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1

Ji, Jinzhu, James W. Head, and Jianzhong Liu. "Pre-Orientale Southwest Peak-Ring Basin: Gravity Structure, Geologic Characteristics, and Influence on Orientale Basin Ring Formation and Ejecta Emplacement." Remote Sensing 13, no. 13 (2021): 2635. http://dx.doi.org/10.3390/rs13132635.

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The Orientale impact basin is the youngest and most well-preserved of the lunar multi-ring basins. The generally well-preserved ring structures and basin facies are distinctly anomalous in the southwestern quadrant; the outer Cordillera ring extends significantly outward, the Outer and Inner Rook mountain rings are more poorly developed and show anomalous characteristics, and the Montes Rook Formation varies widely from its characteristics elsewhere in the basin interior. Based on the gravity, image, and topography data, we confirmed that the southwest region of the Orientale basin represents
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2

Lin, Honglei, Zhiping He, Wei Yang, et al. "Olivine-norite rock detected by the lunar rover Yutu-2 likely crystallized from the SPA-impact melt pool." National Science Review 7, no. 5 (2019): 913–20. http://dx.doi.org/10.1093/nsr/nwz183.

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Abstract Chang’E-4 landed in the South Pole-Aitken (SPA) basin, providing a unique chance to probe the composition of the lunar interior. Its landing site is located on ejecta strips in Von Kármán crater that possibly originate from the neighboring Finsen crater. A surface rock and the lunar regolith at 10 sites along the rover Yutu-2 track were measured by the onboard Visible and Near-Infrared Imaging Spectrometer in the first three lunar days of mission operations. In situ spectra of the regolith have peak band positions at 1 and 2 μm, similar to the spectral data of Finsen ejecta from the M
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3

Gorter, J. D. "THE PETROLEUM POTENTIAL OF AUSTRALIAN PHANEROZOIC IMPACT STRUCTURES." APPEA Journal 38, no. 1 (1998): 159. http://dx.doi.org/10.1071/aj97009.

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This paper examines proven, probable, possible and speculative impact structures in Australian Phanerozoic strata and their petroleum potential. There are two classes of crater: simple and complex. The former usually assumes a bowl shaped depression with a raised and overturned rim with a diameter rarely more than three kilometres, with complex structures generally occurring above diameters of two kilometres in sedimentary rocks and four kilometres in crystalline rocks. Complex craters are characterised by a central uplifted area and a classic 'sombrero' structure and can be very large and hav
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4

Zhu, Meng‐Hua, Kai Wünnemann, and Natalia Artemieva. "Effects of Moon's Thermal State on the Impact Basin Ejecta Distribution." Geophysical Research Letters 44, no. 22 (2017): 11,292–11,300. http://dx.doi.org/10.1002/2017gl075405.

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5

Buchner, Elmar, and Martin Schmieder. "The Steinheim Basin impact crater (SW-Germany) – Where are the ejecta?" Icarus 250 (April 2015): 529–43. http://dx.doi.org/10.1016/j.icarus.2014.12.026.

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6

Wada, K., K. Ishibashi, H. Kimura, et al. "Size of particles ejected from an artificial impact crater on asteroid 162173 Ryugu." Astronomy & Astrophysics 647 (March 2021): A43. http://dx.doi.org/10.1051/0004-6361/202039777.

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A projectile accelerated by the Hayabusa2 Small Carry-on Impactor successfully produced an artificial impact crater with a final apparent diameter of 14.5 ± 0.8 m on the surface of the near-Earth asteroid 162173 Ryugu on April 5, 2019. At the time of cratering, Deployable Camera 3 took clear time-lapse images of the ejecta curtain, an assemblage of ejected particles forming a curtain-like structure emerging from the crater. Focusing on the optical depth of the ejecta curtain and comparing it with a theoretical model, we infer the size of the ejecta particles. As a result, the typical size of t
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7

Yue, Zongyu, Meiping Yang, Mengna Jia, et al. "Refined model age for Orientale Basin derived from zonal crater dating of its ejecta." Icarus 346 (August 2020): 113804. http://dx.doi.org/10.1016/j.icarus.2020.113804.

