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Journal articles on the topic 'ISM'

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Author: Grafiati

Published: 4 June 2021

Last updated: 11 September 2023

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1

Choi, Woorak, Chang-Goo Kim, and Aeree Chung. "Ram Pressure Stripping of the Multiphase ISM: A Detailed View from TIGRESS Simulations." Astrophysical Journal 936, no. 2 (September 1, 2022): 133. http://dx.doi.org/10.3847/1538-4357/ac82ba.

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Abstract Ram pressure stripping (RPS) is a process that removes the interstellar medium (ISM) quickly, playing a vital role in galaxy evolution. Previous RPS studies have treated the ISM as single-phase or lack the resolution and physical processes to properly capture the full multiphase ISM. To improve this simplification, we introduce an inflowing, hot intracluster medium (ICM) into a self-consistently modeled ISM in a local patch of star-forming galactic disks using the TIGRESS framework. Our simulations reveal that the workings of RPS are not only direct acceleration of the ISM by ICM ram pressure but also mixing-driven momentum transfer involving significant phase transition and radiative cooling. The hot ICM passes through the low-density channels of the porous, multiphase ISM; shreds the cool ISM; and creates mixing layers. The ICM momentum is transferred through the mixing layers while populating the intermediate-temperature gas and radiating thermal energy away. The mixed gas extends beyond galactic disks and forms stripped tails that cool back unless the ICM fluxes are large enough to prevent cooling until they escape the simulation domain. The mixing-driven momentum transfer predicts that the more ICM mixes in, the faster the ISM moves, resulting in the anticorrelation of outflow velocity and gas metallicity of the stripped ISM. The compression of the ISM disks due to the ICM ram pressure enhances star formation rates up to 50% compared to the model without ICM. With the ICM ram pressure higher than the disk anchoring pressure, star formation is quenched within ∼100 Myr.

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2

Rothstein, Eric. ""Organicism," Rupturalism, and Ism-ism." Modern Philology 85, no. 4 (May 1988): 588–609. http://dx.doi.org/10.1086/391665.

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3

Watanabe, Takashi, and Yoshihiro Sugi. "Computer Simulation Tests of Feedback Error Learning Controller with IDM and ISM for Functional Electrical Stimulation in Wrist Joint Control." Journal of Robotics 2010 (2010): 1–11. http://dx.doi.org/10.1155/2010/908132.

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Feedforward controller would be useful for hybrid Functional Electrical Stimulation (FES) system using powered orthotic devices. In this paper, Feedback Error Learning (FEL) controller for FES (FEL-FES controller) was examined using an inverse statics model (ISM) with an inverse dynamics model (IDM) to realize a feedforward FES controller. For FES application, the ISM was tested in learning off line using training data obtained by PID control of very slow movements. Computer simulation tests in controlling wrist joint movements showed that the ISM performed properly in positioning task and that IDM learning was improved by using the ISM showing increase of output power ratio of the feedforward controller. The simple ISM learning method and the FEL-FES controller using the ISM would be useful in controlling the musculoskeletal system that has nonlinear characteristics to electrical stimulation and therefore is expected to be useful in applying to hybrid FES system using powered orthotic device.

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4

Antonuccio-Delogu, V., and J. Silk. "AGN feedback from jet-ISM/IGM interactions." Proceedings of the International Astronomical Union 3, S245 (July 2007): 31–32. http://dx.doi.org/10.1017/s1743921308017201.

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AbstractWe study the propagation of relativistic jets originating from AGNs within the Interstellar/Intergalactic Medium of their host galaxies, and use it to build a model for the inihibition of stellar formation within the expanding cocoon.

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5

Lee, Jaehyun, Taysun Kimm, Jérémy Blaizot, Harley Katz, Wonki Lee, Yun-Kyeong Sheen, Julien Devriendt, and Adrianne Slyz. "Simulating Jellyfish Galaxies: A Case Study for a Gas-rich Dwarf Galaxy." Astrophysical Journal 928, no. 2 (April 1, 2022): 144. http://dx.doi.org/10.3847/1538-4357/ac5595.

