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Journal articles on the topic 'Reconfinement'

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1

Bietry, Guillaume. "Un reconfinement allégé face à la deuxième vague." Soins 65, no. 849 (October 2020): 5. http://dx.doi.org/10.1016/s0038-0814(20)30224-3.

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2

Nalewajko, Krzysztof. "Dissipation efficiency of reconfinement shocks in relativistic jets." Monthly Notices of the Royal Astronomical Society: Letters 420, no. 1 (December 20, 2011): L48—L52. http://dx.doi.org/10.1111/j.1745-3933.2011.01193.x.

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3

Nalewajko, Krzysztof. "Polarization of synchrotron emission from relativistic reconfinement shocks." Monthly Notices of the Royal Astronomical Society 395, no. 1 (May 1, 2009): 524–30. http://dx.doi.org/10.1111/j.1365-2966.2009.14559.x.

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4

de Thé, Priscille. "Confinement, déconfinement, reconfinement, où est donc le nord ?" Contraste N° 53, no. 1 (March 17, 2021): 163–71. http://dx.doi.org/10.3917/cont.053.0163.

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5

Falle, S. A. E. G., and M. J. Wilson. "M87: an example of a reconfining jet." Canadian Journal of Physics 64, no. 4 (April 1, 1986): 470–73. http://dx.doi.org/10.1139/p86-086.

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A model is presented to explain the observed positions of the knots in the jet of the radio source M87. It is supposed that the knots represent shocks in a supersonic fluid jet caused by a pressure imbalance between the jet and the surrounding medium. The positions of the knots are determined by the product of the jet's Mach number and radius, and by the variation in the external pressure, which brings about a reconfinement of the jet.
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6

Nalewajko, Krzysztof, and Marek Sikora. "A structure and energy dissipation efficiency of relativistic reconfinement shocks." Monthly Notices of the Royal Astronomical Society 392, no. 3 (January 21, 2009): 1205–10. http://dx.doi.org/10.1111/j.1365-2966.2008.14123.x.

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7

Levinson, A., and N. Globus. "Reconfinement of highly magnetized jets: implications for HST-1 in M87." Monthly Notices of the Royal Astronomical Society 465, no. 2 (November 10, 2016): 1608–12. http://dx.doi.org/10.1093/mnras/stw2902.

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8

Gourgouliatos, Konstantinos N., and Serguei S. Komissarov. "Reconfinement and loss of stability in jets from active galactic nuclei." Nature Astronomy 2, no. 2 (December 11, 2017): 167–71. http://dx.doi.org/10.1038/s41550-017-0338-3.

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9

Nalewajko, K., and M. Sikora. "Polarization of synchrotron emission from relativistic reconfinement shocks with ordered magnetic fields." Astronomy & Astrophysics 543 (July 2012): A115. http://dx.doi.org/10.1051/0004-6361/201219359.

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10

Desvallées, Lise, Olivier Coutard, and Jonathan Rutherford. "The politics of domestic energy vulnerability in the Barcelona region, between deconfinement and reconfinement." Geoforum 116 (November 2020): 201–10. http://dx.doi.org/10.1016/j.geoforum.2020.08.009.

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11

Matsumoto, Jin, Serguei S. Komissarov, and Konstantinos N. Gourgouliatos. "Magnetic inhibition of the recollimation instability in relativistic jets." Monthly Notices of the Royal Astronomical Society 503, no. 4 (March 22, 2021): 4918–29. http://dx.doi.org/10.1093/mnras/stab828.

