Now showing items 941-960 of 7550

    • Lecaros, R.; López Ríos, J.; Ortega Palma, Jaime; Zamorano, S. (IOP, 2020)
      In this article we deal with a class of geometric inverse problem for bottom detection by one single measurement on the free surface in water-waves. We found upper and lower bounds for the size of the region enclosed between ...
    • Lanas, Fernando J.; Martínez Conde, Francisco J.; Alvarado, Diego; Moreno Vieyra, Rodrigo; Mendoza Araya, Patricio; Jiménez Estévez, Guillermo (MDPI, 2020)
      Microgrids have the potential to provide security and flexibility to power systems through the integration of a wide range of resources, including distributed energy storage, usually in the form of batteries. An aggregation ...
    • Marian, Max; Bartz, Marcel; Wartzack, Sandro; Rosenkranz, Andreas (MDPI, 2020)
      Apart from complex numerical models to predict the tribological behavior of elastohydrodynamically lubricated contacts, non-dimensional similarity groups and analytically solvable proximity equations can be used to estimate ...
    • Clerc Gavilán, Marcel; Coullet, Pierre; Rojas, Rene G.; Tlidi, Mustapha (American Institute of Physics, 2020)
      This Focus Issue on instabilities and nonequilibrium structures includes invited contributions from leading researchers across many different fields. The issue was inspired in part by the “VII Instabilities and Nonequilibrium ...
    • Ávalos, Sebastián; Kracht Gajardo, Willy; Ortiz, Julian (MDPI, 2020)
      Ore hardness plays a critical role in comminution circuits. Ore hardness is usually characterized at sample support in order to populate geometallurgical block models. However, the required attributes are not always available ...
    • Padmapriya, D.; Dhayanithi, D.; Rashid, A.; Rahul, M. T.; Kalarikkal, N.; Muneeswaran, M.; Giridharan, NV (Indian Acad Sciences, 2020)
      Multiferroic composite with the general formula (1 - x)BaTiO3-xCoFe(2)O(4)(x= 0.05, 0.15, 0.25, 0.35 and 0.45) has been synthesized by a standard solid-state reaction route. Powder X-ray diffraction analysis confirms the ...
    • Schultheis, M.; Rojas Arriagada, A.; Cunha, K.; Zoccali, M.; Chiappini, C.; Zasowski, G.; Queiroz, A. B. A.; Minniti, D.; Fritz, T.; García Hernández, D. A.; Nitschelm, C.; Zamora, O.; Hasselquist, S.; Fernández-Trincado, J. G.; Muñoz, R. R. (EDP Sciences, 2020)
      The Galactic center region, including the nuclear disk, has until recently been largely avoided in chemical census studies because of extreme extinction and stellar crowding. Large, near-IR spectroscopic surveys, such as ...
    • Marín, Carolina; Rodríguez, Inés; Godoy, Benigno; González Maurel, Osvaldo; Le Roux, Petrus; Medina, Eduardo; Bertin, Daniel (Springer, 2020)
      New stratigraphic, lithological and petrographic analyses of La Poruna scoria cone (21 degrees 53 ' S-68 degrees 30 ' W, Central Andes, northern Chile) allow the reconstruction of the eruptive sequence of this monogenetic ...
    • Anderson, L. D.; Sormani, M. C.; Ginsburg, Adam; Glover, Simon C.O.; Heywood, I.; Rammala, I.; Schuller, F.; Csengeri, T.; Urquhart, J. S.; Bronfman Aguiló, Leonardo (IOP Publishing, 2020)
      Sgr.E is a massive star formation complex found toward the Galactic center that consists of numerous discrete, compact H II regions. It is located at the intersection between the central molecular zone (CMZ) and the far ...
    • Correa, Isabel C.; Arias, Paola A.; Rojas, Maisa (Wiley, 2021)
      In this article, multiple methods for estimating the onset and demise of the South American Monsoon System (SAMS) are evaluated during the period 1979-2018. The results obtained from indices based on precipitation, outgoing ...
