Academic literature on the topic 'Icmesa'
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Journal articles on the topic "Icmesa"
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Uhlmann, E. "DISMANTLING OF THE ICMESA TRICHLOROPHENOL PLANT." Health Physics 55, no. 6 (December 1988): 1020. http://dx.doi.org/10.1097/00004032-198812000-00036.
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Bozza-Marrubini, Marialuisa. "Three Major Disasters in Italy. Experiences of Niguarda-Ca'Granda Staff of Milan." Prehospital and Disaster Medicine 1, S1 (1985): 414–19. http://dx.doi.org/10.1017/s1049023x00045325.
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The medical and nursing staff of the Niguarda-Ca' Granda Hospital of Milano has been involved in three major disasters that occurred in Italy in the years 1976 and 1980: (1) the earthquake of May 6, 1976 in a northeastern region (Friuli); (2) the ICMESA plant explosion of July 10, 1976 in Seveso (Milano) and (3) the earthquake of November 23, 1980 in the region of Irpinia (Southern Italy).Friuli Earthquake 1976On May 7, 1976, about 12 hours after the earthquake struck, the Udine Hospital, located at about 15 km from the border of the disaster area, contacted by phone the director of the Ca' Granda Hospital in Milano, requesting a relief staff of operating room and ICU nurses. The Udine Hospital was undamaged and was overburdened by work for the surgical, orthopedic and medical treatment of the rescue victims. The staff requested was needed to relieve the exhausted local nursing staff. Extra staff was needed also to accompany ambulances with patients that, after initial triage and treatment, were evacuated to other hospitals outside the seismic area.
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Kilpua, E. K. J., A. Isavnin, A. Vourlidas, H. E. J. Koskinen, and L. Rodriguez. "On the relationship between interplanetary coronal mass ejections and magnetic clouds." Annales Geophysicae 31, no. 7 (July 23, 2013): 1251–65. http://dx.doi.org/10.5194/angeo-31-1251-2013.
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Abstract. The relationship of magnetic clouds (MCs) to interplanetary coronal mass ejections (ICMEs) is still an open issue in space research. The view that all ICMEs would originate as magnetic flux ropes has received increasing attention, although near the orbit of the Earth only about one-third of ICMEs show clear MC signatures and often the MC occupies only a portion of the more extended region showing ICME signatures. In this work we analyze 79 events between 1996 and 2009 reported in existing ICME/MC catalogs (Wind magnetic cloud list and the Richardson and Cane ICME list) using near-Earth observations by ACE (Advanced Composition Explorer) and Wind. We perform a systematic comparison of cases where ICME and MC signatures coincided and where ICME signatures extended significantly beyond the MC boundaries. We find clear differences in the characteristics of these two event types. In particular, the events where ICME signatures continued more than 6 h past the MC rear boundary had 2.7 times larger speed difference between the ICME's leading edge and the preceding solar wind, 1.4 times higher magnetic fields, 2.1 times larger widths and they experienced three times more often strong expansion than the events for which the rear boundaries coincided. The events with significant mismatch in MC and ICME boundary times were also embedded in a faster solar wind and the majority of them were observed close to the solar maximum. Our analysis shows that the sheath, the MC and the regions of ICME-related plasma in front and behind the MC have different magnetic field, plasma and charge state characteristics, thus suggesting that these regions separate already close to the Sun. Our study shows that the geometrical effect (the encounter through the CME leg and/or far from the flux rope center) does not contribute much to the observed mismatch in the MC and ICME boundary times.
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Grison, Benjamin, Jan Souček, Vratislav Krupar, David Píša, Ondrej Santolík, Ulrich Taubenschuss, and František Nĕmec. "Shock deceleration in interplanetary coronal mass ejections (ICMEs) beyond Mercury’s orbit until one AU." Journal of Space Weather and Space Climate 8 (2018): A54. http://dx.doi.org/10.1051/swsc/2018043.
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The CDPP propagation tool is used to propagate interplanetary coronal mass ejections (ICMEs) observed at Mercury by MESSENGER to various targets in the inner solar system (VEX, ACE, STEREO-A and B). The deceleration of ICME shock fronts between the orbit of Mercury and 1 AU is studied on the basis of a large dataset. We focus on the interplanetary medium far from the solor corona, to avoid the region where ICME propagation modifications in velocity and direction are the most drastic. Starting with a catalog of 61 ICMEs recorded by MESSENGER, the propagation tool predicts 36 ICME impacts with targets. ICME in situ signatures are investigated close to predicted encounter times based on velocities estimated at MESSENGER and on the default propagation tool velocity (500 km s−1). ICMEs are observed at the targets in 26 cases and interplanetary shocks (not followed by magnetic ejecta) in two cases. Comparing transit velocities between the Sun and MESSENGER ($ {\bar{v}}_{\mathrm{SunMess}}$) and between MESSENGER and the targets ($ {\bar{v}}_{\mathrm{MessTar}}$), we find an average deceleration of 170 km s−1 (28 cases). Comparing $ {\bar{v}}_{\mathrm{MessTar}}$ to the velocities at the targets (v Tar), average ICME deceleration is about 160 km s−1 (13 cases). Our results show that the ICME shock deceleration is significant beyond Mercury’s orbit. ICME shock arrival times are predicted with an average accuracy of about six hours with a standard deviation of eleven hours. Focusing on two ICMEs detected first at MESSENGER and later on by two targets illustrates our results and the variability in ICME propagations. The shock velocity of an ICME observed at MESSENGER, then at VEX and finally at STEREO-B decreases all the way. Predicting arrivals of potentially effective ICMEs is an important space weather issue. The CDPP propagation tool, in association with in situ measurements between the Sun and the Earth, can permit to update alert status of such arrivals.
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Zharkova, V., and O. Khabarova. "Additional acceleration of solar-wind particles in current sheets of the heliosphere." Annales Geophysicae 33, no. 4 (April 9, 2015): 457–70. http://dx.doi.org/10.5194/angeo-33-457-2015.
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Abstract. Particles of fast solar wind in the vicinity of the heliospheric current sheet (HCS) or in a front of interplanetary coronal mass ejections (ICMEs) often reveal very peculiar energy or velocity profiles, density distributions with double or triple peaks, and well-defined streams of electrons occurring around or far away from these events. In order to interpret the parameters of energetic particles (both ions and electrons) measured by the WIND spacecraft during the HCS crossings, a comparison of the data was carried out with 3-D particle-in-cell (PIC) simulations for the relevant magnetic topology (Zharkova and Khabarova, 2012). The simulations showed that all the observed particle-energy distributions, densities, ion peak velocities, electron pitch angles and directivities can be fitted with the same model if the heliospheric current sheet is in a status of continuous magnetic reconnection. In this paper we present further observations of the solar-wind particles being accelerated to rather higher energies while passing through the HCS and the evidence that this acceleration happens well before the appearance of the corotating interacting region (CIR), which passes through the spacecraft position hours later. We show that the measured particle characteristics (ion velocity, electron pitch angles and the distance at which electrons are turned from the HCS) are in agreement with the simulations of additional particle acceleration in a reconnecting HCS with a strong guiding field as measured by WIND. A few examples are also presented showing additional acceleration of solar-wind particles during their passage through current sheets formed in a front of ICMEs. This additional acceleration at the ICME current sheets can explain the anticorrelation of ion and electron fluxes frequently observed around the ICME's leading front. Furthermore, it may provide a plausible explanation of the appearance of bidirectional "strahls" (field-aligned most energetic suprathermal electrons) at the leading edge of ICMEs as energetic electrons generated during a magnetic reconnection at the ICME-front current sheet.
