Relevant bibliographies by topics / ISM

Academic literature on the topic 'ISM'

Author: Grafiati
Published: 4 June 2021
Last updated: 11 September 2023

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Journal articles on the topic "ISM"

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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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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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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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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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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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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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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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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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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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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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Dissertations / Theses on the topic "ISM"

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Fierlinger, Katharina M. "Massive stars shaping the ISM." Diss., Ludwig-Maximilians-Universität München, 2014. http://nbn-resolving.de/urn:nbn:de:bvb:19-176288.

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Diese Arbeit befasst sich mit dem Einfluss von Sternen, deren Masse acht Sonnenmassen übersteigt, auf das Interstellare Medium in ihrer Umgebung. Solche massereiche Sterne beenden ihr Dasein mit einer Supernovaexplosion und verlieren im Laufe ihrer - verglichen mit massearmen Sternen - raschen Entwicklung einen großen Teil ihrer Masse über ihre starken Sternwinde. Beispielsweise gibt ein Stern mit 60 Sonnenmassen Anfangsmasse mehr als die doppelte Supernovaenergie über die kinetische Energie seiner Winde in seine Umgebung ab. Sterne entstehen in Regionen mit kaltem, dichtem Gas, den sogenannten Molekülwolken. Beobachtungen zeigen, dass diese Gaswolken turbulent sind. Es ist allerdings noch ungeklärt, woher die beobachtete Turbulenz im Interstellaren Medium ihre Energie bezieht. Die Energieabgabe von massereichen Sternen ist - neben großskaligen gravitativen Instabilitäten in der Scheibe der Milchstraße - eine der möglichen Erklärungen. Beobachtungen erlauben Rückschlüsse auf die eingebrachte Energiemenge und die Längenskalen des Energie liefernden Prozesses. Daher ist es relevant, zu bestimmen, wie viel kinetische Energie ein massereicher Stern in der ihn umgebenden Molekülwolke deponieren kann. Der Schwerpunkt dieser Arbeit sind hydrodynamische Simulationen, die diese Energieeffizienz testen. Dazu wurden aktuelle Sternentwicklungsmodelle in die frei zugänglichen Eulerschen Gittercodes Pluto und Ramses eingebaut. Die Simulationen verwenden das von Eva Ntormousi erstellte Modul für die Berechnung der Heiz- und Kühlprozesse eines Multiphasenmediums. Die Modellrechnungen führten zur Erkenntnis, dass in jener Phase der Simulation, in der die räumliche Auflösung der Modellrechnung die Eneergieeffizienz stark beeinflusst, der größte Energieverlust durch Strahlung an jener Stelle auftritt, an der das vom Stern ausgestoßene Material auf das aufgesammelte Umgebungsgas trifft. An dieser Kontaktfläche treten Mischungsprozesse auf, welche die Energieverluste steigern. Somit können unsere Simulationen in Kombination mit einer Abschätzung der Effizienz und Skalenlänge dieser Mischprozesse eine Aussage treffen, wie viel Energie massereiche Sterne zur Aufrechterhaltung der Turbulenz beitragen können. Für diese Abschätzung der Mischprozesse liefert die Literatur auf Beobachtungen und numerischen Simulationen basierende Richtwerte. Als Anwendungsbeispiel wird in dieser Arbeit die Orion-Eridanus Region diskutiert. In dieser Region wird das radioaktive Isotop 26-Al beobachtet. Dieses Isotop wird vorrangig in massereichen Sternen gebildet. Es kann daher als Indikator für von Sternen ausgestoßene Materie verwendet werden. Interessanterweise zeigen die Beobachtungen dieser Region nur in einem Teil des Gebiets mit Röntgenemission ein 26-Al Signal. Unsere Ramses Modelle berücksichtigen 26-Al und können daher auf Gebiete mit (fehlenden) Korrelationen zwischen Röntgenemission und 26-Al Signal durchsucht werden.
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Harju, J., F. Daniel, O. Sipilae, P. Caselli, J. E. Pineda, R. K. Friesen, A. Punanova, et al. "Deuteration of ammonia in the starless core Ophiuchus/H-MM1." EDP SCIENCES S A, 2017. http://hdl.handle.net/10150/624367.