    • Guglielmo, V.; Saglia, R.; Castander, F. J.; Galametz, A.; Paltani, S.; Bender, R.; Bolzonella, M.; Capak, P.; Ilbert, O.; Masters, D.C.; Stern, D.; Andreon, S.; Auricchio, N.; Balaguera-Antolinez, A.; Baldi, M.; Bardelli, S.; Biviano, A.; Bodendorf, C.; Bonino, D.; Bozzo, E.; Branchini, E.; Brau Nogue, S.; Brescia, M.; Burigana, C.; Cabanac, R.A.; Camera, S.; Capobianco, V.; Cappi, A.; Carbone, C.; Carretero, J.; Carvalho, C.S; Casas, R.; Casas, S.; Castellano, M.; Castignani, G.; Cavuoti, S.; Cimatti, A.; Cledassou, R.; Colodro Conde, C.; Congedo, G.; Conselice, C.J.; Conversi, L.; Copin, Y.; Corcione, L.; Costille, A.; Coupon, J.; Courtois, H. M.; Cropper, M.; Da Silva, A.; De la Torre, S.; Di Ferdinando, D.; Dubath, F.; Duncan, C. A. J.; Dupac, X.; Dusini, S.; Fabricius, M.; Farrens, S.; Ferreira, P. G.; Fotopoulou, S.; Frailis, M.; Franceschi, E.; Fumana, M.; Galeotta, S.; Garilli, B.; Gillis, B.; Giocoli, C.; Gozaliasl, G.; Gracia Carpio, J.; Grupp, F.; Guzzo, L.; Hildebrandt, H.; Hoekstra, H.; Hormuth, F.; Israel, H.; Jahnke, K.; Keihanen, E.; Kermiche, S.; Kilbinger, M.; Kirkpatrick, C. C.; Kitching, T.; Kubik, B.; Kunz, M.; Kurki-Suonio, H.; Laureijs, R.; Ligori, S.; Lilje, P. B.; Lloro, I.; Maino, D.; Maiorano, E.; Maraston, C.; Marggraf, O.; Martinet, N.; Marulli, F.; Massey, R.; Maurogordato, S.; Medinaceli, E.; Mei, S.; Meneghetti, M.; Metcalf, R. Benton; Meylan, G.; Moresco, M.; Moscardini, L.; Munari, E.; Nakajima, R.; Neissner, C.; Niemi, S.; Nucita, A.A.; Padilla, C.; Pasian, F.; Patrizii, L.; Pocino, A.; Poncet, M.; Pozzetti, L.; Raison, F.; Renzi, A.; Rhodes, J.; Riccio, G.; Romelli, E.; Roncarelli, M.; Rossetti, E.; Sanchez, A. G.; Sapone, D.; Schneider, P.; Scottez, V.; Secroun, A.; Serrano, S.; Sirignano, C.; Sirri, G.; Sureau, F.; Tallada Crespi, P.; Tavagnacco, D.; Taylor, A. N.; Tenti, M.; Tereno, I.; Toledo Moreo, R.; Torradeflot, F.; Tramacere, A.; Valenziano, L.; Vassallo, T.; Wang, Y.; Welikala, N.; Wetzstein, M.; Whittaker, L.; Zacchei, A.; Zamorani, G.; Zoubian, J.; Zucca, E. (EDP Science, 2020)
      The Complete Calibration of the Colour-Redshift Relation survey (C3R2) is a spectroscopic e ffort involving ESO and Keck facilities designed specifically to empirically calibrate the galaxy colour-redshift relation - P(z ...