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Kilpua, E. K. J., C. O. Lee, J. G. Luhmann, and Y. Li. "Interplanetary coronal mass ejections in the near-Earth solar wind during the minimum periods following solar cycles 22 and 23." Annales Geophysicae 29, no. 8 (August 30, 2011): 1455–67. http://dx.doi.org/10.5194/angeo-29-1455-2011.
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Abstract. In this paper we examine the occurrence rates and properties of interplanetary coronal mass ejections (ICMEs) and solar activity levels during the minima following solar cycle 22 (January 1995–December 1997) and 23 (January 2007–April 2010) minima using observations from the OMNI data base. Throughout the minimum following cycle 22 the CME and ICME rates roughly tracked each other, while for the minimum following cycle 23 they diverged. During the minimum after solar cycle 23, there were large variations in the streamer belt structure. During the lowest activity period of cycle 23 (based on sunspot numbers), the ICME rate was about four times higher than during a similar activity period of cycle 22. We propose that this relatively high ICME rate may be due to CME source regions occurring at lower heliolatitudes and due to equatoward deflection of slow and weak CMEs originating from the mid- and high-heliolatitudes. The maximum magnetic fields of the ICMEs identified during the minimum following cycle 23 were ~30 % lower and their radial widths were ~15 % lower compared to the ICMEs observed during the minimum following solar cycle 22. The weak and small ICMEs may result from intrinsically weak CMEs and/or they may represent stronger CMEs that are encountered far away from the center.
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Kilpua, E. K. J., H. Hietala, H. E. J. Koskinen, D. Fontaine, and L. Turc. "Magnetic field and dynamic pressure ULF fluctuations in coronal-mass-ejection-driven sheath regions." Annales Geophysicae 31, no. 9 (September 10, 2013): 1559–67. http://dx.doi.org/10.5194/angeo-31-1559-2013.
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Abstract. Compressed sheath regions form ahead of interplanetary coronal mass ejections (ICMEs) that are sufficiently faster than the preceding solar wind. The turbulent sheath regions are important drivers of magnetospheric activity, but due to their complex internal structure, relatively little is known on the distribution of the magnetic field and plasma variations in them. In this paper we investigate ultra low frequency (ULF) fluctuations in the interplanetary magnetic field (IMF) and in dynamic pressure (Pdyn) using a superposed epoch analysis of 41 sheath regions observed during solar cycle 23. We find strongest fluctuation power near the shock and in the vicinity of the ICME leading edge. The IMF and Pdyn ULF power have different profiles within the sheath; the former is enhanced in the leading part of the sheath, while the latter is increased in the trailing part of the sheath. We also find that the ICME properties affect the level and distribution of the ULF power in sheath regions. For example, sheath regions associated with strong or fast ICMEs, or those that are crossed at intermediate distances from the center, have strongest ULF power and large variation in the power throughout the sheath region. The weaker or slower ICMEs, or those that are crossed centrally, have in general considerably weaker ULF power with relatively smooth profiles. The strong and abrupt decrease of the IMF ULF power at the ICME leading edge could be used to distinguish the ICME from the preceding sheath plasma.
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Mishra, Wageesh, Kunjal Dave, Nandita Srivastava, and Luca Teriaca. "Multipoint remote and in situ observations of interplanetary coronal mass ejection structures during 2011 and associated geomagnetic storms." Monthly Notices of the Royal Astronomical Society 506, no. 1 (July 13, 2021): 1186–97. http://dx.doi.org/10.1093/mnras/stab1721.
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ABSTRACT We present multipoint remote and in situ observations of interplanetary coronal mass ejection (ICME) structures during the year 2011. The selected ICMEs arrived at Earth on 2011 March 11 and 2011 August 6, and led to geomagnetic storms. Around the launch of these CMEs from the Sun, the coronagraphs onboard STEREO-Aand-B and SOHO enabled the CMEs to be imaged from three longitudinally separated viewpoints. We attempt to identify the in situ plasma and magnetic parameters of the ICME structures at multiple locations, for example at both STEREO spacecraft and also at the ACE/Wind spacecraft near the first Sun–Earth Lagrangian point (L1), to investigate the global configuration, interplanetary propagation, arrival times and geomagnetic response of the ICMEs. The near-Earth identified ICMEs of March 11 and August 6 formed as a result of the interaction of two successive CMEs observed in the inner corona on March 7 (for the March 11 ICME) and on August 3–4 (for the August 6 ICME). Our study suggests that the structures associated with interacting CMEs, possibly as a result of deflection or large sizes, may reach to even larger longitudinally separated locations in the heliosphere. Our multipoint in situ analysis shows that the characteristics of the same shock, propagating in a pre-conditioned medium, may be different at different longitudinal locations in the heliosphere. Similarly, multiple cuts through the same ejecta/complex ejecta, formed as a result of CME–CME interaction, are found to have inhomogeneous properties. The study highlights the difficulties in connecting the local observations of an ICME from a single in situ spacecraft to its global structures.
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Raghav, Anil N., and Zubair I. Shaikh. "The pancaking of coronal mass ejections: an in situ attestation." Monthly Notices of the Royal Astronomical Society: Letters 493, no. 1 (January 17, 2020): L16—L21. http://dx.doi.org/10.1093/mnrasl/slz187.
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ABSTRACT The interplanetary counterparts of coronal mass ejections (ICMEs) are the leading driver of severe space weather. Their morphological evolution in interplanetary space and the prediction of their arrival time at Earth are the ultimate focus of space weather studies, because of their scientific and technological effects. Several investigations in the last couple of decades have assumed that ICMEs have a circular cross-section. Moreover, various models have also been developed to understand the morphology of ICMEs based on their deformed cross-section. In fact, simulation studies have suggested that the initial circular cross-section flattens significantly during their propagation in the solar wind and this is referred to as ‘pancaking’. However, an observational verification of this phenmenon is still pending and it will eventually be the primary concern of several morphological models. Here, we report the first unambiguous observational evidence of extreme flattening of the cross-section of ICMEs, similar to pancaking, based on in situ measurements of 30 ICME events. In fact, we conclude that the cross-section of ICME flux ropes transformed into a two-dimensional planar magnetic structure. Such a deformed morphological feature not only alters the prediction of their arrival time but also has significant implications in solar-terrestrial physics, the energy budget of the heliosphere, charged particle energization, turbulence dissipation and enhanced geo-effectiveness, etc.
