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1

Wen Yan, Wen Yan, Yuan Yao Yuan Yao, Yuxin Sun Yuxin Sun, Hoyt W. Chad Hoyt W. Chad, Yanyi Jiang Yanyi Jiang, and Longsheng Ma Longsheng Ma. "Zeeman slowing atoms using the magnetic field from a magneto-optical trap." Chinese Optics Letters 17, no. 4 (2019): 040201. http://dx.doi.org/10.3788/col201917.040201.

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2

Hou Yue, 侯越, 周湶 Zhou Quan, 欧阳希 Ouyang Xi, 陈伟根 Chen Weigen та 董润榆 Dong Runyu. "基于磁光晶体和光纤光栅的反射式磁场传感器". Acta Optica Sinica 44, № 11 (2024): 1128004. http://dx.doi.org/10.3788/aos240579.

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3

Liu Sichen, 刘思晨, 黄怿 Huang Yi, 邓传鲁 Deng Chuanlu та ін. "基于磁致折变效应的掺铒光纤磁场传感器温度特性研究". Chinese Journal of Lasers 49, № 9 (2022): 0910002. http://dx.doi.org/10.3788/cjl202249.0910002.

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4

Zhang Xuan, 张轩, 郝鹏 Hao Peng, 苏亚 Su Ya, 姚鹏辉 Yao Penghui та 姚晓天 Yao X. Steve. "基于磁光晶体的光纤三维磁场传感器研究". Laser & Optoelectronics Progress 60, № 9 (2023): 0928004. http://dx.doi.org/10.3788/lop220883.

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5

Rochalska, M., and A. Orzeszko-Rywka. "Magnetic field treatment improves seed performance." Seed Science and Technology 33, no. 3 (2005): 669–74. http://dx.doi.org/10.15258/sst.2005.33.3.14.

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6

TUROLLA, ROBERTO, and PAOLO ESPOSITO. "LOW-MAGNETIC-FIELD MAGNETARS." International Journal of Modern Physics D 22, no. 13 (2013): 1330024. http://dx.doi.org/10.1142/s0218271813300243.

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It is now widely accepted that soft gamma repeaters and anomalous X-ray pulsars are the observational manifestations of magnetars, i.e. sources powered by their own magnetic energy. This view was supported by the fact that these "magnetar candidates" exhibited, without exception, a surface dipole magnetic field (as inferred from the spin-down rate) in excess of the electron critical field (≃ 4.4×1013 G). The recent discovery of fully qualified magnetars, SGR 0418+5729 and Swift J1822.3-1606, with dipole magnetic field well in the range of ordinary radio pulsars posed a challenge to the standar
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Xing-yu WANG, 王星宇, 师振莲 Zhen-lian SHI, 李子亮 Zi-liang LI, 顾正宇 Zheng-yu GU, 王鹏军 Peng-jun WANG та 张靖 Jing ZHANG. "高偏置磁场下磁场空间分布对玻色爱因斯坦凝聚体自由飞行的影响". Acta Sinica Quantum Optica 28, № 1 (2022): 8. http://dx.doi.org/10.3788/jqo20222801.0501.

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8

Lim, Byeong-Seon, Sung-Pyo Hong, and Young-Kil Kim. "A Study on Actuation Probability of Underwater Weapon Based on Magnetic Field." Journal of the Korean Institute of Information and Communication Engineering 17, no. 5 (2013): 1253–58. http://dx.doi.org/10.6109/jkiice.2013.17.5.1253.

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9

Wu, Yan, Yan Lu, Xiang Zhao, and Liang Zuo. "Effects of Magnetic Field Intensity on Carbon Diffusion in Pure Iron in the Single-Phase Austenite Region." Materials Science Forum 706-709 (January 2012): 2372–77. http://dx.doi.org/10.4028/www.scientific.net/msf.706-709.2372.

