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Journal articles on the topic 'Magnetic blowout'

Author: Grafiati

Published: 28 June 2021

Last updated: 3 February 2022

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1

Drake, J. F., and G. R. Burkhart. "Magnetic blowout during collisionless reconnection." Geophysical Research Letters 19, no. 11 (1992): 1077–80. http://dx.doi.org/10.1029/92gl01034.

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2

Tomisaka, Kohji. "Blowout of superbubble in Galactic magnetic field." Astrophysical Journal 361 (September 1990): L5. http://dx.doi.org/10.1086/185814.

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3

Sweet, David, Edward Ott, Thomas M. Antonsen, Daniel P. Lathrop, and John M. Finn. "Blowout bifurcations and the onset of magnetic dynamo action." Physics of Plasmas 8, no. 5 (2001): 1944–52. http://dx.doi.org/10.1063/1.1342228.

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4

Cong, Shen, Zhi Hai Fan, Dong Feng Li, Ke Tong, and Nan Ji. "Fracture Failure Analysis of the Blowout Preventer Ram in an Oilfield." Materials Science Forum 1035 (June 22, 2021): 458–63. http://dx.doi.org/10.4028/www.scientific.net/msf.1035.458.

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This paper gives a thorough investigation on the fracture failure of the blowout preventer (BOP) ram. Through appearance inspection, magnetic powder inspection, physicochemical inspection, metallographic inspection and scanning electron microscope (SEM), the main fracture reason of the BOP ram is that there was some original cracks in the BOP ram before fracture, during the service process the bop ram is subjected to impact load, therefore brittle fracture occurs due to the high brittleness of the gate material (which is caused by large internal structure) and low anti-crack propagation abilit

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5

Bellan, P. M., and J. W. Higley. "Magnetic suppression of arc blowout in a model arc furnace." IEEE Transactions on Plasma Science 20, no. 6 (1992): 1026–35. http://dx.doi.org/10.1109/27.199568.

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6

Yanik, Bahar, Bahri Keyik, Isik Conkbayir, and M. Akif Teber. "Carotid blowout syndrome with oronasal hemorrhage: magnetic resonance imaging findings." Japanese Journal of Radiology 29, no. 1 (2011): 72–75. http://dx.doi.org/10.1007/s11604-010-0503-4.

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7

Rojek, Artur. "An experimental analysis of DC magnetic blowout high-speed circuit breakers’ parameters." Eastern-European Journal of Enterprise Technologies 4, no. 5 (106) (2020): 35–40. http://dx.doi.org/10.15587/1729-4061.2020.210232.

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8

Jones, Douglas L., Gus L. Hoehn, and Arthur F. Kuckes. "Improved Magnetic Model for Determination of Range and Direction to a Blowout Well." SPE Drilling Engineering 2, no. 04 (1987): 316–22. http://dx.doi.org/10.2118/14388-pa.

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9

Nishida, Y. "Diagnosis of Magnetic Resonance Imaging (MRI) for Blowout FractureâThree Advantages of MRI." Japanese Journal of Ophthalmology 43, no. 5 (1999): 446. http://dx.doi.org/10.1016/s0021-5155(99)00073-8.

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10

Zhu, Xiaoshuai, Huaning Wang, Xin Cheng, and Chong Huang. "A Solar Blowout Jet Caused by the Eruption of a Magnetic Flux Rope." Astrophysical Journal 844, no. 2 (2017): L20. http://dx.doi.org/10.3847/2041-8213/aa8033.

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11

TASHIRO, Shinichi, Shuichi ITODA, Takahiro MORICHI, MURPHY B. Anthony, and Manabu TANAKA. "Numerical simulation of magnetic blowout process of air arc plasma in electrical contacts." QUARTERLY JOURNAL OF THE JAPAN WELDING SOCIETY 38, no. 2 (2020): 74s—78s. http://dx.doi.org/10.2207/qjjws.38.74s.

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12

Cai, Baoping, Yonghong Liu, Xiaojie Tian, et al. "Optimization of Submersible Solenoid Valves for Subsea Blowout Preventers." IEEE Transactions on Magnetics 47, no. 2 (2011): 451–58. http://dx.doi.org/10.1109/tmag.2010.2100825.