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Matamoros, Carolina Salas, Karl Ludwig Klein, and Gerard Trottet. "Microwave radio emissions as a proxy for coronal mass ejection speed in arrival predictions of interplanetary coronal mass ejections at 1 AU." Journal of Space Weather and Space Climate 7 (2017): A2. http://dx.doi.org/10.1051/swsc/2016038.
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The propagation of a coronal mass ejection (CME) to the Earth takes between about 15 h and several days. We explore whether observations of non-thermal microwave bursts, produced by near-relativistic electons via the gyrosynchrotron process, can be used to predict travel times of interplanetary coronal mass ejections (ICMEs) from the Sun to the Earth. In a first step, a relationship is established between the CME speed measured by the Solar and Heliospheric Observatory/Large Angle and Spectrometric Coronagraph (SoHO/LASCO) near the solar limb and the fluence of the microwave burst. This relationship is then employed to estimate speeds in the corona of earthward-propagating CMEs. These speeds are fed into a simple empirical interplanetary acceleration model to predict the speed and arrival time of the ICMEs at Earth. The predictions are compared with observed arrival times and with the predictions based on other proxies, including soft X-rays (SXR) and coronographic measurements. We found that CME speeds estimated from microwaves and SXR predict the ICME arrival at the Earth with absolute errors of 11 ± 7 and 9 ± 7 h, respectively. A trend to underestimate the interplanetary travel times of ICMEs was noted for both techniques. This is consistent with the fact that in most cases of our test sample, ICMEs are detected on their flanks. Although this preliminary validation was carried out on a rather small sample of events (11), we conclude that microwave proxies can provide early estimates of ICME arrivals and ICME speeds in the interplanetary space. This method is limited by the fact that not all CMEs are accompanied by non-thermal microwave bursts. But its usefulness is enhanced by the relatively simple observational setup and the observation from ground, which makes the instrumentation less vulnerable to space weather hazards.
Dissertations / Theses on the topic "Icmesa"
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Skan, Moa. "Reconstructing ICMEs with the toroidal Grad-Shafranov method." Thesis, Uppsala universitet, Institutet för rymdfysik, Uppsalaavdelningen, 2019. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-382398.
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The main objective of this thesis is to model the magneticstructure of interplanetary coronal mass ejections (ICME) measuredin-situ from the WIND spacecraft positioned at L1. The modeling isdone by a magnetohydrodynamic reconstruction technique based onthe GS equation with a toroidal geometry. The purpose has been toextend the application of the reconstruction program to real dataand to test its performance when different input parameters arechanged. Two events are presented; 16-17 May 2012 and 15-16 May2005 ICMEs have been successfully reconstructed with this model. The main achievements of the study are that a) the code now worksfor real data b) the important parameters that can be changed fordifferent reconstructions in the code are the number of iterationsused to find the optimal Z-axis, the plasma pressure and the orderof the polynomial fitting of the flux functional, c) if all crosssection reconstructions for different variations of theseparameters strongly resembles each other then this is anindication that the model approximation is good and that the fluxrope exists. The results have been compared and verified withpreviously published studies of these events. Using a toroidal geometry for the GS reconstruction method weobtain very similar results to the one obtained with differentreconstruction techniques.This implies that at L1, the ICMEs haveexpanded so much that a cylindrical geometry is sufficient todescribe the flux rope geometry. The toroidal Grad-Shafranovreconstruction technique is best suited for circular, or slightlyelongated, flux rope cross section profiles but have been provento work for one complex ejecta consisting of two merged fluxropes. The toroidal model might become an important asset in thefuture when data from spacecraft closer to the Sun, such as ParkerSolar Probe and Solar Orbiter, is public. When the major radius ofthe flux rope is smaller the choice of geometry will most likelyhave a larger role than for measurements at L1 and so, thetoroidal Grad-Shafranov reconstruction technique will probably bethe better alternative of the models that exists today.
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Al-Shakarchi, Duraid A. Mohammed. "A multi-spacecraft study of interacting ICMEs and CIRs in interplanetary space." Thesis, Aberystwyth University, 2018. http://hdl.handle.net/2160/d6aab112-56cc-4c69-9f0c-371f74f78a33.
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This thesis is concerned with studying the interactions of interplanetary large-scale structures with the solar wind and with each other based on multi spacecraft in-situ observations. These structures include: interplanetary coronal mass ejections (ICMEs), stream interaction regions SIRs and heliospheric plasma sheets HPSs. During their propagation through interplanetary space, ICMEs can interact with each other or with CIRs, making space weather forecasting more difficult. Interaction can change their configurations, dynamics, magnetic field and plasma morphologies. This includes flux rope deformation, reverse shock formation, radio emission enhancement, proton temperature increases, and ICME deflections. Caution should be exercised regarding geomagnetic storm forecasting that depends upon ICME magnetic field observations close to the sun, especially when there is an interaction with co-rotating structures, because this interaction could change the profile of the magnetic field measurements. Chapter 3 is a case study that aims to understand more about this interaction based on multi spacecraft in-situ measurements. During September 09- 10, 2011 the ACE, Wind and The Solar and Heliospheric Observatory(SOHO) spacecraft measured a complex interaction between an ICME and a co-rotating interaction region CIR associated with the HPS. A forward shock, sheath, and magnetic cloud was followed by the CIR and a high-speed stream (HSS) originating from a large equatorial coronal hole. Except for a few short periods, the suprathermal electrons are unidirectional with a 180 ̊ pitch angle, suggesting a scenario that the magnetic field of the ICME is open through interchange reconnection. Signatures of interaction between the ICME, CIR and subsequent HSS is distributed throughout the event and not concentrated in a specific position suggesting that the structures have become entangled, or embedded. The forward shock was strong and the ICME speed is not enough to drive it. We attributed the most likely source of the shock as the ICME-CIR interaction. Distinct and Interesting features due to the ICME-CIR/HSS interaction are the heating flux discontinuity upstream of the ICME front shock, the very high proton density in the shock, the significant speed elevation within the sheath, the distortion of Bz in the magnetic cloud, the indistinct location of the stream interface, the unidirectional domination of the suprathermal electrons and the reverse shock at the rear boundary of the CIR. A few days earlier, The Solar Terrestrial Relation Observatory (STEREO) B recorded the passage of the CIR in absence of an ICME. Despite the disruption of the ICME, some general features of the CIR are preserved, showing compression of the CIR by the ICME by a factor of ∼ 4, and enabling some qualitative comparison and further insight into the interaction. Chapter 4 presents an In-Situ study