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Effects of magnetic field intensity on carbon diffusion in pure iron in the single-phase austenite region were investigated. Specimens of high purity iron (99.99%) were buried in an air-proof melting pot filled up with cementation agent, and respectively subjected to isothermal annealing at 930° for 25 min with a heating rate of 5°C /min, and then cooled in the furnace. A magnetic field with different intensity was applied during the whole heating, isothermal holding and cooling processes. The results showed that the magnetic field annealing obviously hinders the carbon diffusion in the direct
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10

MOTOZAWA, Masaaki, Kyohei KINO, Tatsuo SAWADA, Yasuo KAWAGUCHI, and Mitsuhiro FUKUTA. "Effect of Magnetic Field Direction on Forced Convective Heat Transfer of Magnetic Fluid." Journal of the Japan Society of Applied Electromagnetics and Mechanics 23, no. 3 (2015): 612–17. http://dx.doi.org/10.14243/jsaem.23.612.

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11

Kangkang Lü, 吕康康, 刘兴 Liu Xing, 姜晨 Jiang Chen та ін. "基于磁流体包覆的长周期光纤光栅磁场传感器". Laser & Optoelectronics Progress 59, № 23 (2022): 2305001. http://dx.doi.org/10.3788/lop202259.2305001.

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12

Kuznetsov, B. I., T. B. Nikitina, I. V. Bovdui, K. V. Chunikhin, V. V. Kolomiets, and B. B. Kobylianskiy. "IMPROVE OF UNCERTAIN MICROSATELLITE MAGNETIC CLEANLINESS BASED ON MAGNETIC FIELD SPATIAL HARMONICS COMPENSATION." Tekhnichna Elektrodynamika 2025, no. 1 (2025): 3–11. https://doi.org/10.15407/techned2025.01.003.

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Problem of microsatellite magnetic cleanliness (MMC) improving by magnetic field (MF) spatial harmonics compensa-tion and magnetic characteristics uncertainty (MCU) sensitivity reducing considered. Prediction and control by uncer-tain microsatellite MC design are geometric inverse magneto static problem (GIMSP) reduced to vector game solution. Vector payoff calculated based on development method for analytical calculation of magnetostatic field induction of spherical sources in the Cartesian coordinate system (CCS) using Wolfram Mathematica ® software. Both vector game solution calculated base
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13

Fujisawa, Kotaro. "Magnetic field structures inside magnetars with strong toroidal field." Proceedings of the International Astronomical Union 9, S302 (2013): 423–26. http://dx.doi.org/10.1017/s1743921314002658.

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AbstractWe have analyzed the magnetized equilibrium studies with strong toroidal magnetic fields and found that the negative toroidal current density inside the star is very important for the strong toroidal magnetic fields. The strong toroidal magnetic fields require the strong poloidal current, but the strong poloidal current results in the localized strong toroidal current density in the axisymmetric system. This localized toroidal current changes the magnetic field configuration and makes the size of the toroidal magnetic field region smaller. As a result, the toroidal magnetic field energ
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14

Zhiyan, Zhang, Xie Zehui, Ma Hongzhong, and Qin Zhong. "ANALYSIS OF DEMAGNETIZATION FAULT BACK-EMF OF PERMANENT MAGNET SYNCHRONOUS MOTOR USING MATHEMATICAL MODEL BASED ON MAGNETIC FIELD SUPERPOSITION PRINCIPLE." Tekhnichna Elektrodynamika 2016, no. 2 (2016): 42–48. http://dx.doi.org/10.15407/techned2016.02.042.

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15

Lambri, O. A., D. Gargicevich, F. Tarditti, et al. "Magnetic Field Dependent Damping of Magnetic Particle Filled Polypropylene." Solid State Phenomena 184 (January 2012): 449–54. http://dx.doi.org/10.4028/www.scientific.net/ssp.184.449.

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The behavior of internal friction Q-1 and dynamic shear modulus has been studied in polypropylene charged with either different volume fraction or size of magnetite (Fe3O4) particles, as a function of the applied magnetic field at 318 K. An increase of the alternating (AC) magnetic field oscillating with 50 Hz, leads to an increase of the internal friction. In addition, during the subsequently decreasing alternating magnetic field, the internal friction decreases, but a hysteretic behavior appeared. In fact, the internal friction of the decreasing part of magnetic field amplitude is found to b
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16

Motozawa, Masaaki, Yuta Iizuka, and Tatsuo Sawada. "OS8-2-2 Ultrasonic analysis of clustering structures in magnetic fluid under magnetic field." Abstracts of ATEM : International Conference on Advanced Technology in Experimental Mechanics : Asian Conference on Experimental Mechanics 2007.6 (2007): _OS8–2–2–1—_OS8–2–2–5. http://dx.doi.org/10.1299/jsmeatem.2007.6._os8-2-2-1.

