Results 21 to 30 of about 3,608,924 (307)
Development of a Machine Learning Forecast Model for Global Horizontal Irradiation Adapted to Tibet Based on Visible All-Sky Imaging
Remote Sensing, 2023 The Qinghai-Tibet Plateau is rich in renewable solar energy resources. Under the background of China’s “dual-carbon” strategy, it is of great significance to develop a global horizontal irradiation (GHI) prediction model suitable for Tibet.Lingxiao Wu, Tianlu Chen, Nima Ciren, Dui Wang, Huimei Meng, Ming Li, Wei Zhao, Jingxuan Luo, Xiaoru Hu, Shengjie Jia, Li Liao, Yubing Pan, Yinan Wang +12 moredoaj +1 more sourceRETRACTED: EEG Signal Connectivity for Characterizing Interictal Activity in Patients With Mesial Temporal Lobe Epilepsy
Frontiers in Neurology, 2021 Over the last decade, several methods for analysis of epileptiform signals in electroencephalography (EEG) have been proposed. These methods mainly use EEG signal features in either the time or the frequency domain to separate regular, interictal, and ...Leonardo R. da Costa, Leonardo R. da Costa, Brunno M. de Campos, Brunno M. de Campos, Marina K. M. Alvim, Gabriela Castellano, Gabriela Castellano +6 moredoaj +1 more sourceRed Dwarfs as Sources of Cosmic Rays [PDF]
EPJ Web of Conferences, 2022 The Pamela, Fermi, AMS-02 spectrometer experimental data cannot be explained using the diffusive models of propagation of cosmic-rays accelerated at the supernova shocks and require the existence of nearby sources of cosmic rays at the distances less ...Sinitsyna Vera Yu., Sinitsyna Vera G., Stozhkov Yurii I. +2 moredoaj +1 more sourceCharmed Galaxies [PDF]
EPJ Web of Conferences, 2023 The quest for finding the origins of cosmic rays has been going on for many decades. Cosmic rays as charged particles react to cosmic magnetic fields and typically travel in diffusive motion through the Universe.Becker Tjus Julia, Rhode Wolfgangdoaj +1 more sourceObservation of a large-scale anisotropy in the arrival directions of cosmic rays above 8 × 1018 eV [PDF]
Science, 2017 Cosmic rays are atomic nuclei arriving from outer space that reach the highest energies observed in nature. Clues to their origin come from studying the distribution of their arrival directions.A. Aab, P. Abreu, M. Aglietta, I. Al Samarai, I. Albuquerque, I. Allekotte, A. Almela, J. Alvarez Castillo, J. Álvarez-Muñiz, G. A. Anastasi, L. Anchordoqui, B. Andrada, S. Andringa, C. Aramo, F. Arqueros, N. Arsene, Hernán Asorey, P. Assis, J. Aublin, G. Avila, A. Badescu, A. Bălăceanu, F. Barbato, R. J. Barreira Luz, J. Beatty, K. Becker, J. Bellido, C. Bérat, M. Bertaina, X. Bertou, P. Biermann, P. Billoir, J. Biteau, S. Blaess, A. Blanco, J. Blazek, C. Bleve, M. Boháčová, D. Boncioli, C. Bonifazi, N. Borodai, A. Botti, J. Brack, I. Brancus, T. Bretz, A. Bridgeman, F. Briechle, P. Buchholz, A. Bueno, S. Buitink, M. Buscemi, K. Caballero-Mora, L. Caccianiga, A. Cancio, F. Canfora, L. Caramete, R. Caruso, A. Castellina, G. Cataldi, L. Cazon, A. Chavez, J. Chinellato, J. Chudoba, R. Clay, A. Cobos, R. Colalillo, A. Coleman, L. Collica, M. Coluccia, R. Conceição, G. Consolati, F. Contreras, M. Cooper, S. Coutu, C. Covault, J. Cronin, S. D'Amico, B. Daniel, S. Dasso, K. Daumiller, B. Dawson, R. D. de Almeida, S. D. de Jong, G. De Mauro, J. D. M. de Mello Neto, I. De Mitri, J. de Oliveira, V. de Souza, J. Debatin, O. Deligny, C. Di Giulio, A. di Matteo, M. L. Díaz Castro, F. Diogo, C. Dobrigkeit, J. D'Olivo, Q. Dorosti, R. D. dos Anjos, M. Dova, A. Dundović, J. Ebr, R. Engel, M. Erdmann, M. Erfani, C. Escobar, J. Espadanal, A. Etchegoyen, H. Falcke, G. Farrar, A. Fauth, N. Fazzini, F. Fenu, B. Fick, J. M. Figueira, A. Filipčič, O. Fratu, M. Freire, T. Fujii, A. Fuster, R. Gaior, B. Garcia, D. García-Pinto, F. Gaté, H. Gemmeke, A. Gherghel-Lascu, P. Ghia, U. Giaccari, M. Giammarchi, M. Giller, D. Glas, C. Glaser, G. Golup, M. Gómez Berisso, P. F. Gómez