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Abstract We investigate the formation of jellyfish galaxies using radiation-hydrodynamic simulations of gas-rich dwarf galaxies with a multiphase interstellar medium (ISM). We find that the ram-pressure-stripped (RPS) ISM is the dominant source of molecular clumps in the near wake within 10 kpc from the galactic plane, while in situ formation is the major channel for dense gas in the distant tail of the gas-rich galaxy. Only 20% of the molecular clumps in the near wake originate from the intracluster medium (ICM); however, the fraction reaches 50% in the clumps located at 80 kpc from the galactic center since the cooling time of the RPS gas tends to be short owing to the ISM–ICM mixing (≲10 Myr). The tail region exhibits a star formation rate of 0.001–0.01 M ⊙ yr−1, and most of the tail stars are born in the stripped wake within 10 kpc from the galactic plane. These stars induce bright Hα blobs in the tail, while Hα tails fainter than 6 × 1038 erg s−1 kpc−2 are mostly formed via collisional radiation and heating due to mixing. We also find that the stripped tails have intermediate X-ray-to-Hα surface brightness ratios (1.5 ≲ F X/F Hα ≲ 20), compared to the ISM (≲1.5) or pure ICM (≫20). Our results suggest that jellyfish features emerge when the ISM from gas-rich galaxies is stripped by strong ram pressure, mixes with the ICM, and enhances the cooling in the tail.

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6

Stout, Jeffrey. "Ism-Mongering." Annual of the Society of Christian Ethics 10 (1990): 55–62. http://dx.doi.org/10.5840/asce1990105.

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7

DeJarnett, Larry R. "ISM Interviews." Journal of Information Systems Management 3, no. 1 (January 1986): 81–84. http://dx.doi.org/10.1080/07399018608965237.

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8

Eagle, John. "ISM Interviews…" Journal of Information Systems Management 4, no. 3 (January 1987): 90–92. http://dx.doi.org/10.1080/07399018708962869.

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9

Donald Rully, A. "ISM INTERVIEWS…" Journal of Information Systems Management 5, no. 1 (January 1988): 86–88. http://dx.doi.org/10.1080/07399018808962903.

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10

Reynolds, Carl H. "ISM INTERVIEWS…" Journal of Information Systems Management 5, no. 2 (January 1988): 92–95. http://dx.doi.org/10.1080/07399018808962919.

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11

Brady, Ivan. "Cannibal-ism." Anthropology and Humanism Quarterly 11, no. 4 (December 1986): 87. http://dx.doi.org/10.1525/ahu.1986.11.4.87.

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12

Brady, Ivan. "Cannibal-ism." Anthropology Humanism Quarterly 11, no. 4 (December 1986): 87. http://dx.doi.org/10.1525/ahu.1986.11.4.87.2.

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13

Strate, Lance. "Journal-ism." Explorations in Media Ecology 17, no. 3 (September 1, 2018): 229–30. http://dx.doi.org/10.1386/eme.17.3.229_2.

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14

Winter, Sarah. "Humanitarian(ism)." Victorian Literature and Culture 46, no. 3-4 (2018): 723–28. http://dx.doi.org/10.1017/s1060150318000669.

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15

Kenney, Jeffrey D. P., Hugh Crowl, Jacqueline van Gorkom, and Bernd Vollmer. "Spiral Galaxy - ICM Interactions in the Virgo Cluster." Symposium - International Astronomical Union 217 (2004): 370–75. http://dx.doi.org/10.1017/s0074180900197979.

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We discuss HI and optical evidence for ongoing ICM-ISM interactions in 6 Hi-deficient Virgo cluster spiral galaxies. One of the clearest cases is the highly inclined Virgo galaxy NGC 4522, which has a normal stellar disk but a truncated gas disk, and lots of extraplanar gas right next to the gas truncation radius in the disk. Unusually strong HI, Hα and radio continuum emission are all detected from the extraplanar gas. The radio continuum polarized flux and spectral index peak on the side opposite the extraplanar gas, suggesting ongoing pressure by the ICM. Four other HI-deficient edge-on Virgo spirals show evidence of extraplanar ISM gas or exhibit asymmetries in their disk HI distributions, but contain much less extraplanar HI than NGC 4522. Comparison with recent simulations suggests this difference may be evolutionary, with large surface densities of extraplanar gas observed only in early phases of an ICM-ISM interaction. In NGC 4569, the Hα image shows 2 effects of ICM pressure on the galaxy ISM. An anomalous arm of HII regions, possibly extraplanar, emerges from the edge of a truncated Hα disk. This resembles the arms seen in simulations which are formed by the combined effects of wind pressure plus rotation. An extended nebulosity near the minor axis, also in the NW, is interpreted as a starburst outflow bubble disturbed by ICM wind pressure.

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16

McClure-Griffiths, N. M. "New results from Galactic ISM surveys: The frothy ISM." Astronomische Nachrichten 333, no. 5-6 (June 2012): 497–504. http://dx.doi.org/10.1002/asna.201211694.

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17

Burton, Adrian. "All‐true‐ism." Frontiers in Ecology and the Environment 19, no. 9 (November 2021): 540. http://dx.doi.org/10.1002/fee.2427.