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Context. Ammonia and its deuterated isotopologues probe physical conditions in dense molecular cloud cores. The time-dependence of deuterium fractionation and the relative abundances of different nuclear spin modifications are supposed to provide a means of determining the evolutionary stages of these objects. Aims. We aim to test the current understanding of spin-state chemistry of deuterated species by determining the abundances and spin ratios of NH2D, NHD2 and ND3 in a quiescent, dense cloud. Methods. Spectral lines of NH3, NH2D, NHD2, ND3 and N2D+ were observed towards a dense, starless core in Ophiuchus with the APEX, GBT and IRAM 30-m telescopes. The observations were interpreted using a gas-grain chemistry model combined with radiative transfer calculations. The chemistry model distinguishes between the different nuclear spin states of light hydrogen molecules, ammonia and their deuterated forms. Different desorption schemes can be considered. Results. High deuterium fractionation ratios with NH2D = NH3 similar to 0 : 4, NHD2 = NH2D similar to 0 : 2 and ND3 = NHD2 similar to 0 : 06 are found in the core. The observed ortho/para ratios of NH2D and NHD2 are close to the corresponding nuclear spin statistical weights. The chemistry model can approximately reproduce the observed abundances, but consistently predicts too low ortho/para-NH2D, and too large ortho/para-NHD2 ratios. The longevity of N2H+ and NH3 in dense gas, which is prerequisite to their strong deuteration, can be attributed to the chemical inertia of N-2 on grain surfaces. Conclusions. The discrepancies between the chemistry model and the observations are likely to be caused by the fact that the model assumes complete scrambling in principal gas-phase deuteration reactions of ammonia, which means that all the nuclei are mixed in reactive collisions. If, instead, these reactions occur through proton hop/hydrogen abstraction processes, statistical spin ratios are to be expected. The present results suggest that while the deuteration of ammonia changes with physical conditions and time, the nuclear spin ratios of ammonia isotopologues do not probe the evolutionary stage of a cloud.
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Kissmann, Ralf. "Numerical investigation of the turbulent ISM." [S.l.] : [s.n.], 2007. http://deposit.ddb.de/cgi-bin/dokserv?idn=98361265X.

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Noack, Vanessa. "Heroic Soldier-ism: Beautified Power Asymmetry." Thesis, Linköpings universitet, Institutionen för tema, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-166690.

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The Swedish Armed Forces can be considered a hegemonic masculine organisation with deeply embedded patterns of patriarchy, as well as fratriarchy represented by notions of homogeneity and the male soldier. Women are highly underrepresented and face multiple double standards related to their performance of gender and more precisely performance of femininity. However, the Swedish Armed Forces claim to be an inclusive organisation and advertise this through different recruiting strategies, which display women in uniforms. This thesis uses the methodology of qualitative research by combining the methods of critical discourse analysis and critical visual analysis to analyse the representation and the performativity of gender in a recruiting advertisement for inclusivity by the Swedish Armed Forces. I argue that this advertisement led to a certain form of reproducing stereotypical notions of femininity by representing women who embody certain requirements connected to beauty standards. At the same time, notions of hegemonic masculinity and patriarchy are challenged through the representation of women in military uniforms.
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Gan, Kok Chek. "A Java implementation of Peer ISM /." Leeds, 2001. http://www.leeds.ac.uk/library/counter2/compstmsc/20002001/gan%5Fpdf.zip.

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Menacho, Veronica. "The violent ISM in Haro 11." Licentiate thesis, Stockholms universitet, Institutionen för astronomi, 2018. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-163310.