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8

Premovic, Pavle, Nikola Nikolic, Mirjana Pavlovic, and Katja Panov. "Geochemistry of the cretaceous-tertiary transition boundary at Blake Nose (N. W. Atlantic): Cosmogenic Ni." Journal of the Serbian Chemical Society 69, no. 3 (2004): 205–23. http://dx.doi.org/10.2298/jsc0403205p.

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The Cretaceous-Tertiary (KT) boundary transition at the Blake Nose Plateau recovered by ODP Leg 171B (site 1049, hole A, core 17X, section 2) contains an ejecta bed (thickness ca. 17 cm) marking a late Cretaceous asteroid impact. The nature and geochemical composition of this bed imply that it originated mainly from the target rocks of the Chicxulub impact site (Yucatan Peninsula, Mexico), the site of the presumed asteroid impact. The ejecta bed of hole 1049A contains relatively high concentrations of Ni (up to 165 ppm) within the carbonate fraction. It is reasoned that this enhancement repres
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9

Dessart, L., D. J. Hillier, and K. D. Wilk. "Impact of clumping on core-collapse supernova radiation." Astronomy & Astrophysics 619 (October 30, 2018): A30. http://dx.doi.org/10.1051/0004-6361/201833278.

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There is both observational and theoretical evidence that the ejecta of core-collapse supernovae (SNe) are structured. Rather than being smooth and homogeneous, the material is made of over-dense and under-dense regions of distinct composition. Here, we have explored the effect of clumping on the SN radiation during the photospheric phase using 1D non-local thermodynamic equilibrium radiative transfer and an ejecta model arising from a blue-supergiant explosion (yielding a Type II-peculiar SN). Neglecting chemical segregation, we adopted a velocity-dependent volume-filling factor approach that
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10

Nozaki, Kenta, Masahiro Nishida, Koichi Hayashi, and Sunao Hasegawa. "Ejecta Size Distribution Resulting from Hypervelocity Impacts between Aluminum Alloys." Applied Mechanics and Materials 566 (June 2014): 338–43. http://dx.doi.org/10.4028/www.scientific.net/amm.566.338.

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We investigated the effects of impact velocity on ejecta size when aluminum alloy 2017-T4 spheres with a diameter of 3.2 mm impacted aluminum alloy 6061-T6 targets with a thickness of 30 mm at velocities of 2 to 7 km/s. We used a two-stage light-gas gun at the Institute of Space and Astronautical Science (ISAS)/Japan Aerospace Exploration Agency (JAXA). To examine the scattering angles of the ejecta, the following was placed 50 mm in front of the target: a witness plate (150 mm × 150 mm, 2 mm in thickness) made of copper with a hole of 30 mm. The ejection behaviors of fragments were observed u
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11

Wallace, M. W., V. A. Gostin, and R. R. Keays. "Geological Note: Discovery of the acraman impact ejecta blanket in the officer basin and its stratigraphic significance." Australian Journal of Earth Sciences 36, no. 4 (1989): 585–87. http://dx.doi.org/10.1080/08120098908729511.

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12

Zain, P. S., R. P. Di Sisto, and G. C. de Elía. "Impacts on Ceres and Vesta: Source regions, cratering, and fragmentation." Astronomy & Astrophysics 652 (August 2021): A122. http://dx.doi.org/10.1051/0004-6361/202039373.

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Context. Ceres and Vesta are the largest members of the main belt (MB). They were visited by the NASA Dawn spacecraft between 2011 and 2018, which provided a great sample of detailed observations of the surface of both bodies. Aims. We perform a study on the impacts on Ceres and Vesta. We aim to determine the size-frequency distribution (SFD) of impactors and to identify and quantify the contribution of each source region, as well as the craters produced and fragments ejected in these impact events. Methods. We used a multipart collisional evolution model of the MB called ACDC (Asteroid Collis
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13

Inceli, Ozge. "The Perceptions of English Teachers to the SIOP® Model and Its Impact on Limited English Proficiency." Journal of Ethnic and Cultural Studies 2, no. 1 (2015): 15. http://dx.doi.org/10.29333/ejecs/13.