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18

LaGasse, Robert C. "The ISM Industry:." Journal of Microwave Power and Electromagnetic Energy 34, no. 2 (January 1999): 65–126. http://dx.doi.org/10.1080/08327823.1999.11688389.

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19

Hayes, Edgar H. "ISM Interviews [tdot]." Journal of Information Systems Management 3, no. 2 (January 1986): 73–76. http://dx.doi.org/10.1080/07399018608965251.

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20

Williams, Carl C. "ISM Interviews[tdot]." Journal of Information Systems Management 3, no. 3 (January 1986): 81–84. http://dx.doi.org/10.1080/07399018608965266.

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21

Victor Janulaitis, M. "ISM Interviews[tdot]." Journal of Information Systems Management 3, no. 4 (January 1986): 88–92. http://dx.doi.org/10.1080/07399018608965281.

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22

Morino, Mario M. "ISM INTERVIEWS[tdot]." Journal of Information Systems Management 4, no. 4 (January 1987): 76–78. http://dx.doi.org/10.1080/07399018708962885.

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23

Bohannan, Paul, and Edward T. Hall. "An “ism” Problem." Anthropology News 31, no. 5 (May 1990): 3. http://dx.doi.org/10.1111/an.1990.31.5.3.1.

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24

LERNER, RABBI MICHAEL. "Overcoming Trump-ism." Tikkun 32, no. 1 (2017): 4–8. http://dx.doi.org/10.1215/08879982-3769001.

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25

Onuf, Nicholas. "Making Terror/ism." International Relations 23, no. 1 (March 2009): 53–60. http://dx.doi.org/10.1177/0047117808100609.

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26

Onaka, Takashi. "ISM Diagnostics: Dust." Proceedings of the International Astronomical Union 8, S292 (August 2012): 259–66. http://dx.doi.org/10.1017/s1743921313001324.

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AbstractInfrared (IR) observations provide significant information on the lifecycle of dust grains in the interstellar medium (ISM), which is crucial for the understanding of the evolution of matter in the universe. The IR spectral energy distribution (SED) of the dust emission tells us the relative abundance of sub-micron grains, very small grains, and carriers of the unidentified infrared (UIR) emission bands, since they emit the far-IR, the mid-IR, and the UIR bands from the near- to mid-IR, respectively. On the other hand, the UIR emission bands themselves offer a useful means to probe the physical conditions from which the band emission arises because each band is assigned to a specific C-H or C-C vibration mode and because its relative intensity should reflect the properties of the band carriers and the physical conditions of the environment. Here the two diagnostic methods using IR observations are briefly described together with examples of the observational results. Implications for the dust lifecycle are also discussed.

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27

Harding, Mike. "Trans-what-ism?" New Scientist 196, no. 2628 (November 2007): 26. http://dx.doi.org/10.1016/s0262-4079(07)62776-6.

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28

Introna, Lucas D., and Edgar A. Whitley. "Against method‐ism." Information Technology & People 10, no. 1 (March 1997): 31–45. http://dx.doi.org/10.1108/09593849710166147.

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29

Madsen, Vibeke Thøis. "The challenges of introducing internal social media – the coordinators’ roles and perceptions." Journal of Communication Management 21, no. 1 (February 6, 2017): 2–16. http://dx.doi.org/10.1108/jcom-04-2016-0027.

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Purpose The purpose of this paper is to explore the challenges associated with introducing internal social media (ISM) into organizations in order to help them reap the benefits of coworker communication on ISM. Design/methodology/approach The paper is based on an exploratory study in ten organizations. The data were collected in semi-structured interviews with ISM coordinators in Spring 2014. Findings According to the ISM coordinators, four challenges were associated with introducing ISM: coworkers could perceive communication on ISM as not work related; coworkers might not understand the informal nature of communication on ISM, and self-censorship might stop them communicating on ISM; ISM was not considered a “natural” part of the daily routines in the organizations; and top managers mainly supported ISM in words, not in action. Research limitations/implications The study is based on the perceptions of ISM coordinators. Further research is called for to explore both coworker perceptions and actual communication on ISM. Practical implications Practitioners introducing ISM should be aware of these four challenges, and should help coworkers to make sense of communication on ISM as work-related communication among coworkers. ISM coordinators’ perceptions of their own role in relation to coworker communication on ISM make a difference. Originality/value The study provides insights into the key challenges associated with introducing ISM, as well as the role of ISM coordinators as community facilitators and sense-givers.