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This thesis introduces briefly physical processes operating in the ISM around massive starsand focuses on the impact strong stellar feedback has in creating large-scale structures in a galaxy.Stellar feedback is ubiquitous in star forming galaxies and its effect on the ISM depends strongly on the energy output from the most massive stars (M$\geq$7 \Mo ) and the properties of the surrounding gas. Starburst galaxies are among the most active in producing %galaxies are among the most active galaxies and produce a large amount of massive star clusters %or even super star clusters (SSC; M$_{cl} \geq 10^5$ \Mo ), with stellar populations up to thousands of massive stars. %The most massive stars (M$\geq$30 \Mo ) are lives short, but they In the first 4 Myr of the star clusters evolution, radiative feedback of the most massive stars (M$\geq$30 \Mo ) are at work. Large amount of ionizing photons are released to the ambient medium while radiative pressure compress the surrounding gas. At the same time their stellar winds inject continuously mechanical energy and momentum in their surrounding. This mechanical feedback is then at later ages, until $\sim$ 40 Myrs, maintained by supernova explosions from the less massive stars. Strong stellar feedback tends to develop large-scale structures such as bubbles, loops, filaments and outflows. These are transient structures and can be seen as imprints of how the released energy is clearing or has cleared paths in the ISM. Strong stellar feedback can have devastating consequences in dwarf galaxies due to their shallow gravitational potential. It can accelerate outflows with velocities larger than their escape velocities. In this way, dwarf galaxies can lose a large fraction of their gas mass, which will be crucial in their subsequent evolution.On the other hand, galactic winds might be responsible to create holes in the ISM, allowing the easily-absorbed ionizing photons (Lyman continuum photons, LyC) to escape the galaxy. Studies on a few LyC leaking galaxies have shown that this mechanisms might have preference from a density-bound scenario, which takes place in galaxies with a highly ionized halo. In my paper I used deep MUSE observations to analyse the impact strong stellar feedback has in the starburst and Lyman continuum emitting galaxy: Haro 11. The paper presents three emission line diagnostics aiming to analyse the condition of the warm ionized gas in this galaxy, which are the \Ha\ emission, the level of ionization in gas and the presence of fast shocks. These diagnostics are presented in maps of 50 \kms\ bins in a velocity range from -400 to 350 \kms . Haro 11 shows a violent ISM whose warm ionized gas is almost completely shaped by effect of stellar feedback from the most massive star forming regions in the centre. Arcs, shells, outflows paths and galactic scale ionizing cones are imprinted in ISM of Haro 11. Our analysis suggests the presence of a kpc-scale superbubble which might have created galactic holes in the ISM. Beside of that, Haro 11 shows a highly ionized halo. Both mechanisms appear to facilitate the escape of LyC in this galaxy. %Finally, we observe emission at velocities up to thousand \kms\ which could hints to gas escaping the galaxy. Finally the paper presents estimates of the gas mass fraction that could escape the gravitational potential of the galaxy.
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Čanda, Pavel. "Bezdrátový přenos dat v pásmu ISM." Master's thesis, Vysoké učení technické v Brně. Fakulta elektrotechniky a komunikačních technologií, 2011. http://www.nusl.cz/ntk/nusl-219136.

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Wireless extension of serial communication of RS232 standard, with using RF transceivers RFM12BP type, with transmissions errors correction. Device will be batery powered and low power consumption is required.
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Zapletal, Ondřej. "Nositelné antény pracující v ISM pásmu." Master's thesis, Vysoké učení technické v Brně. Fakulta elektrotechniky a komunikačních technologií, 2016. http://www.nusl.cz/ntk/nusl-242011.

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Presented thesis is oriented on wearable antennas. The main aim of this thesis is to introduce the basic properties, measurement of textile’s electric properties and several manufacturing methods. The antenna design for the ISM 5.8 GHz bandwidth is also included and further observed by numerical model in CST Microwave Studio. The impact of flexibility and the influence of human tissue are evaluated in the case of designed equipment. According to the optimized design was made several samples by various technologies and samples were measured. Achieved results are further compared to equivalent results listed in actual available references.
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Dale, D. A., D. O. Cook, H. Roussel, J. A. Turner, L. Armus, A. D. Bolatto, M. Boquien, et al. "Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624375.