of a compound stream event measured by the STEREO B on March20-25, 2011. During the period, in situ results were obtained by STEREO B measuring a compound stream containing several interacting structures. An analysis of these results suggests that the stream consists of two interplanetary coronal mass ejections (ICMEs) followed by an embedded ICME/CIR. The third ICME has merged with, and is embedded within, a CIR. A significant stream interface has appeared within the ICME3 revealing the ability of this structure to penetrate the magnetic flux rope and change its physical properties, particularly its temperature. The sudden appearance of ICME3 within the fast wind side of the CIR causes the temperature to drop suddenly to its lowest level in about 1.2 hours, from 3.89 x 105 K to 1.07 x 104 K. Conversely, the fast wind which follows the CIR influences not only the ICME3 temperature but also its plasma β. In addition, the third ICME impacts the CIR through expansion and deceleration. Penetration of a forward pressure wave driven by this combined ICME-CIR causes an increase in the temperature and plasma beta of the second ICME and part of the first. Despite the presence of signatures from four large-scale interacting structures within the compound stream, it is difficult to reconcile the in-situ sequence with remote sensing observations of CMEs and ejecta close to the Sun. Compound streams therefore remain difficult to interpret, and further understanding of the subject will depend on the future study of similar events. Chapter 5 concentrates on tracking the evolution of a CIR during its propagation through the interplanetary spiral pattern (180 degrees of longitude) and its interaction with other interplanetary structures from period 20 April 2011 to 8 May 2011 based on multi spacecraft in situ observations (STEREO B, WIND, ACE and STEREO A). The results reveal an interaction with two-magnetic cloud flux ropes embedded within the CIR at Lagrange L1 and STEREO A (STA) positions. The role of these interplanetary magnetic flux ropes was noticeable on the CIR morphology by changing its reverse shock and stream interaction (SI) behaviours, with an obvious appearance of the SI within the magnetic cloud flux rope which is embedded with the CIR. The appearance of the reverse shock at STEREO B (STB), disappearance at L1 region, and then an appearance at STEREO A, imply that the CIR reverse shock behaviour was subjected to the local interplanetary circumstance, such as transient ICME interactions. It also reveals the CIR’s ability to recover its magnetic field and plasma morphology after disruption by ICMEs. The L1 ICME changes the CIR speed and dynamic pressure profiles. consequently, the acting forces at both reverse shock sides have changed, leading to the disappearance of the reverse shock at L1. At STA, the ICME deceleration has moved the position of the CIR’s maximum speed (Vmax) back to the rear CIR boundary, similar to position at STB. The SIs location has approached the Vmax location. These two changes made the profile of the dynamic pressure near the rear of the CIR to return to a state similar to that seen at STB, and thus, the reverse shock reappears. The ICME-CIR interaction at L1 and STA effects the HCS by the growth of the heliospheric plasma sheet (HPS) at the front of the events which coincided with the existence of the magnetic clouds within the CIR.
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Moreira, Mélsi. "ICMS :." Florianópolis, SC, 1999. http://repositorio.ufsc.br/xmlui/handle/123456789/81095.
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Dissertação (Mestrado) - Universidade Federal de Santa Catarina, Centro de Ciências Jurídicas.Made available in DSpace on 2012-10-18T23:09:09Z (GMT). No. of bitstreams: 0Bitstream added on 2016-01-09T04:20:53Z : No. of bitstreams: 1 152749.pdf: 5639113 bytes, checksum: 68323fd73990d54dcfd6f643b92af3e6 (MD5)
Este trabalho enfoca, como temática central o estudo sobre a sonegação fiscal do ICMS no Estado de Santa Catarina e o dano social dela decorrente. Responde ele ás seguintes a) Existe sonegação fiscal deste imposto no Estado? b) Ela causa dano social - aqui entendendo-se a postergação e/ou ausência de obras e serviços públicos - á população catarinense?
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Jorge, Plínio Augusto Lemos. "Não-cumulatividade no ICMS." Pontifícia Universidade Católica de São Paulo, 2009. https://tede2.pucsp.br/handle/handle/8629.
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Previous issue date: 2009-06-04The object of this work is the study of the non-cumulativeness principle in the ICMS concept. In this way, it aims to accomplish this study under the parameter of Constitutional supremacy, taking under consideration the hierarchy of the rules of positive law. The quality of principle assigned to the non-cumulativeness is a recurring theme at work, before the necessity of situating above other rules of Brazilian positive law to demonstrate, in a clear way, the necessity of its observance. Therefore, we will study the Brazilian constitutional system and the competence in creation of tributes in the course of the work, following the study about the general constitutional as well as the taxation principles. It approaches the ICMS characteristics using the incidence of taxation origin of this income and from then on, it leads to the non-cumulativeness principle study, its origin, concepts and its relation to the Complementary Law. Finally, it sets up the study of the principle under the established exceptions in the Federal Constitution and the created exceptions made by the infra-constitutional legislator. Due to the amplitude of the theme, a few epistemological cuts will be made. However, no dissolution of the continuity of the work object was implied. On the contrary, there was an effort to deepen the work theme so as to demonstrate the peculiarities of the non-cumulativeness in the Brazilian legal ordinance. Anyway, the conclusion aimed claims the close importance of the non-cumulativeness principle as a unique route to the correct incidence of the ICMS
O presente trabalho tem por objeto o estudo do princípio da não-cumulatividade no âmbito do ICMS. Busca-se, destarte, realizar o estudo tendo como parâmetro a supremacia Constitucional, levando-se em consideração a hierarquia das normas de Direito Positivo. A qualidade de princípio atribuída a não-cumulatividade é tema recorrente no trabalho, ante a necessidade de situá-la acima das outras normas do Direito Positivo brasileiro para demonstrar, de forma clara e cristalina, a necessidade de sua observância. Para tanto, no decorrer do trabalho estudaremos o sistema constitucional brasileiro e a competência para a criação dos tributos, seguindo-se para o estudo sobre os princípios constitucionais gerais e os princípios constitucionais tributários. Aborda-se as características do ICMS utilizando-se, para tanto, a regra matriz de incidência tributária deste imposto e a partir daí passa-se ao estudo do princípio da não-cumulatividade, sua origem, conceitos e sua relação com a Lei Complementar. Faz-se, por fim, o estudo do princípio em face das exceções estabelecidas na Constituição Federal e as exceções criadas pelo legislador infraconstitucional. Alguns cortes epistemológicos serão feitos, dada a amplitude do tema, sem, contudo, implicar dissolução de continuidade do assunto objeto do trabalho. Ao contrário, procurou-se o aprofundamento do tema, de sorte a demonstrar as peculiaridades da não-cumulatividade no ordenamento legal brasileiro. De todo modo, a conclusão almejada diz com a inafastável importância do princípio da não-cumulatividade, como único trajeto à correta incidência do ICMS
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Roncaratti, Luanna Sant’Anna. "O ICMS como subsistema político." reponame:Repositório Institucional da UnB, 2007. http://repositorio.unb.br/handle/10482/2524.