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Limited English proficiency is the difficulty in comprehension and production in English. In this study, the efficiency of the Sheltered Instruction Observation Protocol (SIOP) Model was examined to indicate the components that are lesson preparation, building background, comprehensible input, strategies, interaction, practice and application, lesson delivery, review and assessment. The basic purpose of the research was to investigate how teachers improve the student’s language performance for limited English proficiency through using the SIOP® Model. In this paper, a qualitative research appr
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14

Li, L., Z. Yue, C. Zhang, and D. Li. "REMOTE SENSING OBSERVATIONS AND NUMERICAL SIMULATION FOR MARTIAN LAYERED EJECTA CRATERS." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLII-3 (April 30, 2018): 865–70. http://dx.doi.org/10.5194/isprs-archives-xlii-3-865-2018.

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To understand past Martian climates, it is important to know the distribution and nature of water ice on Mars. Impact craters are widely used ubiquitous indicators for the presence of subsurface water or ice on Mars. Remote sensing observations and numerical simulation are powerful tools for investigating morphological and topographic features on planetary surfaces, and we can use the morphology of layered ejecta craters and hydrocode modeling to constrain possible layering and impact environments. The approach of this work consists of three stages:Firstly, the morphological characteristics of
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15

Hassler, Scott W., Bruce M. Simonson, Dawn Y. Sumner, and Louis Bodin. "Paraburdoo spherule layer (Hamersley Basin, Western Australia): Distal ejecta from a fourth large impact near the Archean-Proterozoic boundary." Geology 39, no. 4 (2011): 307–10. http://dx.doi.org/10.1130/g31526.1.

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16

Kyte, Frank T., and Jennifer A. Bostwick. "Magnesioferrite spinel in Cretaceous/Tertiary boundary sediments of the Pacific basin: Remnants of hot, early ejecta from the Chicxulub impact?" Earth and Planetary Science Letters 132, no. 1-4 (1995): 113–27. http://dx.doi.org/10.1016/0012-821x(95)00051-d.

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17

Bulla, M. "possis: predicting spectra, light curves, and polarization for multidimensional models of supernovae and kilonovae." Monthly Notices of the Royal Astronomical Society 489, no. 4 (2019): 5037–45. http://dx.doi.org/10.1093/mnras/stz2495.

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ABSTRACT We present possis, a time-dependent three-dimensional Monte Carlo code for modelling radiation transport in supernovae and kilonovae. The code incorporates wavelength- and time-dependent opacities, and predicts viewing-angle dependent spectra, light curves, and polarization for both idealized and hydrodynamical explosion models. We apply the code to a kilonova model with two distinct ejecta components, one including lanthanide elements with relatively high opacities and the other devoid of lanthanides and characterized by lower opacities. We find that a model with total ejecta mass $M
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18

SCHULTE, PETER, JAN SMIT, ALEXANDER DEUTSCH, TOBIAS SALGE, ANDREA FRIESE, and KILIAN BEICHEL. "Tsunami backwash deposits with Chicxulub impact ejecta and dinosaur remains from the Cretaceous-Palaeogene boundary in the La Popa Basin, Mexico." Sedimentology 59, no. 3 (2011): 737–65. http://dx.doi.org/10.1111/j.1365-3091.2011.01274.x.

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19

Premovic, Pavle, Milena Krsmanovic, Bratislav Todorovic, Mirjana Pavlovic, Nikola Nikolic, and Dragan Djordjevic. "Geochemistry of the cretaceous-tertiary boundary (Fish Clay) at Stevns Klint (Denmark): Ir, Ni and Zn in kerogen." Journal of the Serbian Chemical Society 71, no. 7 (2006): 793–806. http://dx.doi.org/10.2298/jsc0607793p.

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Geochemical analyses of trace metals (Ir, Ni and Zn) in the kerogen of the black marl of the Cretaceous-Tertiary boundary succession (Fish Clay) at Stevns Klint (H?jerup Church) were undertaken. The data for this kerogen were in accordance with a previous hypothesis that this (insoluble) geoorganic polymer was derived from humic substances (mainly humic acids) of a nearshore soil. Substantial proportions of Ir, Ni and Zn within the kerogen structure were probably contained in these substances arriving at the sedimentary site. It is proposed that these humics were probably transported by acid s
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20

Mercer, Cameron M., Kelsey E. Young, John R. Weirich, et al. "Refining lunar impact chronology through high spatial resolution 40Ar/39Ar dating of impact melts." Science Advances 1, no. 1 (2015): e1400050. http://dx.doi.org/10.1126/sciadv.1400050.

