. There was confusion between the magnetic work intended to provide improved charts for navigation purposes and the scientific research designed to help solve the causes of terrestrial magnetism and it’s effects. The magnetic work of the expedition was divided into three distinct operations. Firstly, observations were made at sea in the ship’s purpose built magnetic observatory and using a recently developed instrument for the determination of magnetic dip and force. The results were ultimately never published due to the inadequacy of the instrument and the difficulties of taking reliable observations at sea. Secondly, a fixed observatory was established at the base station in Antarctica where a different set of instruments recorded the magnetic elements almost continuously over the two-year stay of the expedition. There was sufficient data from those observations to form the core of the scientific reports on terrestrial magnetism, but large amounts of data were considered unreliable and either discarded, or included with cautionary notes. Thirdly, magnetic observations made on exploratory sledging journeys away from the ice station added evidence for theoretical determination of the location of the South Magnetic Pole and for mapping the lines of equal magnetic declination radiating from it. The conclusions from these journeys were brought into doubt by evidence from later expeditions. During fund raising and promotion of the expedition, Sir Clements Markham, President of the Royal Geographical Society stated firstly, that products of the magnetic research would include new magnetic charts of value to mariners and secondly, there would be significant leaps in knowledge informing magnetic theory. These were ambitious objectives and neither were realised, although the data collected did add to knowledge of the characteristic fluctuations of the magnetic field at high latitudes. Collaborative arrangements planned between the Discovery, the German Gauss expedition and various established land observatories never reached their potential. This was partly due to an error in the timing of synchronous observations, but mainly a result of collapse of the intended post-expedition data sharing arrangements related to rejection by the Germans of the unreliable data from Discovery and failure by the English to publish data in a mutually useful format. The thesis closes with analysis of how well the Discovery’s outcomes matched their potential and concludes that, with respect to magnetic science, institutional failures led to avoidable deficiencies in areas of recruitment, training, governance and leadership, procedures, instrumentation and post-expedition management of data and publication preparations.
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Heil, Clifford William. "Paleo-and environmental magnetic studies of late Cenozoic estuarine, lacustrine, and terrestrial sediments /." View online ; access limited to URI, 2008. http://0-digitalcommons.uri.edu.helin.uri.edu/dissertations/AAI3314457.

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Lawrence, Gareth Rhys. "MHD analysis of the solar-terrestrial interaction : development of tools for studying magnetopause reconnection and the plasma depletion layer." Thesis, University of Sussex, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.241659.

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Martineau, Ryan J. "Parameterized Least-Squares Attitude History Estimation and Magnetic Field Observations of the Auroral Spatial Structures Probe." DigitalCommons@USU, 2015. https://digitalcommons.usu.edu/etd/4482.

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Terrestrial auroras are visible-light events caused by charged particles trapped by the Earth's magnetic eld precipitating into the atmosphere along magnetic eld lines near the poles. Auroral events are very dynamic, changing rapidly in time and across large spatial scales. Better knowledge of the low of energy during an aurora will improve understanding of the heating processes in the atmosphere during geomagnetic and solar storms. The Auroral Spatial Structures Probe is a sounding rocket campaign to observe the middle-atmosphere plasma and electromagnetic environment during an auroral event with multipoint simultaneous measurements for fine temporal and spatial resolution. The auroral event in question occurred on January 28, 2015, with liftoff the rocket at 10:41:01 UTC. The goal of this thesis is to produce clear observations of the magnetic eld that may be used to model the current systems of the auroral event. To achieve this, the attitude of ASSP's 7 independent payloads must be estimated, and a new attitude determination method is attempted. The new solution uses nonlinear least-squares parameter estimation with a rigid-body dynamics simulation to determine attitude with an estimated accuracy of a few degrees. Observed magnetic eld perturbations found using the new attitude solution are presented, where structures of the perturbations are consistent with previous observations and electromagnetic theory.
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Books on the topic "Terrestial Magnetism"

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Christie, S. Hunter. Report upon a letter addressed by M. Le Baron de Humboldt to His Royal Highness the president of the Royal Society, and communicated by His Royal Highness to the council. [S.l: s.n., 1986.

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Terrestrial magnetism. New York: Springer, 2011.

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Hulot, G., A. Balogh, U. R. Christensen, C. Constable, M. Mandea, and N. Olsen, eds. Terrestrial Magnetism. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-7955-1.

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Sierra, Malú. Elqui: El cielo está más cerca. Santiago, Chile: (s.n.), 1986.

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Trigg, D. F. The automatic magnetic observatory system AMOS III =: Le réseau d'observatoires magnétiques automatiques AMOS III. Ottawa: Energy, Mines and Resources Canada, Earth Physics Branch, 1985.

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Lefroy, J. H. Magnetical and meteorological observations at Lake Athabasca and Fort Simpson. London: Longman, Brown, Green, and Longmans, 1985.

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Gordon, Andrew. Methods and results of Toronto observations. [Hamilton, Ont.?: s.n., 1991.

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Zhdanov, M. S. Integral transforms in geophysics. Berlin: Springer-Verlag, 1987.

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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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Huaning, Wang, and Xu R. L, eds. Solar-terrestrial magnetic activity and space environment: Proceedings of the COSPAR Colloquium on Solar-Terrestrial Magnetic Activity and Space Environment (STMASE), held in the NAOC in Beijing, China, September 10-12, 2001. Oxford, UK: Pergamon, 2002.