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30

Putra, Adi Pratama, and Adi Mulyadi. "Design an Automatic Transfer Switch for Solar Power Plant." Logic : Jurnal Rancang Bangun dan Teknologi 22, no. 1 (March 30, 2022): 9–12. http://dx.doi.org/10.31940/logic.v22i1.9-12.

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This paper discusses the automatic transfer switch (ATS) in solar power plants. ATS is used to transfer the main electrical power to a backup power source (battery). PLN power cannot supply electricity continuously due to non-standard ATS installations, blackouts, disturbances to the generating system, and distribution system. Two ATS systems are proposed to control the switching process of PLN and PLTS automatically using inverter standby mode (ISM) and inverter off mode (IOM). The results of the application of ISM to PLN and PLTS can supply power needs based on switching techniques to avoid equipment damage. While IOM can save battery for inverter power supply.

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31

Falceta-Gonçalves, D., G. Kowal, and A. Lazarian. "Properties of MHD turbulence and its consequences for the ISM and ICM." Proceedings of the International Astronomical Union 5, H15 (November 2009): 464–65. http://dx.doi.org/10.1017/s174392131001029x.

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AbstractIt is well known that the interstellar (ISM) and intergalactic (ICM) media are threaded by large scale magnetic fields. The understanding of its role on the dynamics of the media is, however, still in progress. For the ISM, magnetic fields may control or, at least, play a major role on the turbulence cascade leading to the star formation process. The ICM, on the other hand, is assumed to be thermally dominated but still the magnetic field may play an important role on the processes of acceleration and propagation of cosmic rays. In this work we provide a review of the latest theoretical results on the evolution of MHD turbulence under collisional and collisionless plasma approaches.

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32

Franchetto, Andrea, Stephanie Tonnesen, Bianca M. Poggianti, Benedetta Vulcani, Marco Gullieuszik, Alessia Moretti, Rory Smith, et al. "Evidence for Mixing between ICM and Stripped ISM by the Analysis of the Gas Metallicity in the Tails of Jellyfish Galaxies." Astrophysical Journal Letters 922, no. 1 (November 1, 2021): L6. http://dx.doi.org/10.3847/2041-8213/ac3664.

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Abstract Hydrodynamical simulations show that the ram pressure stripping in galaxy clusters fosters a strong interaction between stripped interstellar medium (ISM) and the surrounding medium, with the possibility of intracluster medium (ICM) cooling into cold gas clouds. Exploiting the MUSE observation of three jellyfish galaxies from the GAs Stripping Phenomena in galaxies with MUSE (GASP) survey, we explore the gas metallicity of star-forming clumps in their gas tails. We find that the oxygen abundance of the stripped gas decreases as a function of the distance from the parent galaxy disk; the observed metallicity profiles indicate that more than 40% of the most metal-poor stripped clouds are constituted by cooled ICM, in qualitative agreement with simulations that predict mixing between the metal-rich ISM and the metal-poor ICM.

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33

Zhang, Qing-zhong, Xian-yun Hu, Wen-qin Yao, Xiao-li Wan, Zi-cong Liang, Rong-min Dang, Zheng-min Yang, and Ya-lan Xia. "Pharmacologic Effect of Miao Medicine Illicium simonsii Maxim. on Collagen-Induced Arthritis in Rats." Evidence-Based Complementary and Alternative Medicine 2018 (October 11, 2018): 1–7. http://dx.doi.org/10.1155/2018/2398379.

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Objectives. To study the pharmacologic effect and mechanism of action of Miao medicine Illicium simonsii Maxim. (ISM) in treating rheumatoid arthritis. Methods. Sixty rats were randomly divided to six groups: normal control (normal), collagen-induced arthritis (CIA) model (model), CIA + tripterygium glycosides (TG), CIA + ISM high dose oral (ISM-H), CIA + ISM low-dose oral (ISM-L), and CIA + ISM topical application (ISM-T). The treatment doses were selected based on published reports and folk medicine practice. The outcome measurements included paw swelling, joint pathology, organ index, blood count, T helper 17 (Th17) cell count, and interleukin-6 (IL-6) level. Results. Compared to the CIA model group, all treatment groups showed a significant reduction in paw swelling, blood vessel pathology, Th17 cell count, and IL-6 levels (p < 0.05 or p < 0.01). All treatment groups showed alleviated foot swelling and lower total number of white blood cells, and these effects were observed earlier with oral ISM than topical ISM. The effect of ISM was weaker than that of TG. In addition, less organ damage was observed with topical ISM than oral ISM but better than TG. Conclusions. These results suggest that, by downregulating Th17 cells, ISM inhibits the production of Il-6, thereby alleviating the proliferation of endothelial and rheumatoid-like cells and leukocytosis in CIA rats, ultimately eliminating foot swelling.