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Quantitative constraints on the ages of melt-forming impact events on the Moon are based primarily on isotope geochronology of returned samples. However, interpreting the results of such studies can often be difficult because the provenance region of any sample returned from the lunar surface may have experienced multiple impact events over the course of billions of years of bombardment. We illustrate this problem with new laser microprobe 40Ar/39Ar data for two Apollo 17 impact melt breccias. Whereas one sample yields a straightforward result, indicating a single melt-forming event at ca. 3.8
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21

Mayer, Hans C., and Rouslan Krechetnikov. "Flat plate impact on water." Journal of Fluid Mechanics 850 (July 12, 2018): 1066–116. http://dx.doi.org/10.1017/jfm.2018.461.

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While the classical problem of a flat plate impact on a water surface at zero dead-rise angle has been studied for a long time both theoretically and experimentally, it still presents a number of challenges and unsolved questions. Hitherto, the details of the flow field – especially at early times and close to the plate edge, where the classical inviscid theory predicts a singularity in the velocity field and thus in the free surface deflection, so-called ejecta – have not been studied experimentally, which led to mutually contradicting suppositions in the literature. On one hand, it motivated
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22

Ricardo, Nomensen, Hendra Amijaya, and Salahuddin Husein. "Basin Evolution Palispatic Model of Bonaparte Basin, Australia Northwest Shelf." Journal of Applied Geology 2, no. 2 (2018): 83. http://dx.doi.org/10.22146/jag.39988.

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This research area is located on the Australian NW Shelf close to the westernedge of the Sahul Platform. This research is aimed to generate the palispatic basin model of Bonaparte Basin, Australian Northwest Shelf. It is to predict the impact of Neogene collision on the petroleum system distribution on Australian Northwest Shelf. The main data used in this research are seismic data using qualitative method analysis. The well data is used to well-seismic tied. After data acquisition, the seismic data are interpreted based on the horizon and structure interpretation. These interpretation are to
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23

Figueira, Joana, Jordi José, Enrique García-Berro, Simon W. Campbell, Domingo García-Senz, and Shazrene Mohamed. "Three-dimensional simulations of the interaction between the nova ejecta, accretion disk, and companion star." Astronomy & Astrophysics 613 (May 2018): A8. http://dx.doi.org/10.1051/0004-6361/201731545.

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Context. Classical novae are thermonuclear explosions hosted by accreting white dwarfs in stellar binary systems. Material piles up on top of the white dwarf star under mildly degenerate conditions, driving a thermonuclear runaway. The energy released by the suite of nuclear processes operating at the envelope, mostly proton-capture reactions and β+-decays, heats the material up to peak temperatures ranging from 100 to 400 MK. In these events, about 10−3–10−7 M⊙, enriched in CNO and, sometimes, other intermediate-mass elements (e.g., Ne, Na, Mg, and Al) are ejected into the interstellar medium
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24

Desai, D., B. D. Metzger, and F. Foucart. "Imprints of r-process heating on fall-back accretion: distinguishing black hole–neutron star from double neutron star mergers." Monthly Notices of the Royal Astronomical Society 485, no. 3 (2019): 4404–12. http://dx.doi.org/10.1093/mnras/stz644.

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ABSTRACT Mergers of compact binaries containing two neutron stars (NS–NS), or a neutron star and a stellar mass black hole (NS–BH), are likely progenitors of short-duration gamma-ray bursts (SGRBs). A fraction ${\gtrsim } 20{{\ \rm per\ cent}}$ of SGRBs is followed by temporally extended (≳minute-long), variable X-ray emission, attributed to ongoing activity of the central engine. One source of late-time engine activity is fall-back accretion of bound tidal ejecta; however, observed extended emission light curves do not track the naively anticipated, uninterrupted t−5/3 power-law decay, instea
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25

Hernandez Pardo, Orlando. "Vichada meteorite impact effects from simulation of regional environmental consequences of a meteoroid impact on Earth." Earth Sciences Research Journal 22, no. 1 (2018): 7–12. http://dx.doi.org/10.15446/esrj.v22n1.65459.