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13

Cox, Donald P. "Structure of the Diffuse Interstellar Medium." International Astronomical Union Colloquium 120 (1989): 500–510. http://dx.doi.org/10.1017/s0252921100024313.

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ABSTRACTThe interstellar medium has a thick disk structure (|z | ≲ 1500 pc, the ECL or extracloud layer) with a thin zone of cloud contamination at |z | ≲ 100 pc. The properties of all components other than clouds (e.g. cosmic rays, magnetic field, extracloud matter, pressure) drop slowly with |z| across the thick distribution, giving this layer a very important influence in the evolution of superbubbles. It seems likely to quench blowout or breakout and virtually all fountain activity. The weight of this layer stabilizes the clouds at low z; its high pressure and low density provide a cushion

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14

Poletto, Giannina, Alphonse C. Sterling, Stefano Pucci, and Marco Romoli. "The contribution of X-ray polar blowout jets to the solar wind mass and energy." Proceedings of the International Astronomical Union 8, S300 (2013): 239–42. http://dx.doi.org/10.1017/s1743921313011046.

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AbstractBlowout jets constitute about 50% of the total number of X-ray jets observed in polar coronal holes. In these events, the base magnetic loop is supposed to blow open in what is a scaled-down representation of two-ribbon flares that accompany major coronal mass ejections (CMEs): indeed, miniature CMEs resulting from blowout jets have been observed. This raises the question of the possible contribution of this class of events to the solar wind mass and energy flux. Here we make a first crude evaluation of the mass contributed to the wind and of the energy budget of the jets and related m

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15

Vourlidas, Angelos, and David F. Webb. "Streamer-blowout Coronal Mass Ejections: Their Properties and Relation to the Coronal Magnetic Field Structure." Astrophysical Journal 861, no. 2 (2018): 103. http://dx.doi.org/10.3847/1538-4357/aaca3e.

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16

Ito, Shokichi, Yoshihiro Kawase, and Satoshi Tatsuoka. "3-D Finite Element Analysis of Magnetic Blowout Forces on the Arc in Molded Case Circuit Breakers." IEEJ Transactions on Power and Energy 113, no. 10 (1993): 1100–1105. http://dx.doi.org/10.1541/ieejpes1990.113.10_1100.

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17

Kawase, Y., H. Mori, H. Inoue, and S. Ito. "3-D finite element analysis of magnetic blowout forces acting on the arc in vacuum circuit breakers." IEEE Transactions on Magnetics 32, no. 3 (1996): 1681–84. http://dx.doi.org/10.1109/20.497579.

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18

Moore, Ronald L., and Alphonse C. Sterling. "The Coronal‐dimming Footprint of a Streamer‐Puff Coronal Mass Ejection: Confirmation of the Magnetic‐Arch‐Blowout Scenario." Astrophysical Journal 661, no. 1 (2007): 543–50. http://dx.doi.org/10.1086/516620.

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19

Ito, S., Y. Kawase, and H. Mori. "3-D finite element analysis of magnetic blowout forces acting on the arc in molded case circuit breakers." IEEE Transactions on Magnetics 33, no. 2 (1997): 2053–56. http://dx.doi.org/10.1109/20.582717.

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20

Timur, Emre. "Magnetic susceptibility and VLF-R investigations for determining geothermal blowout contaminated area: a case study from Alaşehir (Manisa/Turkey)." Environmental Earth Sciences 72, no. 7 (2014): 2497–510. http://dx.doi.org/10.1007/s12665-014-3158-0.

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21

Cox, D. P. "Characteristics of the diffuse interstellar medium." Symposium - International Astronomical Union 147 (1991): 3–10. http://dx.doi.org/10.1017/s0074180900198705.