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Dissertação (mestrado)—Universidade de Brasília, Instituto de Ciência Política, Programa de Pós-Graduação, 2007.Submitted by Fernanda Weschenfelder (nandaweschenfelder@gmail.com) on 2009-12-04T13:36:59Z No. of bitstreams: 1 2007_LuannaSant'AnnaRoncaratti.PDF: 637344 bytes, checksum: 04057c653d0564f908edbd8855adf3df (MD5)
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A matéria tributária tem sido um dos principais temas na agenda pública brasileira dos últimos anos. A carga tributária no Brasil tem aumentado de forma significativa e inúmeras reformas do sistema tributário têm sido propostas. O tema torna-se ainda mais relevante quando se percebe que estas reformas não foram aprovadas e que as distorções tributárias do sistema brasileiro não têm sido minimizadas, comprometendo a promoção do desenvolvimento do país. Esta dissertação visa a tratar a questão tributária no Brasil sob a ótica da ciência política, buscando aplicar a ela o modelo analítico de subsistema de governo. Para tanto, optou-se por dois recortes no objeto de estudo. O primeiro refere-se à escolha do Imposto sobre a Circulação de Mercadorias e Serviços – ICMS - para ser examinado. O segundo recorte é temporal e envolve o período de 1987 a 2006. Assim, o objetivo da dissertação é examinar o subsistema de governo que envolve o ICMS no Brasil no período entre 1987 e 2006. Ou seja, busca-se compreender a forma na qual as medidas que se referem a esse tributo surgem, como funcionam as arenas onde são discutidas, como são tratadas e quais os principais atores que as influenciam. O método utilizado na realização da pesquisa foi a seleção de alguns eventos importantes para o subsistema do ICMS e a descrição desses acontecimentos, de forma a se destacar como eles ocorreram, onde e quais os participantes envolvidos. Dois tipos de eventos foram tratados: episódios marcantes de guerra fiscal entre Estados federados e tentativas de alterações do sistema tributário brasileiro. Para se construir um quadro explicativo adequado acerca do subsistema de governo do ICMS, apresentou-se as teorias e modelos analíticos que fundamentaram a escolha do objeto de estudo, discorreu-se sobre as principais características do sistema tributário brasileiro, descreveu-se os eventos selecionados e, por fim, realizou-se a análise de como se estrutura o subsistema, apontando as suas especificidades, suas arenas, seus atores e sua dinâmica de atuação. _______________________________________________________________________________ ABSTRACT
The tributary subject has been one of the main themes in the Brazilian public agenda on the last years. The tax burden in Brazil has considerably increased and many reforms of the tributary system have been proposed. The subject becomes even more relevant when it is noted that these reforms were not approved and that the tributary distortions of the Brazilian system have not been reduced, jeopardizing the development of the country. This dissertation aims to treat the tributary question in Brazil under the political science optic, seeking to apply to it the analytical model of political subsystem. To accomplish that, two cutout were made in the study object. The first one refers to the choice of the Tax over the Circulation of Goods and Services (ICMS) to be examined. The second cutout is temporal and involves the period of 1987 to 2006. Then, the objective of the dissertation is to examine the political subsystem that involves the ICMS in Brazil during the period between 1987 and 2006. This study seeks to comprehend the form in which the decisions referred to this tax emerge, how the arenas where they are discussed work, how they are treated and which are the main actors influencing them. The method utilized in this inquiry was the selection of some important events to the ICMS subsystem and the description of these happenings; seeking to accentuate how they occurred, where and which were the participants involved. Two kinds of events were approached: important episodes of fiscal war between states and tentatives of alteration in the Brazilian tributary system. In order to construct an appropriate picture to explicate the political subsystem of ICMS, theories and analytical models that founded the choice of the study subject were presented, the main characteristics of the Brazilian tributary system were discussed, the selected events were described and an analysis of the structure of the subsystem were made, pointing out its specificities, its arenas, its actors and its dynamic.
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Pacheco, Filho Velocino. "A substituição tributária no ICMS /." Florianópolis, SC, 1999. http://repositorio.ufsc.br/xmlui/handle/123456789/80598.
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Vasconcellos, Mônica Pereira Coelho de. "ICMS: distorções e medidas de reforma." Universidade de São Paulo, 2013. http://www.teses.usp.br/teses/disponiveis/2/2133/tde-06022014-135007/.
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A dissertação tem por objetivo empreender uma análise, sob o ângulo jurídico, da tributação do consumo por meio do ICMS, que representa atualmente o tributo de maior arrecadação dentre tantos outros existentes em nosso país. O estudo demonstra que, rompendo com a prática comum a outros países, de atribuir a tributação sobre o consumo ao poder central, no Brasil, a competência para instituição e a capacidade para cobrança do ICMS foram alocadas às diversas unidades subnacionais integrantes da Federação, que acabou provocando graves assimetrias e distorções em nosso sistema tributário. Ademais, a estrutura consagrada constitucionalmente, chancelando a competência dos Estados da Federação relativamente ao ICMS, acirrou a guerra fiscal, praticada por meio da concessão de incentivos à margem da legislação vigente, de um lado, e, em contrapartida, a reação de alguns Estados, tão questionável quanto a própria concessão irregular de benefícios fiscais, no sentido de negar o reconhecimento do crédito de ICMS já pago em outras unidades da Federação. O estudo concentra-se, portanto, em analisar o perfil do ICMS, as limitações ao aproveitamento de crédito e a consequente guerra fiscal, para tratar da possibilidade de reforma tributária que pretende alterar significativamente a estrutura do referido imposto, a fim de permitir uma convivência equilibrada entre os Entes da Federação, a fim de garantir uma política econômica voltada para aceleração do crescimento do país.The purpose of the dissertation is the analysis, from a legal viewpoint, of tax on consumption, through Sales Tax (ICMS), which currently represents the tax which is most paid among so many others existing in our country. The study shows that, breaking with the common practice of other countries, namely, of attributing taxation on consumption to the central government, in Brazil, competence for the institution and capacity of imposing ICMs has been allocated to several sub-national units comprised in the government, which finally triggered severe asymmetries and distortions in our tax system. Moreover, the structure constitutionally acknowledged, which approves the competence of the Federal States referent to the ICMS, intensified the fiscal war, practiced by concession of incentives beyond, on the one hand, the legislation in force, and, on the other, the reaction of some States, as questionable as the irregular concession of tax benefits, in the sense of refusing to acknowledge ICMS credit already paid in other Federal States. The study is therefore focused on analyzing the ICMS features, the limitations for the offset of ICMS credits and the consequent fiscal war, in order to address the possibility of a tax reform which seeks to significantly alter the structure of aforesaid tax, in order to allow for a balanced relationship between the Federal States, so as to ensure an economic policy directed towards an upturn in the growth of the country.
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Albuquerque, Gustavo Augusto Nunes de. "O impacto da desoneração do ICMS nas exportações sobre a arrecadação do ICMS no estado do Ceará." reponame:Repositório Institucional da UFC, 2009. http://www.repositorio.ufc.br/handle/riufc/24939.