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This study estimates the regional environmental consequences of the impactor extraterrestrial body that could produce the probable Vichada impact crater structure on the Vichada Plain, in Colombia, South America. This paper details the parameter assumptions upon which the estimation is made. It describes an approach to quantifying the principal impact processes that could have affected the landscape in the vicinity of the probable Vichada impact event in the past. The key parameters are impactor diameter, impactor density, impact velocity before atmospheric entry, impact angle, and the distanc
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26

Heinzel, J., M. W. Coughlin, T. Dietrich, et al. "Comparing inclination-dependent analyses of kilonova transients." Monthly Notices of the Royal Astronomical Society 502, no. 2 (2021): 3057–65. http://dx.doi.org/10.1093/mnras/stab221.

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ABSTRACT The detection of the optical transient AT2017gfo proved that binary neutron star mergers are progenitors of kilonovae (KNe). Using a combination of numerical-relativity and radiative-transfer simulations, the community has developed sophisticated models for these transients for a wide portion of the expected parameter space. Using these simulations and surrogate models made from them, it has been possible to perform Bayesian inference of the observed signals to infer properties of the ejected matter. It has been pointed out that combining inclination constraints derived from the KN wi
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27

Thuillet, Florian, Patrick Michel, Shogo Tachibana, Ronald-L. Ballouz, and Stephen R. Schwartz. "Numerical modelling of medium-speed impacts on a granular surface in a low-gravity environment application to Hayabusa2 sampling mechanism." Monthly Notices of the Royal Astronomical Society 491, no. 1 (2019): 153–77. http://dx.doi.org/10.1093/mnras/stz3010.

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ABSTRACT Even if craters are very common on Solar System body surfaces, crater formation in granular media such as the ones covering most of visited asteroids still needs to be better understood, above all in low-gravity environments. JAXA’s sample return mission Hayabusa2, currently visiting asteroid (162173) Ryugu, is a perfect opportunity for studying medium-speed impacts into granular matter, since its sampling mechanism partly consists of a 300 m s−1 impact. In this paper, we look at medium-speed impacts, from 50 to 300 m s−1, into a granular material bed, to better understand crater form
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28

Joy, K. H., J. F. Snape, A. A. Nemchin, et al. "Timing of geological events in the lunar highlands recorded in shocked zircon-bearing clasts from Apollo 16." Royal Society Open Science 7, no. 6 (2020): 200236. http://dx.doi.org/10.1098/rsos.200236.

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Apollo 16 soil-like regolith breccia 65745,7 contains two zircon-bearing clasts. One of these clasts is a thermally annealed silica-rich rock, which mineralogically has affinities with the High Alkali Suite (Clast 1), and yields zircon dates ranging from 4.08 to 3.38 Ga. The other clast is a KREEP-rich impact melt breccia (Clast 2) and yields zircon dates ranging from 3.97 to 3.91 Ga. The crystalline cores of both grains, which yield dates of ca 3.9 Ga, have undergone shock pressure modification at less than 20 GPa. We interpret that the U-Pb chronometer in these zircon grains has been partial
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29

Pan, Li, Xudong Chen, Lu Zhao, and Anran Xiao. "Does Information Asymmetry Impact Sub-Regions’ Cooperation of Regional Water Resource Allocation?" International Journal of Environmental Research and Public Health 16, no. 21 (2019): 4292. http://dx.doi.org/10.3390/ijerph16214292.

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Water resources allocation is an urgent problem for basin authorities. In order to obtain greater economic benefits from limited water supplies, sub-regions must cooperate with each other. To study the influence of cooperation among sub-regions and the symmetry of cooperation information on the interests of the basin authority and each sub-region, this study proposes a regional water allocation model in three different situations: (1) non-cooperation; (2) cooperation and information symmetry; (3) cooperation and information asymmetry. The proposed model clearly reflects the Stackelberg game re
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30

Dessart, Luc, and D. John Hillier. "Radiative-transfer modeling of nebular-phase type II supernovae." Astronomy & Astrophysics 642 (October 2020): A33. http://dx.doi.org/10.1051/0004-6361/202038148.