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17

Петухова, Анастасия, Anastasia Petukhova, Станислав Петухов, and Stanislav Petukhov. "Toroidal models of magnetic field with twisted structure." Solar-Terrestrial Physics 5, no. 2 (2019): 69–75. http://dx.doi.org/10.12737/stp-52201910.

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We present and discuss properties of the following magnetic field models in a magnetic cloud: Miller and Turner solution, modified Miller–Turner solution, Romashets–Vandas toroidal and integral models, and Krittinatham–Ruffolo model. Helicity of the magnetic field in all the models is the main feature of magnetic clouds. The first three models describe the magnetic field inside an ideal torus. In the integral model, parameters of a generating torus ambiguously determine the volume and form of the magnetic field region. In the Krittinatham–Ruffolo model, the cross-section radius of the torus is
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18

Samofalov, V. N. "Peculiarities of galvanomagnetic effects in nonhomogeneous magnetic field." Functional materials 25, no. 2 (2018): 289–93. http://dx.doi.org/10.15407/fm25.02.289.

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19

Pratap Singh, Aditya. "Flow Control Using Magnetic Field in Diverging Microchannel." International Journal of Science and Research (IJSR) 12, no. 5 (2023): 2360–69. http://dx.doi.org/10.21275/sr23526151806.

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20

Kojima, Yasufumi. "Magnetic field evolution in magnetars and its implication to accreting system." Proceedings of the International Astronomical Union 8, S290 (2012): 235–36. http://dx.doi.org/10.1017/s1743921312019783.

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AbstractThe evolution of magnetic field is numerically studied for an isolated magnetar, assuming vacuum exterior. Nonlinear coupling between poloidal and toroidal components of the magnetic field can be seen in the initial Hall-drift timescale. Consequently, the polar field at the surface is highly distorted during the phase. This result is suggestive. Fixed dipole magnetic field has been used so far in the theoretical study of the interaction between magnetosphere and accreting matter. In the accretion to magnetar, time-dependent polar magnetic field should be taken into account.
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21

Li Yongqian, 李永倩, 温芳芳 Wen Fangfang та 王劭龙 Wang Shaolong. "基于磁流体的温度磁场测量技术研究进展". Laser & Optoelectronics Progress 59, № 5 (2022): 0500003. http://dx.doi.org/10.3788/lop202259.0500003.

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22

Volkov, O. M., and V. P. Kravchuk. "Saturation of Magnetic Films with Spin-Polarized Current in the Presence of a Magnetic Field." Ukrainian Journal of Physics 58, no. 7 (2013): 666–72. http://dx.doi.org/10.15407/ujpe58.07.0666.

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23

Wang, Yonliang, Yongbo Wu, and Mitsuyoshi Nomura. "2206 Magnetic field-assisted polishing of miniature V-grooves using MCF(Magnetic Compound Fluid) slurry." Proceedings of International Conference on Leading Edge Manufacturing in 21st century : LEM21 2015.8 (2015): _2206–1_—_2206–5_. http://dx.doi.org/10.1299/jsmelem.2015.8._2206-1_.

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24

Fujisawa, Kotaro, Akihiro Yatabe, and Shota Kisaka. "Magnetic field configurations of magnetars." Proceedings of the International Astronomical Union 13, S337 (2017): 334–35. http://dx.doi.org/10.1017/s1743921317008997.

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AbstractWe evaluated ambipolar diffusion velocity in a magnetar. Previous studies concerning ambipolar diffusion ignored the presence of the crust, although a magnetar has both core and crust. We considered both core and crust and examined the influence of the crust in this study. We found that the crustal magnetic field can accelerate the ambipolar diffusion in its core.
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25

Ji, Hongzhu, Shengli Pu, Xiang Wang, Guojun Yu, Ning Wang, and Haotian Wang. "Magnetic field sensing based on capillary filled with magnetic fluids." Applied Optics 51, no. 27 (2012): 6528. http://dx.doi.org/10.1364/ao.51.006528.