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There have been several recent changes in perspective on the diffuse interstellar environment, including recognition of a thick disk of warm gas, cosmic rays, and magnetic field. In addition, evidence for a pervasive hot phase driven by supernova disruption has weakened to the point that a quasihomogeneous warm intercloud gas may occupy most of the interstellar volume at midplane, with individual bubbles created by supernovae and OB associations occupying perhaps 10 and 20 per cent respectively. The bubble population is sufficient to explain the high stage ions (0 VI, N V, C IV, perhaps Si IV)

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22

Cox, D. P. "Characteristics of the diffuse interstellar medium." Symposium - International Astronomical Union 147 (1991): 3–10. http://dx.doi.org/10.1017/s0074180900239326.

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There have been several recent changes in perspective on the diffuse interstellar environment, including recognition of a thick disk of warm gas, cosmic rays, and magnetic field. In addition, evidence for a pervasive hot phase driven by supernova disruption has weakened to the point that a quasihomogeneous warm intercloud gas may occupy most of the interstellar volume at midplane, with individual bubbles created by supernovae and OB associations occupying perhaps 10 and 20 per cent respectively. The bubble population is sufficient to explain the high stage ions (0 VI, N V, C IV, perhaps Si IV)

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23

Mankin, Henry J., Francis J. Hornicek, Eduardo Ortiz-Cruz, Jorge Villafuerte, and Mark C. Gebhardt. "Aneurysmal Bone Cyst: A Review of 150 Patients." Journal of Clinical Oncology 23, no. 27 (2005): 6756–62. http://dx.doi.org/10.1200/jco.2005.15.255.

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PurposeWe have reviewed a series of 150 aneurysmal bone cysts treated over the last 20 years.Patients and MethodsThe lesions were principally located in the tibia, femur, pelvis, humerus, and spine and, in most cases, presented the imaging appearance originally described by Jaffe and Lichtenstein as a blowout with thin cortices.ResultsOnly one of the patients was believed to have an osteoblastoma of the spine with secondary development of an aneurysmal bone cyst, and none of the patients developed additional lesions. The patients were treated primarily with curettage and implantation of allogr

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24

Zuo, Shuguang, Duoqiang Li, Yu Mao, and Wenzhe Deng. "Longitudinal vibration analysis and suppression of electric wheel system driven by in-wheel motor considering unbalanced magnetic pull." Proceedings of the Institution of Mechanical Engineers, Part D: Journal of Automobile Engineering 233, no. 11 (2018): 2729–45. http://dx.doi.org/10.1177/0954407018806118.

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With the blowout of electric vehicles recently, the key parts of the electric vehicles driven by in-wheel motors named the electric wheel system become the core of development research. The torque ripple of the in-wheel motor mainly results in the longitudinal dynamics of the electric wheel system. The excitation sources are first analyzed through the finite element method, including the torque ripple induced by the in-wheel motor and the unbalanced magnetic pull produced by the relative motion between the stator and rotor. The accuracy of the finite element model is verified by the back elect

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25

Wang, Q. Daniel. "Chandra large-scale mapping of the Galactic Centre: probing high-energy structures around the central molecular zone." Monthly Notices of the Royal Astronomical Society 504, no. 2 (2021): 1609–18. http://dx.doi.org/10.1093/mnras/stab801.

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ABSTRACT Recent observations have revealed interstellar features that apparently connect energetic activity in the central region of our Galaxy to its halo. The nature of these features, however, remains largely uncertain. We present a Chandra mapping of the central 2° × 4° field of the Galaxy, revealing a complex of X-ray-emitting threads plus plume-like structures emerging from the Galactic Centre (GC). This mapping shows that the northern plume or fountain is offset from a well-known radio lobe (or the GCL), which however may represent a foreground H ii region, and that the southern plume i

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26

Zhang, Q. M. "Simultaneous transverse oscillations of a coronal loop and a filament excited by a circular-ribbon flare." Astronomy & Astrophysics 642 (October 2020): A159. http://dx.doi.org/10.1051/0004-6361/202038557.

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Aims. The aim of this study is to investigate the excitation of kink oscillations in coronal loops and filaments, by analyzing a C3.4 circular-ribbon flare associated with a blowout jet in active region 12434 on 2015 October 16. Methods. The flare was observed in ultraviolet and extreme-ultraviolet wavelengths by the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory (SDO) spacecraft. The line-of-sight (LOS) magnetograms of the photosphere were observed by the Helioseismic and Magnetic Imager on board SDO. Soft X-ray fluxes of the flares in 0.5−4 and 1−8 Å were recorded by th

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27

Low, B. C. "Blowup of force-free magnetic fields in the infinite region of space." Astrophysical Journal 307 (August 1986): 205. http://dx.doi.org/10.1086/164407.