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Nebular phase spectra of core-collapse supernovae (SNe) provide critical and unique information on the progenitor massive star and its explosion. We present a set of one-dimensional steady-state non-local thermodynamic equilibrium radiative transfer calculations of type II SNe at 300 d after explosion. Guided by the results obtained from a large set of stellar evolution simulations, we craft ejecta models for type II SNe from the explosion of a 12, 15, 20, and 25 M⊙ star. The ejecta density structure and kinetic energy, the 56Ni mass, and the level of chemical mixing are parametrized. Our mode
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31

Young, James A., and William S. Longland. "Impact of Alien Plants on Grant Basin Rangelands." Weed Technology 10, no. 2 (1996): 384–91. http://dx.doi.org/10.1017/s0890037x00040136.

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Our purpose is to discuss the impact of alien plants on rangeland ecosystems of the Great Basin in terms of their effects on biological functions. The sagebrush/bunchgrass ranges of western North America are used as a model ecosystem for the impact of alien plants. Alien weed species have been introduced in successive waves, with the success of each new introduction dependent on how well adapted to the environment and how competitive the new weed is with those previously introduced. Annual species have been successful across extensive areas of Great Basin rangelands. Biennial and short- and lo
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Guo, ShengLian, Jing Guo, Jun Zhang, and Hua Chen. "VIC distributed hydrological model to predict climate change impact in the Hanjiang basin." Science in China Series E: Technological Sciences 52, no. 11 (2009): 3234–39. http://dx.doi.org/10.1007/s11431-009-0355-2.

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Kuo, Chun-Chao, Thian Yew Gan, and Jingwen Wang. "Climate change impact to Mackenzie river Basin projected by a regional climate model." Climate Dynamics 54, no. 7-8 (2020): 3561–81. http://dx.doi.org/10.1007/s00382-020-05177-7.

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34

Crawford, David A. "Models of fragment penetration and fireball evolution." International Astronomical Union Colloquium 156 (May 1996): 133–56. http://dx.doi.org/10.1017/s0252921100115490.

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A new analytical model that is calibrated against numerical simulations performed with the CTH shock physics code provides a useful description of the entry of Periodic Comet Shoemaker-Levy 9 into the Jovian atmosphere. Mass loss due to radiative heating of fragments larger than 100 m in diameter is insignificant because of energy conservation during the ablative process. Nevertheless, radiative ablation is a major contributor to atmospheric energy deposition at high altitude and plays an important role in early-time fireball evolution. The analytical model provides the initial conditions from
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35

Glikson, Andrew, and Charlotte Allen. "Iridium anomalies and fractionated siderophile element patterns in impact ejecta, Brockman Iron Formation, Hamersley Basin, Western Australia: evidence for a major asteroid impact in simatic crustal regions of the early Proterozoic earth." Earth and Planetary Science Letters 220, no. 3-4 (2004): 247–64. http://dx.doi.org/10.1016/s0012-821x(04)00062-7.

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36

Xue, Feng, Peng Shi, Simin Qu, Jianjin Wang, and Yanming Zhou. "Evaluating the impact of spatial variability of precipitation on streamflow simulation using a SWAT model." Water Policy 21, no. 1 (2018): 178–96. http://dx.doi.org/10.2166/wp.2018.118.

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Abstract The spatial variability of precipitation is often considered to be a major source of uncertainty for hydrological models. The widely used Soil and Water Assessment Tool (SWAT) is insufficient to calculate a sub-basin's mean areal precipitation (MAP) since it only uses data from the rainfall station nearest to the centroid of each sub-basin. Therefore, Inverse Distance Weighting (IDW), Thiessen Polygons (TP) and Ordinary Kriging (OK) were applied as alternative interpolation methods in this study to calculate sub-basin MAP. The MAP results from the four methods used for the Xixian Basi
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Gao, Yuqin, Yu Yuan, Huaizhi Wang, Zhenxing Zhang, and Liu Ye. "Analysis of impacts of polders on flood processes in Qinhuai River Basin, China, using the HEC-RAS model." Water Supply 18, no. 5 (2018): 1852–60. http://dx.doi.org/10.2166/ws.2018.008.