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We present an update to the ultraviolet-to-radio database of global broadband photometry for the 79 nearby galaxies that comprise the union of the KINGFISH (Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel) and SINGS (Spitzer Infrared Nearby Galaxies Survey) samples. The 34-band data set presented here includes contributions from observational work carried out with a variety of facilities including GALEX, SDSS, Pan-STARRS1, NOAO, 2MASS, Wide-Field Infrared Survey Explorer, Spitzer, Herschel, Planck, JCMT, and the VLA. Improvements of note include recalibrations of previously published SINGS BVRCIC and KINGFISH farinfrared/submillimeter photometry. Similar to previous results in the literature, an excess of submillimeter emission above model predictions is seen primarily for low-metallicity dwarf or irregular galaxies. This 33-band photometric data set for the combined KINGFISH+SINGS sample serves as an important multiwavelength reference for the variety of galaxies observed at low redshift. A thorough analysis of the observed spectral energy distributions is carried out in a companion paper.
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Bieging, John H., Saahil Patel, William L. Peters, L. Viktor Toth, Gábor Marton, and Sarolta Zahorecz. "THE ARIZONA RADIO OBSERVATORY CO MAPPING SURVEY OF GALACTIC MOLECULAR CLOUDS. V. THE SH2-235 CLOUD IN CO J = 2 − 1, 13 CO J = 2 − 1, AND CO J = 3 − 2." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621984.

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We present the results of a program to map the Sh2-235 molecular cloud complex in the CO and (CO)-C-13 J = 2 - 1 transitions using the Heinrich Hertz Submillimeter Telescope. The map resolution is 38 '' (FWHM), with an rms noise of 0.12K brightness temperature, for a velocity resolution of 0.34 km s(-1). With the same telescope, we also mapped the CO J = 3 - 2 line at a frequency of 345 GHz, using a 64 beam focal plane array of heterodyne mixers, achieving a typical rms noise of 0.5 K brightness temperature with a velocity resolution of 0.23 km s(-1). The three spectral line data cubes are available for download. Much of the cloud appears to be slightly sub-thermally excited in the J = 3 level, except for in the vicinity of the warmest and highest column density areas, which are currently forming stars. Using the CO and (CO)-C-13. J = 2 - 1 lines, we employ an LTE model to derive the gas column density over the entire mapped region. Examining a 125 pc(2). region centered on the most active star formation in the vicinity of Sh2-235, we find that the young stellar object surface density scales as approximately the 1.6-power of the gas column density. The area distribution function of the gas is a steeply declining exponential function of gas column density. Comparison of the morphology of ionized and molecular gas suggests that the cloud is being substantially disrupted by expansion of the H II regions, which may be triggering current star formation.
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Books on the topic "ISM"

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A, Begmatov Ė. Ism chiroĭi. Toshkent: Ŭzbekiston respublikasi fanlar akademii͡a︡sining "Fan" nashriëti, 1994.

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JAPON: Ism. Tōkyō: Kyūryūdō, 2011.

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Ism trigonometry 7e. [Place of publication not identified]: Cengage Learning, Inc, 2012.

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Malīkah, Sharīf. al-Ism, Miṣrīyah. al-Qāhirah: al-Ḥaḍārah lil-Nashr, 2005.

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Jurayd, ʻAbd al-ʻAzīz. Mujarrad ism: Riwāyah. Kuwait: Āfāq lil-Nashr, 2019.

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Haqqi, A. H. Ism-e-azam. Lahore: Ali Mian, 2003.

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Kitāb mālūsh ism. 2nd ed. Bayrūt, Lubnān: Dār al-Shurūq, 2009.

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Malīkah, Sharīf. al-Ism, Miṣrīyah. al-Qāhirah: al-Ḥaḍārah lil-Nashr, 2005.

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Fiʻlan ism nadārad. Tihrān: Nashr-i Ufuq, 2002.

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Haqqi, A. H. Ism-e-azam. Lahore: Ali Mian, 2003.