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34

Triani, Dian P., Manodeep Sinha, Darren J. Croton, Eli Dwek, and Camilla Pacifici. "Exploring the relation between dust mass and galaxy properties using Dusty SAGE." Monthly Notices of the Royal Astronomical Society 503, no. 1 (March 5, 2021): 1005–16. http://dx.doi.org/10.1093/mnras/stab558.

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ABSTRACT We explore the relation between dust and several fundamental properties of simulated galaxies using the Dusty SAGE semi-analytic model. In addition to tracing the standard galaxy properties, Dusty SAGE also tracks cold dust mass in the interstellar medium (ISM), hot dust mass in the halo, and dust mass ejected by feedback activity. Based on their ISM dust content, we divide our galaxies into two categories: ISM dust-poor and ISM dust-rich. We split the ISM dust-poor group into two subgroups: halo dust-rich and dust-poor (the latter contains galaxies that lack dust in both the ISM and halo). Halo dust-rich galaxies have high outflow rates of heated gas and dust and are more massive. We divide ISM dust-rich galaxies based on their specific star formation rate (sSFR) into star-forming and quenched subgroups. At redshift z = 0, we find that ISM dust-rich galaxies have a relatively high sSFR, low bulge-to-total (BTT) mass ratio, and high gas metallicity. The high sSFR of ISM dust-rich galaxies allows them to produce dust in the stellar ejecta. Their metal-rich ISM enables dust growth via grain accretion. The opposite is seen in the ISM dust-poor group. Furthermore, ISM dust-rich galaxies are typically late-types, while ISM dust-poor galaxies resemble the early-type population, and we show how their ISM content evolves from being dust-rich to dust-poor. Finally, we investigate dust production from z = 3 to z = 0 and find that all groups evolve similarly, except for the quenched ISM dust-rich group.

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35

Birkenbihl, Rainer P., and Walter Vielmetter. "Complete maps of IS1, IS2, IS3, IS4, IS5, IS30 and IS150 locations in Escherichia coli K12." Molecular and General Genetics MGG 220, no. 1 (December 1989): 147–53. http://dx.doi.org/10.1007/bf00260869.

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36

Ge, Chong, Rongxin Luo, Ming Sun, Masafumi Yagi, Pavel Jáchym, Alessandro Boselli, Matteo Fossati, et al. "An H α/X-ray orphan cloud as a signpost of intracluster medium clumping." Monthly Notices of the Royal Astronomical Society 505, no. 4 (June 1, 2021): 4702–16. http://dx.doi.org/10.1093/mnras/stab1569.

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ABSTRACT Recent studies have highlighted the potential significance of intracluster medium (ICM) clumping and its important implications for cluster cosmology and baryon physics. Many of the ICM clumps can originate from infalling galaxies, as stripped interstellar medium (ISM) mixing into the hot ICM. However, a direct connection between ICM clumping and stripped ISM has not been unambiguously established before. Here, we present the discovery of the first and still the only known isolated cloud (or orphan cloud [OC]) detected in both X-rays and H α in the nearby cluster A1367. With an effective radius of 30 kpc, this cloud has an average X-ray temperature of 1.6 keV, a bolometric X-ray luminosity of ∼3.1 × 1041 erg s−1, and a hot gas mass of ∼1010 M⊙. From the Multi-Unit Spectroscopic Explorer (MUSE) data, the OC shows an interesting velocity gradient nearly along the east-west direction with a low level of velocity dispersion of ∼80 km s−1, which may suggest a low level of the ICM turbulence. The emission line diagnostics suggest little star formation in the main H α cloud and a low-ionization (nuclear) emission-line regions like spectrum, but the excitation mechanisms remain unclear. This example shows that stripped ISM, even long after the initial removal from the galaxy, can still induce ICM inhomogeneities. We suggest that the magnetic field can stabilize the OC by suppressing hydrodynamic instabilities and thermal conduction. This example also suggests that at least some ICM clumps are multiphase in nature and implies that the ICM clumps can also be traced in H α. Thus, future deep and wide-field H α surveys can be used to probe the ICM clumping and turbulence.

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37

Hanik, Ummi, and Muhammad Afif Amrulloh. "Analisis Sintaksis Kāna wa-Akhawātuhā dalam Kitab al-‘Arabīyah li-al-Nāshi’īn." Al-Ma‘rifah 16, no. 2 (October 30, 2019): 122–31. http://dx.doi.org/10.21009/almakrifah.16.02.02.