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Abstract Flood control with polders is prevalent in East China. Their impact on flood processes is critically important for flood control, but has not been well documented. The Qinhuai River Basin was selected as the study area. A Hydrologic Engineering Center – River Analysis System (HEC-RAS) hydraulic model was developed to simulate and predict storm flood processes and the associated impact of polders. The study shows that the HEC-RAS model is capable of simulating the impact of polders on flood processes in the Qinhuai River Basin. The polders increased the water level outside of the polde
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Yu, Yang, Patrick Michel, Stephen R. Schwartz, Shantanu P. Naidu, and Lance A. M. Benner. "Ejecta cloud from the AIDA space project kinetic impact on the secondary of a binary asteroid: I. mechanical environment and dynamical model." Icarus 282 (January 2017): 313–25. http://dx.doi.org/10.1016/j.icarus.2016.09.008.

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39

Walker, James D., Sidney Chocron, and Donald J. Grosch. "Size scaling of hypervelocity-impact ejecta mass and momentum enhancement: Experiments and a nonlocal-shear-band-motivated strain-rate-dependent failure model." International Journal of Impact Engineering 135 (January 2020): 103388. http://dx.doi.org/10.1016/j.ijimpeng.2019.103388.

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Lyra, Barbara Ucelis, and Daniel Rigo. "Deforestation impact on discharge regime in the Doce River Basin." Ambiente e Agua - An Interdisciplinary Journal of Applied Science 14, no. 4 (2019): 1. http://dx.doi.org/10.4136/ambi-agua.2370.

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The construction of scenarios using hydrological models can evaluate the hydrological response in watersheds, due to changes in the soil use. In this context, this study analyzed the consequences of deforestation in the hydrological behavior of the Doce River Basin, which has a drainage area of approximately 86.715 km². The basin presents problems regarding water availability, floods, indiscriminate deforestation and inadequate soil management. The Model of Large Basins (MGB-IPH) was selected, using daily data from 1990 to 2014, 11 fluviometric, 81 rainfall and 12 meteorological stations, nume
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Carnahan, Evan, Jason M. Amundson, and Eran Hood. "Impact of glacier loss and vegetation succession on annual basin runoff." Hydrology and Earth System Sciences 23, no. 3 (2019): 1667–81. http://dx.doi.org/10.5194/hess-23-1667-2019.

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Abstract. We use a simplified glacier-landscape model to investigate the degree to which basin topography, climate regime, and vegetation succession impact centennial variations in basin runoff during glacier retreat. In all simulations, annual basin runoff initially increases as water is released from glacier storage but ultimately decreases to below preretreat levels due to increases in evapotranspiration and decreases in orographic precipitation. We characterize the long-term (> 200 years) annual basin runoff curves with four metrics: the magnitude and timing of peak basin runoff, the ti
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Hogg, Charlie A. R., Stuart B. Dalziel, Herbert E. Huppert, and Jörg Imberger. "Inclined gravity currents filling basins: the impact of peeling detrainment on transport and vertical structure." Journal of Fluid Mechanics 820 (May 5, 2017): 400–423. http://dx.doi.org/10.1017/jfm.2017.196.

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Transport of dense fluid by an inclined gravity current can control the vertical density structure of the receiving basin in many natural and industrial settings. A case familiar to many is a lake fed by river water that is dense relative to the lake water. In laboratory experiments, we pulsed dye into the basin inflow to visualise the transport pathway of the inflow fluid through the basin. We also measured the evolving density profile as the basin filled. The experiments confirmed previous observations that when the turbulent gravity current travelled through ambient fluid of uniform density
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Shi, Yu Zhi, Hai Jiao Liu, Ming Yuan Fan, and Ji Wen Huang. "Quantifying Impact of Climate Change on Watershed Hydrologic Cycle Based on Multi-GCM Model." Advanced Materials Research 726-731 (August 2013): 3451–56. http://dx.doi.org/10.4028/www.scientific.net/amr.726-731.3451.