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Book chapters on the topic "ISM"

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Reinelt, Janelle. "International/ism." In Performance Studies, 281–88. London: Macmillan Education UK, 2014. http://dx.doi.org/10.1007/978-1-137-46315-9_32.

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Loomba, Ania. "Commune-ism." In Revolutionary Desires, 112–55. London; New York: Routledge, 2019.: Routledge, 2018. http://dx.doi.org/10.4324/9781351209717-4.

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Furnham, Adrian. "Face-ism and shape-ism at work." In The Talented Manager, 102–4. London: Palgrave Macmillan UK, 2012. http://dx.doi.org/10.1057/9780230369764_24.

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Ottaviani, Alessandro. "Epigenesis/Preformation(ism)." In Lecture Notes in Morphogenesis, 159–63. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-51324-5_33.

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Newman, Fred, and Lois Holzman. "Against Against-ism." In Critical Discursive Psychology, 46–51. London: Palgrave Macmillan UK, 2002. http://dx.doi.org/10.1057/9781403914651_3.

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Sithole, Tendayi. "Ante-Marx(ism)." In Marxism and Decolonization in the 21st Century, 186–209. London: Routledge, 2021. http://dx.doi.org/10.4324/9781003148302-12.

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Fridman, Leonid, Alexander Poznyak, and Francisco Javier Bejarano. "Observer Based on ISM." In Robust Output LQ Optimal Control via Integral Sliding Modes, 21–30. New York, NY: Springer New York, 2014. http://dx.doi.org/10.1007/978-0-8176-4962-3_3.

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Fridman, Leonid, Alexander Poznyak, and Francisco Javier Bejarano. "Multimodel and ISM Control." In Robust Output LQ Optimal Control via Integral Sliding Modes, 59–75. New York, NY: Springer New York, 2014. http://dx.doi.org/10.1007/978-0-8176-4962-3_6.

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Biswas, Sukumar. "The Interstellar Medium (ISM)." In Cosmic Perspectives in Space Physics, 445–68. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-011-4651-7_9.

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Russo, Nancy, and Erik Stolterman. "Identifying Assumptions Underlying ISM." In Business Information Technology Management, 56–71. London: Palgrave Macmillan UK, 2000. http://dx.doi.org/10.1057/9780333977675_5.

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Conference papers on the topic "ISM"

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WEISSGLAS, PETER. "IT-ISM." In Proceedings of Nobel Symposium 92. IMPERIAL COLLEGE PRESS, 1995. http://dx.doi.org/10.1142/9781908979681_0026.

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Chen, Hsiao-Wen. "GRB Afterglows as a New ISM and IGM Probe." In GAMMA-RAY BURSTS IN THE SWIFT ERA: Sixteenth Maryland Astrophysics Conference. AIP, 2006. http://dx.doi.org/10.1063/1.2207950.

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Prabhakar, Dinesh Kumar, and Sukomal Pal. "ISM@FIRE-2014." In the Forum for Information Retrieval Evaluation. New York, New York, USA: ACM Press, 2015. http://dx.doi.org/10.1145/2824864.2824880.

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Prabhakar, Dinesh Kumar, Shantanu Dubey, Bharti Goel, and Sukomal Pal. "ISM@FIRE-2014." In the Forum for Information Retrieval Evaluation. New York, New York, USA: ACM Press, 2015. http://dx.doi.org/10.1145/2824864.2824881.

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Won Kyu Jeung, Chang Hyun Lim, Jingli Yuan, Seung Wook Park, Seog Moon Choi, and Sung Yi. "Reflowable ISM WLP." In 2008 58th Electronic Components and Technology Conference (ECTC 2008). IEEE, 2008. http://dx.doi.org/10.1109/ectc.2008.4549985.

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"Preface: The 3rd ISM International Statistical Conference 2016 (ISM III)." In THE 3RD ISM INTERNATIONAL STATISTICAL CONFERENCE 2016 (ISM-III): Bringing Professionalism and Prestige in Statistics. Author(s), 2017. http://dx.doi.org/10.1063/1.4982830.