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Book chapters on the topic "Terrestial Magnetism"

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Glassmeier, Karl-Heinz, and Joachim Vogt. "Magnetic Polarity Transitions and Biospheric Effects." In Terrestrial Magnetism, 387–410. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7955-1_14.

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Hulot, Gauthier, André Balogh, Ulrich R. Christensen, Catherine G. Constable, Mioara Mandea, and Nils Olsen. "The Earth’s Magnetic Field in the Space Age: An Introduction to Terrestrial Magnetism." In Terrestrial Magnetism, 1–7. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7955-1_1.

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Fournier, Alexandre, Gauthier Hulot, Dominique Jault, Weijia Kuang, Andrew Tangborn, Nicolas Gillet, Elisabeth Canet, Julien Aubert, and Florian Lhuillier. "An Introduction to Data Assimilation and Predictability in Geomagnetism." In Terrestrial Magnetism, 247–91. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7955-1_10.

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Amit, Hagay, Roman Leonhardt, and Johannes Wicht. "Polarity Reversals from Paleomagnetic Observations and Numerical Dynamo Simulations." In Terrestrial Magnetism, 293–335. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7955-1_11.

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Aubert, Julien, John A. Tarduno, and Catherine L. Johnson. "Observations and Models of the Long-Term Evolution of Earth’s Magnetic Field." In Terrestrial Magnetism, 337–70. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7955-1_12.

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Petrovay, K., and U. R. Christensen. "The Magnetic Sun: Reversals and Long-Term Variations." In Terrestrial Magnetism, 371–85. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7955-1_13.

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Gubbins, David. "Terrestrial Magnetism: Historical Perspectives and Future Prospects." In Terrestrial Magnetism, 9–27. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7955-1_2.

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Matzka, J., A. Chulliat, M. Mandea, C. C. Finlay, and E. Qamili. "Geomagnetic Observations for Main Field Studies: From Ground to Space." In Terrestrial Magnetism, 29–64. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7955-1_3.

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Olsen, N., G. Hulot, and T. J. Sabaka. "Measuring the Earth’s Magnetic Field from Space: Concepts of Past, Present and Future Missions." In Terrestrial Magnetism, 65–93. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7955-1_4.

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Thébault, Erwan, Michael Purucker, Kathryn A. Whaler, Benoit Langlais, and Terence J. Sabaka. "The Magnetic Field of the Earth’s Lithosphere." In Terrestrial Magnetism, 95–127. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7955-1_5.

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Conference papers on the topic "Terrestial Magnetism"

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Abramenko, V. I. "SELF-ORGANIZED CRITICALITY OF SOLAR MAGNETISM." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2019. http://dx.doi.org/10.31725/0552-5829-2019-3-6.

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Kutsenko, A. S. "DIFFERENTIAL ROTATION OF MAGNETIC STRUCTURES WITH DIFFERENT TOTAL UNSIGNED MAGNETIC FLUX." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2019. http://dx.doi.org/10.31725/0552-5829-2019-265-268.

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Feldman, William C. "Magnetic reconnection in the terrestrial magnetosphere." In AIP Conference Proceedings Volume 144. AIP, 1986. http://dx.doi.org/10.1063/1.35653.

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Kutsenko, O. K., A. S. Kutsenko, and V. I. Abramenko. "MAGNETIC POWER SPECTRA OF DECAYING ACTIVE REGIONS." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2019. http://dx.doi.org/10.31725/0552-5829-2019-269-272.

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Merzlyakov, V. L., and L. I. Starkova. "SOLAR CORONA EFFECTS OF MAGNETIC FIELD GENERATION." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2019. http://dx.doi.org/10.31725/0552-5829-2019-293-296.

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Kholtygin, A. F., A. V. Moiseeva, I. A. Yakunin, O. A. Tsiopa, and A. F. Valeev. "FAST STELLAR PULSATIONS AND LOCAL MAGNETIC FIELDS." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2020. http://dx.doi.org/10.31725/0552-5829-2020-317-320.

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Derteev, S. B., B. B. Mikhalyaev, and L. N. Dzhimbeeva. "MODEL OF CME WITH A HELICAL MAGNETIC FIELD." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2019. http://dx.doi.org/10.31725/0552-5829-2019-145-148.

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Zhivanovich, I., and A. A. Solov’ev. "DISTRIBUTION OF MAGNETIC FIELD IN BIPOLAR SUNSPOT GROUPS." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2019. http://dx.doi.org/10.31725/0552-5829-2019-173-176.

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Ramachandran, Narayanan. "A Terrestrial Microgravity Simulator Using Magnetic Levitation." In AIAA SPACE 2009 Conference & Exposition. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2009. http://dx.doi.org/10.2514/6.2009-6524.

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Merzlyakov, V. L., and L. I. Starkova. "EVOLUTION CHANGES OF MAGNETIC FIELD STRUCTURE OF SOLAR CORONA." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2018. http://dx.doi.org/10.31725/0552-5829-2018-287-290.

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Reports on the topic "Terrestial Magnetism"

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Hagerty, James D. Impedance Compensation Method for Giant Magneto-Impedance Magnetic Sensors to Null Out the Terrestrial Residual Magnetic Field. Fort Belvoir, VA: Defense Technical Information Center, October 2011. http://dx.doi.org/10.21236/ada557425.

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Boteler, D. H., G. Jansen van Beek, and J. Hruska. Magnetic activity in Canada during the solar- terrestrial disturbance of 24-25 March 1991. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 1995. http://dx.doi.org/10.4095/205060.

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You might also be interested in the extended bibliographies on the topic 'Terrestial Magnetism' for particular source types:
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