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Single climate model has much uncertainty on quantifying climate change, this paper proposes a new method, reliability ensemble averaging based on Bayesian weighted average (REA-BMA) to calculate the comprehensive climate change and then combines large-scale distributed watershed hydrologic cycling model SWAT to quantifying the effect of future climate change on basin water resources. The data sets from 1961 to 2040 of GCM models (HadCM3, CGCM3, BCCR, CSIRO) and three emission scenarios (A2, A1B and B2) are taking for uncertainty analysis and Huntai River basin in China is selected as study ca
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Bui, Quy Ngoc, Nga Thi Le, Quan Anh Duong, and Anh Mai Thi Tran. "Asessment of flood risk on human in downstream of Vu Gia - Thu Bon river basin by combining GIS and hydraulic model." Journal of Mining and Earth Sciences 61, no. 4 (2020): 46–56. http://dx.doi.org/10.46326/jmes.2020.61(4).05.

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Flooding is a natural disaster that occurs in most parts of Vietnam, causing a lot of damage to people, assets and influence on socio-economic activities. This article analyzes the impact of floods on population in the Vu Gia – Thu basin. In this study, the authors used the result of the hydrolic modeling, the simulated floods in conjunction with the use of GIS software (ArcGIS) to analyze the impact on the population of downstream the Vu Gia – Thu Bon river basin. From there, the study indicated the impact and influence of floods caused on flooded areas in the river basin. The ArcGIS software
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Malamakal, Tom, L. W. Antony Chen, Xiaoliang Wang, et al. "Prescribed burn smoke impact in the Lake Tahoe Basin: model simulation and field verification." International Journal of Environment and Pollution 52, no. 3/4 (2013): 225. http://dx.doi.org/10.1504/ijep.2013.058457.

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Meng-Hua, Zhu, Liu Liang-Gang, and Xu Ao-Ao. "An Impact Model of the Imbrium Basin for Distribution of Thorium on Lunar Surface." Chinese Physics Letters 25, no. 12 (2008): 4490–92. http://dx.doi.org/10.1088/0256-307x/25/12/086.

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Joseph, John F., Hatim O. Sharif, Jeffrey G. Arnold, and David D. Bosch. "The Impact of Asynchronicity on Event-Flow Estimation in Basin-Scale Hydrologic Model Calibration1." JAWRA Journal of the American Water Resources Association 49, no. 2 (2012): 300–318. http://dx.doi.org/10.1111/jawr.12011.

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Yates, David N. "WatBal: An Integrated Water Balance Model for Climate Impact Assessment of River Basin Runoff." International Journal of Water Resources Development 12, no. 2 (1996): 121–40. http://dx.doi.org/10.1080/07900629650041902.

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Zahabiyoun, B., M. R. Goodarzi, A. R. Massah Bavani, and H. M. Azamathulla. "Assessment of Climate Change Impact on the Gharesou River Basin Using SWAT Hydrological Model." CLEAN - Soil, Air, Water 41, no. 6 (2013): 601–9. http://dx.doi.org/10.1002/clen.201100652.

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Ogbu, Kingsley Nnaemeka, Emeka L. Ndulue, Isiguzo Edwin Ahaneku, and Ikenna Joseph Ubah. "Evaluation of the Impact of Climate Change on Streamflow Using SWAT Model." ASM Science Journal 13 (June 24, 2020): 1–8. http://dx.doi.org/10.32802/asmscj.2020.494.

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The Soil and Water Assessment Tool (SWAT) model was applied in this study to simulate stream-flow in the Oyun River Basin. The model was calibrated and validated using monthly stream-flow data for the basin. Model performance was satisfactory for calibration and validation with a coefficient of determination (R2) of 0.69 and 0.88, respectively. Climate change impact on Oyun River was assessed by driving the SWAT model with climate parameters obtained from two global climate models (HadGEM2-ES and BCC-CCSM1-1M) based on RCP 2.6 for 2050 – 2059 and 2080 – 2089 periods. With respect to a baseline
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