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ALBUQUERQUE, Gustavo Augusto Nunes de. O impacto da desoneração do ICMS nas exportações sobre a arrecadação do ICMS no estado do Ceará. 2009. 80 f. Dissertação (mestrado) - Universidade Federal do Ceará, Faculdade de Economia, Administração, Atuária e Contabilidade, Programa de Pós-Graduação em Administração e Controladoria, Fortaleza-CE, 2009.Submitted by Dioneide Barros (dioneidebarros@gmail.com) on 2017-08-22T14:35:39Z No. of bitstreams: 1 2009_dis_ganalbuquerque.pdf: 309143 bytes, checksum: 81c0720fd9e6bb15884977fa8da63dc0 (MD5)
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The exemption of the Tax Movement of Goods and Services (ICMS) on exports of primary products and semi-manufactured products introduced by Complementary Law no. 87/96, known as the Kandir Law, aimed to increase the competitiveness of Brazilian exports and therefore increase the level of growth in the gross domestic product of Brazil. For the justification of the law, the expected economic effect from the tax relief was to generate positive internal revenue tax that would compensate (or more than offset) the losses of tax revenue suffered by the state of Ceará. This study aims to quantify and analyze the loss of tax revenue incurred by the state of Ceará for the period of 1991 to 2007, assuring that the Insurance Revenue Fund, the Budget and Financial Aid were enough to satisfactorily compensate the decrease in revenue. The literature on the subject, using different methodologies, shows many differences in the levels of losses in each State and that compensation arising from the federal government has not been sufficient to offset it. This paper uses the descriptive analysis of the data and analysis of the econometric model. It was found that there was a trend in exports, especially in manufacturing, revealing that the Kandir Law did not impact the expected size. The revenue collection, however, was affected by the tariff reduction, with implications of loss to the Treasury, which were not offset by the constitutional transfers. It can be concluded that the Kandir Law had a negative impact on the collection of ICMS, not identifying a new dynamic in the exports of Ceará.
A desoneração do Imposto sobre Operações Relativas à Circulação de Mercadorias e sobre Prestações de Serviços de Transporte Interestadual e Intermunicipal e de Comunicação (ICMS) nas exportações de produtos primários e semielaborados, instituída pela Lei Complementar n°. 87/96, conhecida como Lei Kandir, teve como objetivo aumentar a competitividade das exportações brasileiras e, por conseguinte, elevar o patamar do crescimento do produto interno bruto do País. Pela justificativa da lei, com a desoneração fiscal, esperava-se efeito econômico positivo que gerasse receita tributária interna capaz de compensar (ou mais do que compensar) as perdas de arrecadação tributária sofridas pelo Ceará. Este estudo objetiva quantificar e analisar as perdas da arrecadação tributária incorridas pelo Ceará para o período 1991 a 2007, verificando se o Seguro-Receita, o Fundo Orçamentário e o Auxílio Financeiro foram suficientes para compensar satisfatoriamente o decréscimo da arrecadação. A literatura sobre o assunto, usando metodologias distintas, mostra muitas divergências quanto aos níveis de perdas em cada Estado brasileiro e que as compensações originadas no Governo Federal não têm sido suficientes para compensá-las. Este trabalho busca utilizar a estatística descritiva dos dados e a análise do modelo econométrico. Foi constatado que houve uma evolução nas exportações, notadamente nos manufaturados, revelando que a Lei Kandir não impactou na dimensão esperada. A arrecadação, no entanto, foi afetada por essa desoneração, com implicações de perdas para o erário, que não foram compensadas pelas transferências constitucionais. Conclui-se que a Lei Kandir produziu efeitos negativos sobre a arrecadação do ICMS, sem ensejar uma nova dinâmica na pauta de exportação cearense
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Cabral, Guilherme Sanrley Ribeiro. "ICMS Ecol?gico: as unidades de conserva??o como instrumento econ?mico para gest?o ambiental municipal." UFVJM, 2018. http://acervo.ufvjm.edu.br/jspui/handle/1/1820.
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Coordena??o de Aperfei?oamento de Pessoal de N?vel Superior (CAPES)
Tem sido cada vez mais imposs?vel separar as an?lises ambientais das influ?ncias econ?micas. Devido a essa rela??o, instrumentos econ?micos t?m sido utilizados como ferramenta de gest?o ambiental. Alguns estados adotaram crit?rios ambientais na distribui??o dos recursos arrecadados pelo ICMS aos munic?pios, conhecidos como ICMS Ecol?gico. Para conhecer melhor o uso deste instrumento nos estados brasileiros e no munic?pio de Diamantina - Minas Gerais, foi realizado um levantamento bibliogr?fico, com base em dados p?blicos e produ??o cient?fica. Uma an?lise da legisla??o de cada estado foi realizada. Sobre Minas Gerais, foi criada uma planilha eletr?nica autom?tica que simula a potencial arrecada??o financeira de um munic?pio, em uma poss?vel cria??o ou modifica??o de uma unidade de conserva??o. Atualmente, dezessete estados brasileiros j? implementaram o ICMS Ecol?gico. Os resultados dessa pol?tica ambiental levaram ao aumento do n?mero e da qualidade das unidades de conserva??o, ? expans?o da ?rea e ao aumento da implanta??o de sistemas de saneamento ambiental. No entanto, ainda ? necess?rio gerar um modelo de distribui??o de recursos baseado nos diversos aspectos da ?rea ambiental, como gest?o e educa??o ambiental, biodiversidade e conserva??o do solo, potencial h?drico, etc. Diamantina possui sete unidades de conserva??o, que totalizam 55816,11 hectares, correspondendo a 14,34% do territ?rio. De 2005 a 2017, o munic?pio j? recebeu cerca de R $ 1.755.285,64, provenientes do subcrit?rio de conserva??o. Em 2017, a coleta m?dia mensal foi de R$ 13.663,83. Relacionando estes valores com a ?rea protegida chegasse a uma taxa de 24 centavos por hectare, o que demonstra a baixa valoriza??o dos servi?os ambientais prestados pelas ?reas protegidas. ? necess?rio alocar uma maior porcentagem de recursos do ICMS ao crit?rio ambiental, al?m de uma reformula??o no c?lculo do ?ndice de conserva??o, de forma a buscar uma melhor remunera??o dos munic?pios que conservam ?reas maiores.
Disserta??o (Mestrado) ? Programa de P?s-Gradua??o em Ci?ncia Florestal, Universidade Federal dos Vales do Jequitinhonha e Mucuri, 2018.
It has been increasingly impossible to separate environmental analyzes from economic influences. Due to this relationship, economic instruments have been used as an environmental management tool. Some states have adopted environmental criteria in the distribution of resources collected by ICMS to municipalities, known as Ecological ICMS. To better understand the use of this instrument in the Brazilian states and in the municipality of Diamantina - Minas Gerais, a bibliographic survey was carried out, based on public data and scientific production. An analysis of the legislation of each state was carried out. About Minas Gerais, an automatic spreadsheet was created that simulates the potential financial collection of a municipality, in a possible creation or modification of a conservation unit. Currently, seventeen Brazilian states have already implemented the Ecological ICMS. The results of this environmental policy led to an increase in the number and quality of conservation units, the expansion of the area and the increase in the implementation of environmental sanitation systems. However, it is still necessary to generate a resource distribution model based on the various aspects of the environmental area, such as environmental management and education, biodiversity and soil conservation, water potential, etc. Diamantina has seven conservation units, which total 55816.11 hectares, corresponding to 14.34% of the territory. From 2005 to 2017, the municipality has already received about R $ 1,755,285.64 from the conservation sub-criterion. In 2017, the average monthly collection was R $ 13,663.83. Relating these values to the protected area reached a ratio of 24 cents per hectare, which shows the low value of environmental services provided by protected areas. It is necessary to allocate a greater percentage of ICMS resources to the environmental criterion, besides a reformulation in the calculation of the conservation index, in order to seek a better remuneration of the municipalities that conserve larger areas.