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26

Kovalevskyy, Sergiy, and Olena Kovalevska. "NEW OPPORTUNITIES FOR PROCESSING MATERIALS IN STRONG MAGNETIC FIELD." Technical Sciences and Technologies, no. 4(26) (2021): 7–14. http://dx.doi.org/10.25140/2411-5363-2021-4(26)-7-14.

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The article shows the most important results of new studies concerning the possibility of influencing the physical and mechanical indicators of the hardness of steel and carbide materials, presented in the form of dimensional samples and non-sharp-ened cutting tool inserts. The main differences in the process of volumetric hardening of articles made of magnetically permeable materials are presented -resonant vibrations with amplitudes commensurate with the subatomic dimensions of the hardened materials. Some results of metallographic studies confirming the structural changes in the material of
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27

Demchenko, V. F., I. V. Krivtsun, I. V. Krikent, and I. V. Shuba. "Force interaction of arc current with self-magnetic field." Paton Welding Journal 2017, no. 3 (2017): 15–24. http://dx.doi.org/10.15407/tpwj2017.03.03.

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28

Bondar, E. A., and D. A. Luzhbin. "Effect of Magnetic Field on Electrodeposition of Nanosize Structures." METALLOFIZIKA I NOVEISHIE TEKHNOLOGII 40, no. 5 (2018): 615–23. http://dx.doi.org/10.15407/mfint.40.05.0615.

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29

Elhag, A., K. Ayuel, and A. AlQarni. "Crystal Field Analysis of the Magnetic Anisotropy of CeAgAs2." International Journal of Scientific Engineering and Research 12, no. 5 (2024): 1–8. https://doi.org/10.70729/se24429220145.

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30

Zyoud, Samer H., and Atef Abdelkader. "Characteristics of Semiconductors Laser Under Influence of Magnetic Field." Journal of Advanced Research in Dynamical and Control Systems 11, no. 10-SPECIAL ISSUE (2019): 682–89. http://dx.doi.org/10.5373/jardcs/v11sp10/20192858.

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31

Dzhala, R. M., V. R. Dzhala, M. I. Melnyk, B. I. Horon, and O. I. Senyuk. "Influence of the pipe defect on its magnetic field." Information extraction and processing 2018, no. 46 (2018): 5–10. http://dx.doi.org/10.15407/vidbir2018.46.005.

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32

GAO, ZHI FU, NA WANG, QIU HE PENG, XIANG DONG LI, and YUAN JIE DU. "PRESSURE OF DEGENERATE AND RELATIVISTIC ELECTRONS IN A SUPERHIGH MAGNETIC FIELD." Modern Physics Letters A 28, no. 36 (2013): 1350138. http://dx.doi.org/10.1142/s0217732313501381.

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Based on our previous work, we deduce a general formula for pressure of degenerate and relativistic electrons, Pe, which is suitable for superhigh magnetic fields, discuss the quantization of Landau levels of electrons, and consider the quantum electrodynamic (QED) effects on the equations of states (EOSs) for different matter systems. The main conclusions are as follows: Pe is related to the magnetic field B, matter density ρ, and electron fraction Ye; the stronger the magnetic field, the higher the electron pressure becomes; the high electron pressure could be caused by high Fermi energy of
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33

V P, Dudarev. "Magnetic Levitation, Based on the Weakening of the Effect of One of the Magnetic Fields on the source of another Magnetic Field when Two Magnetic Fields Interact." Advances in Theoretical & Computational Physics 8, no. 1 (2025): 01–04. https://doi.org/10.33140/atcp.08.01.07.

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The article discusses the device and method of creating an electromagnetic force having a strictly defined action vector. In conventional electromagnetic suspensions, the magnetic field created by the electric charges of one conductor acts on the electric charges of another conductor, while a force arises in it. The second conductor creates its own magnetic field, which acts on the charges of the first conductor and creates a counteracting force. In this case, two acting opposite forces balance each other in the system under consideration. The proposed design separates the paths of propagation
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34

Yushchenko, K. A., A. V. Mats, I. M. Neklyudov, V. I. Sokolenko, and N. A. Chernyak. "Effect of alternating magnetic field on magnetic properties, structure and stressed state of vessel steel welded joints." Paton Welding Journal 2017, no. 4 (2017): 10–13. http://dx.doi.org/10.15407/tpwj2017.04.02.