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This study aims to find out the forms of ism kāna and khabar kāna wa-akhwātuhā. This research is qualitative with a type of library research. Data collection techniques are using the documentation method, while data analysis techniques are using content analysis. The results of this study prove that in al-‘Arabīyah li-al-Nāshi’īn book, volume 4, there are 161 types of ism kāna, while khabar kāna totaling 84 are analyzed based on (1) The i‘rāb aspect and its form there are 38 ism kāna in the form of ism mabnī consisting of 28 ḍamīr mustatir jawāzān, 7 ḍamīr bāriz which are composed of ḍamīr muṭṭaṣil and 3 ism al-ishārah. Likewise, 46 ism kāna in the form of ism mu‘rab; 41 ism mufrad, 3 jam‘ al-taksīr, 1 ism tahnīyah and 1 asmā’ al-khamsah. As for the aspects of its type, there are 77 ism kāna in the form of mudhakkar and mu’annath, 63 consisting of mudhakkar and 14 consisting of mu’annath. (2) 84 khabar kāna consists of 38 khabar mufrad in the form of ism jāmid and ism mushtaq, 33 khabar in the form of fi‘l mudhari‘ and 13 khabar shibh al-jumlah in the form of jār majrūr. This study contributes to the development of studyng Arabic grammar which can be applied in the use of Arabic as in the book.

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38

He, Yue, Juzhi Hou, Erik T. Brown, Shuyun Xie, and Zhengyu Bao. "Timing of the Indian Summer Monsoon onset during the early Holocene: Evidence from a sediment core at Linggo Co, central Tibetan Plateau." Holocene 28, no. 5 (December 11, 2017): 755–66. http://dx.doi.org/10.1177/0959683617744267.

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The spatial and temporal variability, effects, and mechanisms of the Indian Summer Monsoon (ISM) have been investigated intensively during the past few decades. The pattern of a relatively strong ISM during the early to middle Holocene, and a relatively weak ISM in the late Holocene, has been widely demonstrated in both marine and continental records. However, the timing of the ISM onset during the early Holocene remains controversial. Here, we present oxygen isotope record from ostracods and hydrogen isotope record from sedimentary leaf waxes from a sediment core at Linggo Co, a glacier-fed lake on the central Tibetan Plateau, in order to investigate the onset of the ISM. The ostracod δ18O record indicates an early ISM onset at ~11.7 ka, whereas the leaf wax δD record indicates a later ISM onset at ~10 ka. This apparent two-step development of the ISM revealed by aquatic and terrestrial records is confirmed by principal component analysis of nine marine records from the ISM domain. The comparison between isotope records from Linggo Co and the marine records implies that the early ISM onset was likely linked to elevated temperatures in the Northern Hemisphere, while the later ISM onset may be related to intensified precipitation.

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39

Kholifaturrohmah, Kholifaturrohmah, Hasan Busri, and Darul Qutni. "MAṢDAR ṢINĀIY DALAM KITAB AL BARZANJI KARYA SYAIKH JA’FAR AL BARZANJI (ANALISIS MORFOSINTAKSIS)." Lisanul Arab: Journal of Arabic Learning and Teaching 11, no. 2 (December 21, 2022): 15–21. http://dx.doi.org/10.15294/la.v11i2.60992.

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Maṣdar ṣināiy is an ism that includes ya' nisbat along with ta' taknits to show the nature in it. Sometimes it is formed from ism fail, ism maf'ūl, ism tafḍil, ism jāmid, ism alam, and ism maṣdar. The purpose of this study was to determine the origin of the type of maṣdar ṣināiy in the book of Al Barzanji. This research is a qualitative research with library research design. The data is in the form of maṣdar ṣināiy in the book of Al Barzanji. Data collection techniques using documentation techniques. In this study, it was found as many as 33 maṣdar ṣināiy data in the Al Barzanji book, based on the origin of the maṣdar ṣināiy type, there were 7 data from ism fāil, 2 data from ism maf'ūl, 3 data from ism alam, 19 data from ism jāmid , and 2 data came from ism maṣdar. Based on cases and grammatical markers, the researchers found 5 nominative case data with dhummah grammatical markers (vocal u), 1 accusative case data with fathah grammatical markers (vocal a), and 27 genetic case data with kasroh grammatical markers (vocal i). Based on the syntatic function, the researcher found 2 data had a syntatic function as fā’il, 4 data had a syntatic function as khobar, 5 data had a syntatic function as majrur, 11 data had a syntatic function as muḍaf ilaih, 8 data had a syntatic function as tābi’, 1 data had a syntatic function as mustatsna, 1 data had a syntatic function as maḍruf, and 1 data had a syntatic function as inna’s ism.