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Cunha, Rose Dias. "A influência do ICMS na escolha da localização dos centros de distribuição no setor de defensivos agrícolas." Universidade de São Paulo, 2008. http://www.teses.usp.br/teses/disponiveis/12/12139/tde-20012009-161336/.
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Esse trabalho, pertencente à disciplina de Gestão de Operações, é um esforço no sentido de recortar a questão tributária da teoria sobre localização de centros de distribuição, e discutir esse tema sob a visão do ICMS, principal imposto brasileiro aplicado à distribuição de mercadorias. A questão tributária é um elemento usualmente citado como fator presente nas escolhas de localização de unidades produtivas e centros de distribuição. Entretanto, essa variável é ainda considerada como periférica, sendo pouco explorada em pesquisas acadêmicas relacionadas à literatura localizacional. Foram estabelecidos os objetivos de identificar a presença do ICMS nas escolhas por centros de distribuição e encontrar elementos que possam evidenciar afirmações sobre a influência desse imposto nas decisões de quatro empresas do setor de defensivos agrícolas. A metodologia empregada nesse trabalho foi a de estudo de casos múltiplos, baseado na observação e descrição de processos cronológicos de decisão reais, com o suporte de um roteiro de questões para a realização das entrevistas com os responsáveis pela gestão de distribuição A escolha do setor de defensivos deve-se à presença de fortes benefícios fiscais relativos ao ICMS, como isenção de pagamento para faturamento intra-estadual. A pesquisa conseguiu identificar a divisão dos fatores influenciadores da decisão em dois blocos, extra tributários e tributários, sendo os extra correspondentes aos fatores logísticos comumente estudados em pesquisas, como prazos de entrega, custos de transporte e armazenagem e os tributários ligados especificamente ao ICMS. Os resultados encontrados permitem dizer que o ICMS foi um fator presente em todos os processos de decisão, variando segundo as perspectivas financeiras relacionadas às perdas por créditos não aproveitados, implicações legais, vantagens competitivas de preços e custos de transações decorrentes de acordos especiais com clientes. A pesquisa aponta uma afirmação baseada em evidências encontradas nas quatro empresas estudadas de que qualquer decisão por centro de distribuição passa pela validação da área tributária. Além disso, comportamentos e aspectos técnicos semelhantes foram observados na organização e estrutura dos projetos para definir centros de distribuição. Outra importante conclusão é de que existe um grau de conhecimento e consciência comum sobre a influência desse imposto sobre as operações das empresas. Do ponto de vista acadêmico, a grande contribuição desse trabalho é a afirmação de que, dados os mecanismos de fomento, cobrança e compensações do ICMS, as empresas do setor de defensivos podem ter que adotar estratégias de localização que sobrepujam vantagens logísticas. E essa é, provavelmente, uma verdade para qualquer setor onde estejam presentes benefícios fiscais e alto valor agregado das mercadorias comercializadas. O aprofundamento sobre tais estratégias que as empresas devem adotar para lidar com o ICMS é a principal recomendação desse trabalho para futuros estudos acadêmicos.This research, which belongs to the Operations Management subject, is an effort towards investigating the tax issue, inserted in the distribution centers location theory and discussing this theme under ICMS perspective, the main tax regarding goods circulation in Brazil. The tax issue is usually mentioned as one of the aspects to be considered when choosing the localization of manufacturing units and distribution centers. However, this topic is still considered less relevant than other logistics features and therefore is not deeply studied by academic researches related to location literature. There were established the objectives of identifying the presence of ICMS on the decisions concerning distributions centers localizations and finding elements that could be evidences of affirmations regarding its influence on the decisions in four companies of crop protection products. The methodology is a multiple cases study, based on observation and description of real and chronological decision processes, supported by a script of questions to interview the responsible ones for distribution functions. The choice of the crop protection business is due to the strong existence of tax benefits on this field concerning ICMS, such as payment exemption in case of intra state distribution. It was possible to identify two groups of factors, the logistics and the tax ones, being the logistics factors frequently studied as the freight, warehousing costs and lead times issues and the tax factor associated to the specific ICMS subject. The results found allow to state that ICMS was an important variable in all decision processes assuming four perspectives: financial, related to losses due to credits not consumed; legal implications, prices competitiveness advantage and transactions costs regarding special customer agreements. Based on evidences found in the four analyzed companies, this research confirms that any location decision has to be validated by the tax management. In addition, similar behavior and technical aspects were observed on the organization and structure of projects to define distribution centers. Other important conclusion is the common conscience shared among the four companies about the ICMS influence on their operations. From an academic perspective, the main contribution of this study is the affirmation that, given the foment, charging and compensations mechanisms of the ICMS, the companies from the crop protection business analyzed might have to adopt localization strategies that overcomes the logistical advantages. And this is, probably, truth to any sector whereas tax benefits and high value commercialized goods are present. The deep study about those strategies that companies have to adopt to deal with ICMS is the main recommendation of this essay for future academic researches.
Books on the topic "Icmesa"
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Centemeri, Laura. Ritorno a Seveso: Il danno ambientale, il suo riconoscimento, la sua riparazione. [Milan, Italy]: B. Mondadori, 2006.
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La mina vagante: Il disastro di Seveso e la solidarietà nazionale. Milano, Italy: FrancoAngeli, 2010.
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Association, Irish Creamery Milk Suppliers. ICMSA guide to rural development. Limerick: ICMSA, 1994.
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International Conference on Modern Aspects of Superconductivity (4th 1992 Paris, France). ICMAS-92. Edited by Chu Ching-wu 1941-, Fink J, and IITT-International. Gournay sur Marne: IITT-International, 1992.
Find full textBook chapters on the topic "Icmesa"
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Howard, Timothy. "Geometry of CMEs and ICMEs." In Astrophysics and Space Science Library, 101–14. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-8789-1_5.
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Taylor, Ann C. M. "Pax Romana (ICMICA/MIIE)." In World List of Universities / Liste Mondiale des Universites, 792. London: Palgrave Macmillan UK, 1992. http://dx.doi.org/10.1007/978-1-349-12037-6_32.
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Prahl, Ulrich, and Georg J. Schmitz. "Future ICME." In Integrative Computational Materials Engineering, 305–21. Weinheim, Germany: Wiley-VCH Verlag GmbH & Co. KGaA, 2012. http://dx.doi.org/10.1002/9783527646098.ch13.
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Gazis, P. R., A. Balogh, S. Dalla, R. Decker, B. Heber, T. Horbury, A. Kilchenmann, et al. "ICMEs at High Latitudes and in the Outer Heliosphere." In Space Sciences Series of ISSI, 417–51. New York, NY: Springer New York, 2006. http://dx.doi.org/10.1007/978-0-387-45088-9_16.