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35

Singh, Palwinder. "Modern Developments in Magnetic Field Assisted Abrasive Flow Machining Processes." Journal of Advanced Research in Production and Industrial Engineering 06, no. 01 (2019): 1–7. http://dx.doi.org/10.24321/2456.429x.201901.

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36

Lin, Haobin, Ce Feng, Yang Dong, et al. "Simultaneous temperature and magnetic field measurements using time-division multiplexing." Chinese Optics Letters 21, no. 1 (2023): 011201. http://dx.doi.org/10.3788/col202321.011201.

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37

Hijab, Basim. "NEW INTERPRETATION OF THE EARTH’S MAGNETIC FIELD EFFECTS’ ON LIFE." Iraqi Geological Journal 53, no. 2C (2020): 13–25. http://dx.doi.org/10.46717/igj.53.2c.2rs-2020-09-02.

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The relationships of the Earth’s magnetic field intensity and time (the past 320 years) for many locations around the world are obtained, based on the IGRF-13 mathematical model. The results showed that each location on the earth surface has its magnetic intensity relation with time that reflects local variations. The sudden changes (magnetic anomalies) in the Earth’s magnetic field with time are natural phenomena, which are different from place to another. These magnetic anomalies are investigated for possible relationship to the historical records of the influenza pandemic outbreaks. The res
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38

Zhilisbayeva, K., N. Doszhan, and A. Saspayeva. "Changing the magnetic field intensity during the motion of spacecraft." International Journal of Mathematics and Physics 7, no. 1 (2016): 56–64. http://dx.doi.org/10.26577/2218-7987-2016-7-1-56-64.

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39

Korotchenkov, O. O. "Magnetic field-stimulated change of photovoltage in solar silicon crystals." Semiconductor Physics Quantum Electronics and Optoelectronics 16, no. 1 (2013): 72–75. http://dx.doi.org/10.15407/spqeo16.01.072.

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40

Guglielmi, Anatol, Feliks Feygin, and Alexander Potapov. "Ponderomotive redistribution of heavy ions along a magnetic field line." Solar-Terrestrial Physics 10, no. 4 (2024): 14–18. https://doi.org/10.12737/stp-104202402.

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We set up the problem of ponderomotive separation and acceleration of ions with different charge-to-mass ratios under the influence of Alfvén waves, which constantly exist in the magnetosphere in the form of geomagnetic pulsations. Formulas for partial ponderomotive forces acting on light and heavy (metallic) ions are derived. In the quasi-hydrodynamic approximation, a system of equations is obtained which describes the distribution of ions along magnetic field lines in Earth’s magnetosphere. The Clarke number, which characterizes plasma metallicity, is found to be maximum at a minimum magneti
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41

Kolesnyk, Ihor. "Installation for Sintering Metal Powders in a Constant Magnetic Field." International Journal of Science and Research (IJSR) 10, no. 2 (2021): 1169–71. https://doi.org/10.21275/sr21210134754.

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42

Lukiyanets, B., and D. Matulka. "Effect of magnetic field on quantum capacitance of the nanoobject." Mathematical Modeling and Computing 2, no. 2 (2015): 176–82. http://dx.doi.org/10.23939/mmc2015.02.176.

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43

Мордвинов, Александр, Aleksandr Mordvinov, Алексей Певцов, et al. "The reversal of the Sun’s magnetic field in cycle 24." Solar-Terrestrial Physics 2, no. 1 (2016): 3–18. http://dx.doi.org/10.12737/19856.

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Analysis of synoptic data from the Vector Spectromagnetograph (VSM) of the Synoptic Optical Long-term Investigations of the Sun (SOLIS) and the NASA/NSO Spectromagnetograph (SPM) at the NSO/Kitt Peak Vacuum Telescope facility shows that the reversals of solar polar magnetic fields exhibit elements of a stochastic process, which may include the development of specific patterns of emerging magnetic flux, and the asymmetry in activity between Northern and Southern hemispheres. The presence of such irregularities makes the modeling and prediction of polar field reversals extremely hard if possible
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44

Jia Lingyan, 贾灵艳, 梁丽丽 Liang Lili, 谢飞 Xie Fei та ін. "基于磁致伸缩棒的干涉型微纳光纤磁场传感器". Laser & Optoelectronics Progress 60, № 7 (2023): 0728003. http://dx.doi.org/10.3788/lop220893.