    • Blanchard, A.; Camera, S.; Carbone, C.; Cardone, V. F.; Casas, S.; Clesse, S.; Ilic, S.; Kilbinger, M.; Kitching, T.; Kunz, M.; Lacasa, F.; Linder, E.; Majerotto, E.; Markovic, K.; Martinelli, M.; Pettorino, V.; Pourtsidou, A.; Sakr, Z.; Sánchez, A. G.; Sapone, D.; Tutusaus, I.; Yahia-Cherif, S.; Yankelevich, V.; Andreon, S.; Aussel, H.; Balaguera-Antolinez, A.; Baldi, M.; Bardelli, S.; Bender, R.; Biviano, A.; Bonino, D.; Boucaud, A.; Bozzo, E.; Branchini, E.; Brau Nogue, S.; Brescia, M.; Brinchmann, J.; Burigana, C.; Cabanac, R.; Capobianco, V.; Cappi, A.; Carretero, J.; Carvalho, C.S.; Casas, R.; Castander, F. J.; Castellano, M.; Cavuoti, S.; Cimatti, A.; Cledassou, R.; Colodro Conde, C.; Congedo, G.; Conselice, C.J.; Conversi, L.; Copin, Y.; Corcione, L.; Coupon, J.; Courtois, H. M.; Cropper, M.; Da Silva, A.; de la Torre, S.; Di Ferdinando, D.; Dubath, F.; Ducret, F.; Duncan, C. A. J.; Dupac, X.; Dusini, S.; Fabbian, G.; Fabricius, M.; Farrens, S.; Fosalba, P.; Fotopoulou, S.; Fourmanoit, N.; Frailis, M.; Franceschi, E.; Franzetti, P.; Fumana, M.; Galeotta, S.; Gillard, W.; Gillis, B.; Giocoli, C.; Gómez-Álvarez, P.; Gracia Carpio, J.; Grupp, F.; Guzzo, L.; Hoekstra, H.; Hormuth, F.; Israel, H.; Jahnke, K.; Keihanen, E.; Kermiche, S.; Kirkpatrick, C. C.; Kohley, R.; Kubik, B.; Kurki-Suonio, H.; Ligori, S.; Lilje, P. B.; Lloro, I.; Maino, D.; Maiorano, E.; Marggraf, O.; Martinet, N.; Marulli, F.; Massey, R.; Medinaceli, E.; Mei, S.; Mellier, Y.; Metcalf, B.; Metge, J.J.; Meylan, G.; Moresco, M.; Moscardini, L.; Munari, E.; Nichol, R. C.; Niemi, S.; Nucita, A.A.; Padilla, C.; Paltani, S.; Pasian, F.; Percival, W. J.; Pires, S.; Polenta, G.; Poncet, M.; Pozzetti, L.; Racca, G.D.; Raison, F.; Renzi, A.; Rhodes, J.; Romelli, E.; Roncarelli, M.; Rossetti, E.; Saglia, R.; Schneider, P.; Scottez, V.; Secroun, A.; Sirri, G.; Stanco, L.; Starck, J. L.; Sureau, F.; Tallada Crespi, P.; Tavagnacco, D.; Taylor, A. N.; Tenti, M.; Tereno, I.; Toledo Moreo, R.; Torradeflot, F.; Valenziano, L.; Vassallo, T.; Kleijn, G. A. Verdoes; Viel, M.; Wang, Y.; Zacchei, A.; Zoubian, J.; Zucca, E. (EDP Science, 2020)
      Aims. The Euclid space telescope will measure the shapes and redshifts of galaxies to reconstruct the expansion history of the Universe and the growth of cosmic structures. The estimation of the expected performance of the ...
    • Roje, Tomislav; Sáez Hueichapan, Doris; Muñoz, Carlos; Daniele, Linda (MDPI, 2020)
      Generating strategies and techniques to feed the increasing world population is a significant challenge under climate change effects such as drought. Rural areas are especially sensitive to such effects as they are unable ...