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Forsyth, R. J., V. Bothmer, C. Cid, N. U. Crooker, T. S. Horbury, K. Kecskemety, B. Klecker, et al. "ICMEs in the Inner Heliosphere: Origin, Evolution and Propagation Effects." In Space Sciences Series of ISSI, 383–416. New York, NY: Springer New York, 2006. http://dx.doi.org/10.1007/978-0-387-45088-9_15.
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Crooker, N. U., and T. S. Horbury. "Solar Imprint on ICMEs, Their Magnetic Connectivity, and Heliospheric Evolution." In Space Sciences Series of ISSI, 93–109. New York, NY: Springer New York, 2006. http://dx.doi.org/10.1007/978-0-387-45088-9_7.
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Hashibon, Adham, Önder Babur, Mauricio Hanzich, Guillaume Houzeaux, and Bořek Patzák. "Platforms for ICME." In Handbook of Software Solutions for ICME, 533–64. Weinheim, Germany: Wiley-VCH Verlag GmbH & Co. KGaA, 2016. http://dx.doi.org/10.1002/9783527693566.ch8.
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Horstemeyer, Mark F., and Satyam Sahay. "Definition of ICME." In Integrated Computational Materials Engineering (ICME) for Metals, 1–17. Hoboken, NJ, USA: John Wiley & Sons, Inc., 2018. http://dx.doi.org/10.1002/9781119018377.ch1.
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Von Steiger, R., and J. D. Richardson. "ICMEs in the Outer Heliosphere and at High Latitudes: an Introduction." In Space Sciences Series of ISSI, 111–26. New York, NY: Springer New York, 2006. http://dx.doi.org/10.1007/978-0-387-45088-9_8.
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Lario, David. "Radial and latitudinal variations of the energetic particle response to ICMEs." In Solar Eruptions and Energetic Particles, 309–19. Washington, D. C.: American Geophysical Union, 2006. http://dx.doi.org/10.1029/165gm29.
Full textConference papers on the topic "Icmesa"
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Leitner, M., C. J. Farrugia, M. Maksimovic, K. Issautier, N. Meyer-Vernet, M. Moncuquet, and F. Pantellini. "Solar wind quasi invariant within ICMEs." In TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP, 2010. http://dx.doi.org/10.1063/1.3395951.
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"ICMEAE 2019 Commentary." In 2019 International Conference on Mechatronics, Electronics and Automotive Engineering (ICMEAE). IEEE, 2019. http://dx.doi.org/10.1109/icmeae.2019.00001.
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"ICMEAE 2019 Commentary." In 2019 International Conference on Mechatronics, Electronics and Automotive Engineering (ICMEAE). IEEE, 2019. http://dx.doi.org/10.1109/icmeae.2019.00002.
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"ICMEAE 2019 TOC." In 2019 International Conference on Mechatronics, Electronics and Automotive Engineering (ICMEAE). IEEE, 2019. http://dx.doi.org/10.1109/icmeae.2019.00004.
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"ICMEAE 2019 Opinion." In 2019 International Conference on Mechatronics, Electronics and Automotive Engineering (ICMEAE). IEEE, 2019. http://dx.doi.org/10.1109/icmeae.2019.00005.
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"ICMEAE 2019 Committees." In 2019 International Conference on Mechatronics, Electronics and Automotive Engineering (ICMEAE). IEEE, 2019. http://dx.doi.org/10.1109/icmeae.2019.00006.
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"ICMEAE 2019 Index." In 2019 International Conference on Mechatronics, Electronics and Automotive Engineering (ICMEAE). IEEE, 2019. http://dx.doi.org/10.1109/icmeae.2019.00037.
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"ICMEAE 2019 Commentary." In 2019 International Conference on Mechatronics, Electronics and Automotive Engineering (ICMEAE). IEEE, 2019. http://dx.doi.org/10.1109/icmeae.2019.00038.
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Démoulin, Pascal, M. Maksimovic, K. Issautier, N. Meyer-Vernet, M. Moncuquet, and F. Pantellini. "Interaction of ICMEs with the Solar Wind." In TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP, 2010. http://dx.doi.org/10.1063/1.3395866.
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"ICMEAE 2019 Breaker Page." In 2019 International Conference on Mechatronics, Electronics and Automotive Engineering (ICMEAE). IEEE, 2019. http://dx.doi.org/10.1109/icmeae.2019.00003.
Full textReports on the topic "Icmesa"
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Chellappa, Rama, and B. Yegnanarayana. Travel Grant-ICMPS. Fort Belvoir, VA: Defense Technical Information Center, May 2001. http://dx.doi.org/10.21236/ada389862.
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Levesque-Tremblay, Gabriel. International Conference on Microbiome Engineering (ICME 2018). Office of Scientific and Technical Information (OSTI), November 2018. http://dx.doi.org/10.2172/1592173.
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Hall, Charles A., and Thomas A. Porsching. Computational Fluid Dynamics at ICMA (Institute for Computational Mathematics and Applications). Fort Belvoir, VA: Defense Technical Information Center, October 1988. http://dx.doi.org/10.21236/ada204967.
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Hammi, Youssef, Mark F. Horstemeyer, Paul Wang, Francis David, and Ricolindo Carino. Optimization Using Metamodeling in the Context of Integrated Computational Materials Engineering (ICME). Office of Scientific and Technical Information (OSTI), November 2013. http://dx.doi.org/10.2172/1105915.
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Cowles, Bradford A., and Daniel Backman. Advancement and Implementation of Integrated Computational Materials Engineering (ICME) for Aerospace Applications. Fort Belvoir, VA: Defense Technical Information Center, March 2010. http://dx.doi.org/10.21236/ada529049.
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Li, Mei. ICME Guided Development of Advanced Cast Aluminum Alloys for Automotive Engine Applications (ADAPA). Office of Scientific and Technical Information (OSTI), November 2018. http://dx.doi.org/10.2172/1494555.
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Niezgoda, Stephen, Pengyang Zhao, and Yunzhi Wang. ICME for Creep of Ni-Base Superalloys in Advanced Ultra-Supercritical Steam Turbines. Office of Scientific and Technical Information (OSTI), January 2020. http://dx.doi.org/10.2172/1601245.
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Velinov, Peter I. Y., Yordan Tassev, and Dimitrinka Tomova. Study of Unpredicted First Geomagnetic Storm of 2020, Due to Interaction of ICME with Near-earth Space on Аpril 20. "Prof. Marin Drinov" Publishing House of Bulgarian Academy of Sciences, November 2020. http://dx.doi.org/10.7546/crabs.2020.11.12.
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Arsenlis, Athanasios, and John Allison. Integrated Computational Materials Engineering (ICME) Tools for Optimizing Strength of Forged Al-Li Turbine Blades for Aircraft Engines Final Report CRADA No. TC02238.0. Office of Scientific and Technical Information (OSTI), September 2017. http://dx.doi.org/10.2172/1425447.
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Arsenlis, A., and J. Allison. Integrated Computational Materials Engineering (ICME) Tools for Optimizing Strength of Forged Al-Li Turbine Blades for Aircraft Engines Final Report CRADA No. TC02238.0. Office of Scientific and Technical Information (OSTI), March 2021. http://dx.doi.org/10.2172/1774219.
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