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Millett, Kris, and Fahad Ahmad. "Echoes of Terror(ism)." Canadian Social Studies 52, no. 2 (July 12, 2021): 52–67. http://dx.doi.org/10.29173/css25.

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Our paper examines the latest frontier of the “War on Terror,” countering violent extremism (CVE), non-coercive approaches that aim to prevent “radicalization” that may lead to “violent extremism” or terrorism. We look at the recent implementation of CVE in Québec’s education sector. Based on an analysis of key policy documents and interviews with CVE practitioners, we find that: (1) teachers are responsibilized to safeguard society from the risk of terrorism through being expected to “know the signs” of radicalization and to build “resilience,” (2) students are responsibilized as agents who can influence their peers against violent extremist messaging and toward “prosocial” behaviour, and (3) elements of school curriculum are responsibilized, especially social studies education, to provide students with “critical thinking” skills thought to be lacking among those at risk of radicalization. We highlight the inherent contradictions in CVE, which, in Québec, claims to foster pluralism and inclusivity to combat Islamophobia, but as a modality of the “War on Terror” also targets and stigmatizes Muslim communities. Critical discussion of CVE’s social implications are needed to initiate critical dialogue in Canada over the impact of CVE in social services provision and the risk of securitizing the education sector in Québec.

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Sakwa, Richard. "Is Putin an Ism?" Russian Politics 5, no. 3 (August 25, 2020): 255–82. http://dx.doi.org/10.30965/24518921-00503001.

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Abstract The Putin phenomenon represents a complex and dynamic interaction between the character of the man, his policies and leadership style. After over two decades in office, we can ask whether there is such a thing as ‘Putinism’, and if so, what are its main features? What are the criteria to be considered an ‘ism’? At the minimum, it requires some sort of ‘grand strategy’ that underpins policy in domestic and foreign policy, and which unites the two. A grand strategy is defined as some deep structure in domestic and foreign policy that transcends individual leaders and which has some overarching purpose. Putinism in this paper is considered a ‘passive revolution’, allowing a profound transformation to take place in society while the polity remains relatively static. One of the main criticisms levelled against Putin is that he is brilliant at tactics, above all in factional maneuvering, but lacks an over-arching vision of where Russia should go. This paper assesses whether Putin is ultimately an ephemeral phenomenon, or whether the era with which his name is associated will endure in history as a distinctive style of rule.

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Miller, Toby. "Actually Existing Journal-Ism." Social Text, no. 50 (1997): 147. http://dx.doi.org/10.2307/466825.

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Prentice, Thom. "Another "Ism" to Debate." English Journal 89, no. 3 (January 2000): 13. http://dx.doi.org/10.2307/822085.

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Waltner, Robb. "ARCHITECTURE AND URBANE-ISM." Journal of Access Services 3, no. 3 (February 27, 2006): 85–89. http://dx.doi.org/10.1300/j204v03n03_09.

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Becker, Genevieve. "Independent Study Module (ISM)." Journal of Human Lactation 14, no. 4 (December 1998): 287. http://dx.doi.org/10.1177/089033449801400403.

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Šalgovičová, Jarmila, and Vanessa Prajová. "Information Security Management (ISM)." Research Papers Faculty of Materials Science and Technology Slovak University of Technology 20, Special-Number (December 1, 2012): 114–19. http://dx.doi.org/10.2478/v10186-012-0019-0.

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Abstract Currently, all organizations have to tackle the issue of information security. The paper deals with various aspects of Information Security Management (ISM), including procedures, processes, organizational structures, policies and control processes. Introduction of Information Security Management should be a strategic decision. The concept and implementation of Information Security Management in an organization are determined by the corporate needs and objectives, security requirements, the processes deployed as well as the size and structure of the organization. The implementation of ISM should be carried out to the extent consistent with the needs of the organization.

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Gupta, Yashwant. "Pulsars and the ISM." Symposium - International Astronomical Union 199 (2002): 363–68. http://dx.doi.org/10.1017/s0074180900169335.

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Radio signals from pulsars are significantly affected by propagation effects such as dispersion, faraday rotation and scintillations in the interstellar medium (ISM). In this paper, I review some aspects of our understanding about pulsars and interstellar scintillations (ISS). The study of pulsar scintillation has dual benefits in that it allows us to learn about the properties of the ISM using pulsars as probes, as well as to infer some properties about pulsars, using the ISM as a tool. Both these aspects are addressed in this paper. The main emphasis is on recent developments in the following topics : (i) the shape of the spectrum of electron density fluctuations in the interstellar medium (ii) the distribution of scattering plasma in the local ISM and (iii) resolving pulsar emission regions using ISS.