    • Ginski, C.; Menard, F.; Rab, C.; Mamajek, E. E.; van Holstein, R. G.; Benisty, M.; Manara, C. F.; Torres, R. Asensio; Bohn, A.; Birnstiel, T.; Delorme, P.; Facchini, S.; Garufi, A.; Gratton, R.; Hogerheijde, M.; Huang, J.; Kenworthy, M.; Langlois, M.; Pinilla, P.; Pinte, C.; Ribas, Á.; Rosotti, G.; Schmidt, T. O. B.; Van den Ancker, M.; Wahhaj, Z.; Waters, L. B. F. M.; Williams, J.; Zurlo, A. (EDP Science, 2020)
      Context. To understand the formation of planetary systems, it is important to understand the initial conditions of planet formation, that is, the young gas-rich planet forming disks. Spatially resolved, high-contrast ...
    • Steimer, Sarah S.; Patton, Daniel J.; Vu, Tuan V.; Panagi, Marios; Monks, Paul S.; Harrison, Roy M.; Fleming, Zoe L.; Shi, Zongbo; Kalberer, Markus (Copernicus gesellschaft MBH, 2020)
      This study investigates the chemical composition of PM2.5 collected at a central location in Beijing, China, during winter 2016 and summer 2017. The samples were characterised using direct-infusion negative-nano-electros ...
    • Facanha, Agebson Rocha; Darin, Ticianne; Viana, Windson; Sánchez Ilabaca, Jaime (Association for Computing Machinery, USA, 2020)
      BACKGROUND: Knowing their current position in the surroundings constitutes one of the biggest challenges faced by people with visual disabilities when they move around. For them, it is difficult to be aware of the direction ...
    • Mahmoodzadeh, Zahra; Wu, Keo-Yuan; López Droguett, Enrique; Mosleh, Ali (MDPI, 2020)
      Gas pipeline systems are one of the largest energy infrastructures in the world and are known to be very efficient and reliable. However, this does not mean they are prone to no risk. Corrosion is a significant problem in ...
    • Lazzoni, C.; Zurlo, A.; Desidera, S.; Mesa, D.; Fontanive, C.; Bonavita, M.; Ertel, S.; Rice, K.; Vigan, A.; Boccaletti, A.; Bonnefoy, M.; Chauvin, Gaël; Delorme, P.; Gratton, R.; Houllé, M.; Maire, A.L.; Meyer, M.; Rickman, E.; Spalding, E. A.; Asensio Torres, R.; Langlois, M.; Müller, A.; Baudino, J L.; Beuzit, J. L.; Biller, B.; Brandner, W.; Buenzli, E.; Cantalloube, F.; Cheetham, A.; Cudel, M.; Feldt, M.; Galicher, R.; Janson, M.; Hagelberg, J.; Henning, T.; Kasper, M.; Keppler, M.; Lagrange, A. M; Lannier, J.; LeCoroller, H.; Mouillet, D.; Peretti, S.; Perrot, C.; Salter, G.; Samland, M.; Schmidt, T.; Sissa, E.; Wildi, F. (EDP Science, 2020)
      Context. In recent decades, thousands of substellar companions have been discovered with both indirect and direct methods of detection. While the majority of the sample is populated by objects discovered using radial ...
    • Areal, M. B.; Paron, S.; Fariña, C.; Ortega, M. E.; Celis Peña, M.; Rubio López, Mónica (EDP Science, 2020)
      Aims. To advance our knowledge of star formation, in addition to statistical studies and large surveys of young stellar objects (YSOs), it is important to carry out detailed studies towards particular objects. Given that ...
    • Villenave, M.; Menard, F.; Dent, W. R. F.; Duchene, G.; Stapelfeldt, K. R.; Benisty, M.; Boehler, Y.; Van der Plas, G.; Pinte, C.; Telkamp, Z.; Wolff, S.; Flores, C.; Lesur, G.; Louvet, F.; Riols, A.; Dougados, C.; Williams, H.; Padgett, D. (EDP, 2020)
      Aims. We aim to study vertical settling and radial drift of dust in protoplanetary disks from a different perspective: an edge-on view. An estimation of the amplitude of settling and drift is highly relevant to understanding ...