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ABSTRACT In this paper, we describe the results of three-dimensional relativistic magnetohydrodynamic simulations aimed at probing the role of regular magnetic field on the development of the instability that accompanies recollimation of relativistic jets. In particular, we studied the recollimation driven by the reconfinement of jets from active galactic nuclei (AGN) by the thermal pressure of galactic coronas. We find that a relatively weak azimuthal magnetic field can completely suppress the recollimation instability in such jets, with the critical magnetization parameter σcr < 0.01. We argue that the recollimation instability is a variant of the centrifugal instability (CFI) and show that our results are consistent with the predictions based on the study of magnetic CFI in rotating fluids. The results are discussed in the context of AGN jets in general and the nature of the Fanaroff–Riley morphological division of extragalactic radio sources in particular.
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12

Komissarov, Serguei S., Konstantinos N. Gourgouliatos, and Jin Matsumoto. "Magnetic inhibition of centrifugal instability." Monthly Notices of the Royal Astronomical Society 488, no. 3 (July 22, 2019): 4061–73. http://dx.doi.org/10.1093/mnras/stz1973.

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ABSTRACT Recently, it was shown that the centrifugal instability may be important in the dynamics of astrophysical jets undergoing reconfinement by external pressure. However, these studies were limited to the case of unmagnetized flows. Here, we explore the role of the magnetic field within both the Newtonian and relativistic frameworks. Since the jet problem is rather complicated, we focus instead on the simpler problem of cylindrical rotation and axial magnetic field, which shares significant similarity with the jet problem, and consider only axisymmetric perturbations. The studied equilibrium configurations involve a cylindrical interface and they are stable to non-magnetic centrifugal and magnetorotational instabilities everywhere except this interface. We use a heuristic approach to derive the local stability criterion for the interface in the magnetic case and numerical simulations to verify the role of the magnetic field. The theory and simulations agree quite well for Newtonian models but indicate a potential discrepancy for the relativistic models in the limit of high Lorentz factor of the rotational motion at the interface. In general, the magnetic field sets a critical wavelength below which the centrifugal modes are stabilized. We discuss the implication of our findings for the astrophysical jets, which suggest that the centrifugal instability develops only in jets with relatively low magnetization. Namely, the magnetic pressure has to be below the thermal one and for the relativistic case the jets have to be kinetic-energy dominated.
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13

Suswinarto, Dwi Yogyo, Sri Andarini, and Retno Lestari. "Phenomenological Study : Family Experience On And Off Deprivation Stocks On The Mental Disorders Family Experience In The Health Center Area Bantur District Malang East Java." Jurnal Ners dan Kebidanan (Journal of Ners and Midwifery) 2, no. 2 (August 1, 2015): 176–87. http://dx.doi.org/10.26699/jnk.v2i2.art.p176-187.

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The Confinenment action to the mental disordes suffer is the action done by the society to limited the suffer’s mobilitas or activities its done based on the hopeless of the family which the medical effort can not made the suffer better than before. The economic burden is not small, additional with stigma from the society and the less optimal of mental health services base on family. Society and medical”s crew.The result of this researchplore the family experience towar the confinement and re confinement of the disorder’s family members in job area of Bantur Community health service of Malang Regency, East Java Province.The research methodology of this thesis use qualitative research (purposive sampling)about 6 sample. The process of data taking used the deep interview with semi structure helping by interview guide and fieldmemorize, its found 7 theme; 1) The cause of mental disorder, 2) The attitude change, 3) The Family’s comment on this situation, 4) The society stigma, 5) Confinement re confinement, 6) The confinement release, 7) The suffer family and society recovery.According the family conclusion the cause of disorder mental are pfisic condition and social pressure , and the moment of confinement –free-reconfinement happened of the society coment toward the situation stigma of the society and unoptimally the medical service. The free of confinement happened because of the family readiness,society and medical service and government involment. The rehabilition of the suffer after free from the confinement need the support from the family, society, community health service and related government.
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14

Neuberger, Herbert. "Deconstructing Ünsal-Yaffe reconfinement." Physics Letters B, April 2022, 137122. http://dx.doi.org/10.1016/j.physletb.2022.137122.

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15

Bonati, Claudio, Marco Cardinali, Massimo D’Elia, Matteo Giordano, and Fabrizio Mazziotti. "Reconfinement, localization, and thermal monopoles in SU(3) trace-deformed Yang-Mills theory." Physical Review D 103, no. 3 (February 15, 2021). http://dx.doi.org/10.1103/physrevd.103.034506.

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