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Mohamad, Mohd Sham, Wan Nur Syahidah Wan Yusoff, Nor Aida Zuraimi Md Noar, Roslinazairimah Zakaria, and Mohd Rashid Ab Hamid. "Preface: The 2nd ISM International Statistical Conference 2014 (ISM-II)." In THE 2ND ISM INTERNATIONAL STATISTICAL CONFERENCE 2014 (ISM-II): Empowering the Applications of Statistical and Mathematical Sciences. AIP Publishing LLC, 2015. http://dx.doi.org/10.1063/1.4907418.

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Li, Yun, and Huiying Wu. "An Experimental Investigation of Flow Boiling Characteristics in Interconnected Microchannels With Different Slot Arrangement." In ASME 2022 Heat Transfer Summer Conference collocated with the ASME 2022 16th International Conference on Energy Sustainability. American Society of Mechanical Engineers, 2022. http://dx.doi.org/10.1115/ht2022-81624.

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Abstract Flow boiling in microchannels is a promising approach to solve the heat dissipation problems of the electronic components. In this work, two types of interconnected slot microchannels (SM) with the staggered (SSM) and in-line (ISM) arrangement of the slots (W = 300μm, H = 600μm) are fabricated. Flow boiling experiments are conducted in the SMs (W = 300μm, H = 600μm, L = 35mm) at mass fluxes of 118–370 kg/m2·s, with the deionized water being used as the working fluid. It is found that compared with plain-wall microchannels (PM), the critical heat fluxes (CHF) in ISM are increased by 24.3%∼50.0%, and 30.8∼53.1% for SSM within the test range. The comparative study with PM reveals that SMs can significantly promote the bubbly flow. Equally important, IMs increase the effective heat transfer area while facilitating the redevelopment of the liquid film. Therefore, the heat transfer coefficient (HTC) in ISM and SSM are significantly enhanced by 44.8% ∼ 60.9% and 43.7% ∼ 68.3%, respectively. Furthermore, the connection of the microchannels promotes the mixing of the fluid and enables a more uniform flow distribution in microchannels. The interconnected slots provide the lateral expansion space for bubbles, thus suppressing the reversal flow of the bubbles. Compared with ISM, SSM could break out the long slug bubbles more effectively and prevent gigantic bubbles from forming. The two-phase pressure drop in SSM could be reduced by 23% on average compared with ISM. This work is trying to provide an improved design for microchannels to enhance the flow boiling process.
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"ISM 2008 Conference Organizing Committee." In 2008 Tenth IEEE International Symposium on Multimedia. IEEE, 2008. http://dx.doi.org/10.1109/ism.2008.6.

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"ISM 2008 Technical Program Committee." In 2008 Tenth IEEE International Symposium on Multimedia. IEEE, 2008. http://dx.doi.org/10.1109/ism.2008.7.

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Reports on the topic "ISM"

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Petrowski, Michael, Jeffrey Warga, William Brown, Lauren Gagan, Sue Baumann, James Newman, Cheryl MacKenzie, et al. EFCOG Best Practice The intersection of HPI and Work Planning and Control ISM-HPI-22-01 ISM-WP&C-22-01. Office of Scientific and Technical Information (OSTI), November 2022. http://dx.doi.org/10.2172/1898344.

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Petrowski, Michael, Chuck Ramsey, David Boyce, James Newman, Lloyd Keith, Lauri Minton, Sue Baumann, Tamara Shokes, and Ben Close. EFCOG Best Practice HPI for Knowledge Workers ISM-HPI-22-02. Office of Scientific and Technical Information (OSTI), November 2022. http://dx.doi.org/10.2172/1900463.

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Lacetera, Nicola, and Mario Macis. Moral NIMBY-ism? Understanding Societal Support for Monetary Compensation to Plasma Donors in Canada. Cambridge, MA: National Bureau of Economic Research, May 2018. http://dx.doi.org/10.3386/w24572.