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Väisälä, M. S., F. A. Gent, M. Juvela, and M. J. Käpylä. "The supernova-regulated ISM." Astronomy & Astrophysics 614 (June 2018): A101. http://dx.doi.org/10.1051/0004-6361/201730825.

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Context.Efforts to compare polarization measurements with synthetic observations from magnetohydrodynamics (MHD) models have previously concentrated on the scale of molecular clouds.Aims.We extend the model comparisons to kiloparsec scales, taking into account hot shocked gas generated by supernovae and a non-uniform dynamo-generated magnetic field at both large and small scales down to 4 pc spatial resolution.Methods.We used radiative transfer calculations to model dust emission and polarization on top of MHD simulations. We computed synthetic maps of column densityNH, polarization fractionp, and polarization angle dispersionS, and studied their dependencies on important properties of MHD simulations. These include the large-scale magnetic field and its orientation, the small-scale magnetic field, and supernova-driven shocks.Results.Similar filament-like structures ofSas seen in thePlanckall-sky maps are visible in our synthetic results, although the smallest scale structures are absent from our maps. Supernova-driven shock fronts andSdo not show significant correlation. Instead,Scan clearly be attributed to the distribution of the small-scale magnetic field. We also find that the large-scale magnetic field influences the polarization properties, such that, for a given strength of magnetic fluctuation, a strong plane of the sky mean field weakens the observedS, while strengtheningp. The anticorrelation ofpandS, and decreasingpas a function ofNHare consistent across all synthetic observations. The magnetic fluctuations follow an exponential distribution, rather than Gaussian characteristic of flows with intermittent repetitive shocks.Conclusions.The observed polarization properties and column densities are sensitive to the line-of-sight distance over which the emission is integrated. Studying synthetic maps as the function of maximum integration length will further help with the interpretation of observations. The effects of the large-scale magnetic field orientation on the polarization properties are difficult to be quantified from observations solely, but MHD models might turn out to be useful for separating the effect of the large-scale mean field.

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Käpylä, M. J., F. A. Gent, M. S. Väisälä, and G. R. Sarson. "The supernova-regulated ISM." Astronomy & Astrophysics 611 (March 2018): A15. http://dx.doi.org/10.1051/0004-6361/201731228.

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Context.The forcing of interstellar turbulence, driven mainly by supernova (SN) explosions, is irrotational in nature, but the development of significant amounts of vorticity and helicity, accompanied by large-scale dynamo action, has been reported.Aim.Several earlier investigations examined vorticity production in simpler systems; here all the relevant processes can be considered simultaneously. We also investigate the mechanisms for the generation of net helicity and large-scale flow in the system.Methods.We use a three-dimensional, stratified, rotating and shearing local simulation domain of the size 1 × 1 × 2 kpc3, forced with SN explosions occurring at a rate typical of the solar neighbourhood in the Milky Way. In addition to the nominal simulation run with realistic Milky Way parameters, we vary the rotation and shear rates, but keep the absolute value of their ratio fixed. Reversing the sign of shear vs. rotation allows us to separate the rotation- and shear-generated contributions.Results.As in earlier studies, we find the generation of significant amounts of vorticity, the rotational flow comprising on average 65% of the total flow. The vorticity production can be related to the baroclinicity of the flow, especially in the regions of hot, dilute clustered supernova bubbles. In these regions, the vortex stretching acts as a sink of vorticity. In denser, compressed regions, the vortex stretching amplifies vorticity, but remains sub-dominant to baroclinicity. The net helicities produced by rotation and shear are of opposite signs for physically motivated rotation laws, with the solar neighbourhood parameters resulting in the near cancellation of the total net helicity. We also find the excitation of oscillatory mean flows, the strength and oscillation period of which depend on the Coriolis and shear parameters; we interpret these as signatures of the anisotropic-kinetic-α(AKA) effect. We use the method of moments to fit for the turbulent transport coefficients, and findαAKAvalues of the order 3–5 km s−1.Conclusions.Even in a weakly rotationally and shear-influenced system, small-scale anisotropies can lead to significant effects at large scales. Here we report on two consequences of such effects, namely on the generation of net helicity and on the emergence of large-scale flows by the AKA effect, the latter detected for the first time in a direct numerical simulation of a realistic astrophysical system.

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DeMaria, Anthony. "A Third “Ism”: Ageism." Structural Heart 7, no. 1 (January 2023): 100132. http://dx.doi.org/10.1016/j.shj.2022.100132.

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