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45

Dyakin, V. V., O. V. Kudryaschova, and V. Y. Raevskii. "Calculation of the magnetic field strength from a semi-infinite cylinder placed in an arbitrary external field." Дефектоскопия, no. 5 (May 15, 2023): 32–44. http://dx.doi.org/10.31857/s0130308223050044.

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In the model of the semi-infinite cylinder the formulas and the corresponding algorithm for finding the magnetic field strength inside and outside the homogeneous cylinder placed in the external magnetic field of arbitrary configuration are deduced. Testing the results of calculations on these formulas for their correspondence with known physical laws, as well as on their coincidence with well-known analytical answers in the limiting private cases of the forms of magnetics were carried out.
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46

Yakovlev, Dmitry. "Zeeman Splitting of Torsional Oscillation Frequencies of Magnetars." Universe 9, no. 12 (2023): 504. http://dx.doi.org/10.3390/universe9120504.

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Magnetars form a special class of neutron stars possessing superstrong magnetic fields and demonstrating power flares triggered by these fields. Observations of such flares reveal the presence of quasi-periodic oscillations (QPOs) at certain frequencies; they are thought to be excited in the flares. QPOs carry potentially important information on magnetar structure, magnetic field, and mechanisms of magnetar activity. We calculate frequencies of torsional (magneto-elastic) oscillations of the magnetar crust treating the magnetic field effects in the first order of perturbation theory. The theo
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47

Kojima, Yasufumi. "Correct Criterion of Crustal Failure Driven by Intense Magnetic Stress in Neutron Stars." Astrophysical Journal 974, no. 1 (2024): 125. http://dx.doi.org/10.3847/1538-4357/ad7382.

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Abstract Magnetar outbursts are powered by an intense magnetic field. The phenomenon has recently drawn significant attention because of a connection to some fast radio bursts that has been reported. Understanding magnetar outbursts may provide the key to mysterious transient events. The elastic deformation of the solid crust due to magnetic field evolution accumulates over a secular timescale. Eventually, the crust fractures or responds plastically beyond a particular threshold. Determination of the critical limit is required to obtain the shear strain tensor in response to magnetic stress. I
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48

Yang, Sheng Qiang, Wen Hui Li, Hong Ling Chen, and Jin Yu Guo. "The Design and Simulation of the Magnetic Field Formation Components Based on the Technology of Electro Permanent Magnet." Key Engineering Materials 579-580 (September 2013): 781–86. http://dx.doi.org/10.4028/www.scientific.net/kem.579-580.781.

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As a typical kind of surface finishing technology, magnetic abrasive finishing has unique advantages in finishing effect, efficiency and application, it occupies a very important position and has huge potential application value. As the core component of the magnetic abrasive finishing, the magnetic field formation components have a direct impact on the finishing effect and efficiency. Electro permanent magnetic field formation components used in magnetic abrasive finishing are put forward based on the characteristics of electro permanent magnet and its application in crane and clutch. Analyzi
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49

Aoki, Yuta. "High magnetic field pulsars with magnetar-like activity." Proceedings of the International Astronomical Union 8, S291 (2012): 351. http://dx.doi.org/10.1017/s1743921312024076.

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AbstractTo study the origin of magnetars, a unique opportunity is provided by detecting an excess of X-ray thermal radiation of the radio pulsars (rotation powered pulsars) with dipolar magnetic fields as high as magnetars. The excess is probably caused by decay of the magnetic field as seen in magnetars. In order to investigate whether the rotation powered pulsars have the excess flux and the hard-tail component similar to magnetars, we observed PSR J0726-2612 which has a 3.44 s period and a 3 × 1013 G inferred dipolar magnetic field, with Suzaku for 44 ks on 2011 November 16-17. We report th
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50

Rea, N., D. Viganò, G. L. Israel, J. A. Pons, and D. F. Torres. "3XMM J185246.6+003317: ANOTHER LOW MAGNETIC FIELD MAGNETAR." Astrophysical Journal 781, no. 1 (2014): L17. http://dx.doi.org/10.1088/2041-8205/781/1/l17.

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