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28

Pouchain, Ernest Cavalcante, Vanessa Anastacio Pimentel, Roque Soares Martins Neto, et al. "Alterações funcionais como consequências de traumatismo orbitário: revisão da literatura." ARCHIVES OF HEALTH INVESTIGATION 9, no. 5 (2020): 464–67. http://dx.doi.org/10.21270/archi.v9i5.4787.

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Os traumas de face ocorrem por forças externas lesionando o corpo, podendo eles ser locais, gerais ou concomitantes. A etiologia do traumatismo orbitário é diversificada como: quedas, queimaduras e agressões, sendo considerada uma das principais causas de morte no mundo de acordo com Organização Mundial da Saúde (OMS). As fraturas faciais podem se dividir em fraturas dos terço superior, terço médio e terço inferior. As fraturas do tipo Blow-outmantêm as margens orbitais integra, envolvendo apenas parede orbital inferior e ou média. Diplopia e enoftalmia são complicações bem características de

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29

Kurkina, E. S., Yu V. Troshchiev, V. A. Kovalev, and E. D. Kuretova. "Small-Scale Heat Localization with Blowup in the Magnetic-Tube Cross Section During a Solar Flare." Computational Mathematics and Modeling 27, no. 4 (2016): 395–416. http://dx.doi.org/10.1007/s10598-016-9330-5.

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30

Choe, Jinhoon, and Wenting Sun. "Blowoff hysteresis, flame morphology and the effect of plasma in a swirling flow." Journal of Physics D: Applied Physics 51, no. 36 (2018): 365201. http://dx.doi.org/10.1088/1361-6463/aad4dc.

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31

Sweet, David, Edward Ott, John M. Finn, Thomas M. Antonsen, and Daniel P. Lathrop. "Blowout bifurcations and the onset of magnetic activity in turbulent dynamos." Physical Review E 63, no. 6 (2001). http://dx.doi.org/10.1103/physreve.63.066211.

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32

Olsson, P., and S. Teitel. "Search for a vortex loop blowout transition in a type-II superconductor in a finite magnetic field." Physical Review B 67, no. 14 (2003). http://dx.doi.org/10.1103/physrevb.67.144514.

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33

Bhowmik, P., and A. R. Yeates. "Two Classes of Eruptive Events During Solar Minimum." Solar Physics 296, no. 7 (2021). http://dx.doi.org/10.1007/s11207-021-01845-x.

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AbstractDuring solar minimum, the Sun is relatively inactive with few sunspots observed on the solar surface. Consequently, we observe a smaller number of highly energetic events such as solar flares or coronal mass ejections (CMEs), which are often associated with active regions on the photosphere. Nonetheless, our magnetofrictional simulations during the minimum period suggest that the solar corona is still dynamically evolving in response to the large-scale shearing velocities on the solar surface. The non-potential evolution of the corona leads to the accumulation of magnetic free energy a

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34

Kim, Hee-Cheol, Minsung Kim, Sung-Soo Kim, and Ki-Hong Lee. "Bootstrapping BPS spectra of 5d/6d field theories." Journal of High Energy Physics 2021, no. 4 (2021). http://dx.doi.org/10.1007/jhep04(2021)161.

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Abstract We propose a systematic approach to computing the BPS spectrum of any 5d/6d supersymmetric quantum field theory in Coulomb phases, which admits either gauge theory descriptions or geometric descriptions, based on the Nakajima-Yoshioka’s blowup equations. We provide a significant generalization of the blowup equation approach in terms of both properly quantized magnetic fluxes on the blowup $$ \hat{\mathrm{\mathbb{C}}} $$ ℂ ̂ 2 and the effective prepotential for 5d/6d field theories on the Omega background which is uniquely determined by the Chern-Simons couplings on their Coulomb bran

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