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Corriveau, Elizabeth, and Jay Clausen. Application of Incremental Sampling Methodology for subsurface sampling. Engineer Research and Development Center (U.S.), May 2021. http://dx.doi.org/10.21079/11681/40480.

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Historically, researchers studying contaminated sites have used grab sampling to collect soil samples. However, this methodology can introduce error in the analysis because it does not account for the wide variations of contaminant concentrations in soil. An alternative method is the Incremental Sampling Methodology (ISM), which previous studies have shown more accurately captures the true concentration of contaminants over an area, even in heterogeneous soils. This report describes the methods and materials used with ISM to collect soil samples, specifically for the purpose of mapping subsurface contamination from site activities. The field data presented indicates that ISM is a promising methodology for collecting subsurface soil samples containing contaminants of concern, including metals and semivolatile organic compounds (SVOCs), for analysis. Ultimately, this study found ISM to be useful for supplying information to assist in the decisions needed for remediation activities.
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Lebaric, Jovian, Christos Deyannis, and Dimitrios Xifaras. Effects of Ship Compartment Hydrocarbon Fuel Fire and Water Mist Fire Extinguishing on RF Propagation in the 2.4 GHz ISM Band. Fort Belvoir, VA: Defense Technical Information Center, July 1999. http://dx.doi.org/10.21236/ada410522.

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Clausen, Jay, Samuel Beal, Thomas Georgian, Kevin Gardner, Thomas Douglas, and Ashley Mossell. Effects of milling on the metals analysis of soil samples containing metallic residues. Engineer Research and Development Center (U.S.), July 2021. http://dx.doi.org/10.21079/11681/41241.

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Metallic residues are distributed heterogeneously onto small-arms range soils from projectile fragmentation upon impact with a target or berm backstop. Incremental Sampling Methodology (ISM) can address the spatially heterogeneous contamination of surface soils on small-arms ranges, but representative kilogram-sized ISM subsamples are affected by the range of metallic residue particle sizes in the sample. This study compares the precision and concentrations of metals in a small-arms range soil sample processed by a puck mill, ring and puck mill, ball mill, and mortar and pestle prior to analysis. The ball mill, puck mill, and puck and ring mill produced acceptable relative standard deviations of less than 15% for the anthropogenic metals of interest (Lead (Pb), Antimony (Sb), Copper (Cu), and Zinc (Zn)), with the ball mill exhibiting the greatest precision for Pb, Cu, and Zn. Precision by mortar and pestle, without milling, was considerably higher (40% to >100%) for anthropogenic metals. Media anthropogenic metal concentrations varied by more than 40% between milling methods, with the greatest concentrations produced by the puck mill, followed by the puck and ring mill and then the ball mill. Metal concentrations were also dependent on milling time, with concentrations stabilizing for the puck mill by 300 s but still increasing for the ball mill over 20 h. Differences in metal concentrations were not directly related to the surface area of the milled sample. Overall, the tested milling methods were successful in producing reproducible data for soils containing metallic residues. However, the effects of milling type and time on concentrations require consideration in environmental investigations.
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Doerr, T. Gap Analysis Comparing LLNL ISMS and ISO 14001. Office of Scientific and Technical Information (OSTI), August 2004. http://dx.doi.org/10.2172/15014630.

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Seybold, Patricia. IBM/PWC: Is It Good for Customers? Boston, MA: Patricia Seybold Group, August 2002. http://dx.doi.org/10.1571/psgp8-1-02cc.

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Paul Imhoff, Ramin Yazdani, Don Augenstein, Harold Bentley, and Pei Chiu. Intelligent Bioreactor Management Information System (IBM-IS) for Mitigation of Greenhouse Gas Emissions. Office of Scientific and Technical Information (OSTI), April 2010. http://dx.doi.org/10.2172/1010951.

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Przygienda, T., N. Shen, and N. Sheth. M-ISIS: Multi Topology (MT) Routing in Intermediate System to Intermediate Systems (IS-ISs). RFC Editor, February 2008. http://dx.doi.org/10.17487/rfc5120.

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