Vitale, N. González, A. Gorgi, P. Gorham, A. Grillo, T. D. Grubb, F. Guarino, G. Guedes, M. Hampel, P. Hansen, D. Harari, T. Harrison, J. Harton, A. Haungs, T. Hebbeker, D. Heck, P. Heimann, A. Hervé, G. Hill, C. Hojvat, E. Holt, P. Homola, J. Hörandel, P. Horváth, M. Hrabovsky, T. Huege, J. Hulsman, A. Insolia, P. G. Isar, I. Jandt, S. Jansen, J. Johnsen, M. Josebachuili, J. Juryšek, A. Kääpä, O. Kambeitz, K. Kampert, I. Katkov, B. Keilhauer, N. Kemmerich, E. Kemp, J. Kemp, R. Kieckhafer, H. Klages, M. Kleifges, J. Kleinfeller, R. Krause, N. Krohm, D. Kuempel, G. Kukec Mezek, N. Kunka, A. Kuotb Awad, D. LaHurd, M. Lauscher, R. Legumina, M. D. de Oliveira, A. Letessier-Selvon, I. Lhenry-Yvon, K. Link, D. Lo Presti, L. Lopes, R. Lopez, A. López Casado, Q. Luce, A. Lucero, M. Malacari, M. Mallamaci, D. Mandát, P. Mantsch, A. Mariazzi, I. Mariş, G. Marsella, D. Martello, H. Martinez, O. M. Martinez Bravo, J. J. Masías Meza, H. Mathes, S. Mathys, J. Matthews, J. Matthews, G. Matthiae, E. Mayotte, P. Mazur, C. Medina, G. Medina-Tanco, D. Melo, A. Menshikov, K. Merenda, S. Michal, M. Micheletti, L. Middendorf, L. Miramonti, B. Mitrica, D. Mockler, S. Mollerach, F. Montanet, C. Morello, M. Mostafá, A. Müller, G. Müller, M. Muller, S. Müller, R. Mussa, I. Naranjo, L. Nellen, P. Nguyen, M. Niculescu-Oglinzanu, M. Niechciol, L. Niemietz, T. Niggemann, D. Nitz, D. Nosek, V. Novotny, L. Nožka, L. Núñez, L. Ochilo, F. Oikonomou, A. Olinto, M. Palatka, J. Pallotta, P. Papenbreer, G. Parente, A. Parra, T. Paul, M. Pech, F. Pedreira, J. Pkala, R. Pelayo, J. Peña-Rodríguez, L. Pereira, M. Perlin, L. Perrone, C. Peters, S. Petrera, J. Phuntsok, R. Piegaia, T. Pierog, P. Pieroni, M. Pimenta, V. Pirronello, M. Platino, M. Plum, C. Porowski, R. Prado, P. Privitera, M. Prouza, E. Quel, S. Querchfeld, S. Quinn, R. Ramos-Pollán, J. Rautenberg, D. Ravignani, B. Revenu, J. Řídký, F. Riehn, M. Risse, P. Ristori, V. Rizi, W. R. de Carvalho, G. Rodriguez Fernandez, J. R. Rodriguez Rojo, D. Rogozin, M. Roncoroni, M. Roth, E. Roulet, A. Rovero, P. Ruehl, S. Saffi, A. Săftoiu, F. Salamida, H. Salazar, A. Saleh, F. Salesa Greus, G. Salina, F. Sánchez, P. Sanchez-Lucas, E. Santos, E. Santos, F. Sarazin, R. Sarmento, C. A. Sarmiento, R. Sato, M. Schauer, V. Scherini, H. Schieler, M. Schimp, D. Schmidt, O. Scholten, P. Schovánek, F. Schröder, A. Schulz, J. Schumacher, S. Sciutto, A. Segreto, M. Settimo, A. Shadkam, R. Shellard, G. Sigl, G. Silli, O. Sima, A. Śmiałkowski, R. Smida, G. Snow, P. Sommers, S. Sonntag, J. Sorokin, R. Squartini, D. Stanca, S. Stanič, J. Stasielak, P. Stassi, F. Strafella, F. Suarez, M. Suarez Durán, T. Sudholz, T. Suomijärvi, A. Supanitsky, J. Supik, J. Swain, Z. Szadkowski, A. Taboada, O. Taborda, A. Tapia, V. M. Theodoro, C. Timmermans, C. J. Todero Peixoto, L. Tomankova, B. Tomé, G. Torralba Elipe, P. Trávníček, M. Trini, R. Ulrich, M. Unger, M. Urban, J. F. Valdés Galicia, I. Valiño, L. Valore, G. van Aar, P. van Bodegom, A. M. van den Berg, A. van Vliet, E. Varela, B. Vargas Cárdenas, G. Varner, R. Vazquez, D. Veberič, C. Ventura, I. D. Vergara Quispe, V. Verzi, J. Vícha, L. Villaseñor, S. Vorobiov, H. Wahlberg, O. Wainberg, D. Walz, A. Watson, M. Weber, A. Weindl, L. Wiencke, H. Wilczynski, M. Wirtz, D. Wittkowski, B. Wundheiler, L. Yang, A. Yushkov, E. Zas, D. Zavrtanik, M. Zavrtanik, A. Zepeda, B. Zimmermann, M. Ziolkowski, Z. Zong, F. Zuccarello +405 moresemanticscholar +1 more sourceFunctionalized UiO-66-NH2 by trimellitic acid for highly selective adsorption of basic blue 3 from aqueous solutions
Frontiers in Chemistry, 2022 A novel metal-organic framework (MOF) UiO-66-TLA (UiO-66-Trimellitic Acid) was synthesized by one-pot method with trimellitic acid as modifier, which can effectively remove the basic dye Basic Blue 3 (BB3) in wastewater. Modification with carboxyl groups Tingting Wang, Tingting Wang, Tingting Wang, Tingting Wang, Lin Han, Lin Han, Lin Han, Lin Han, Xin Li, Xin Li, Xin Li, Xin Li, Tianen Chen, Tianen Chen, Shifeng Wang, Shifeng Wang, Shifeng Wang +16 moredoaj +1 more sourceThe origin of cosmic rays [PDF]
Journal of Physics G: Nuclear and Particle Physics, 1999 It is generally regarded that the bulk of cosmic rays originate in the Galaxy and that those below the 'knee' (the rapid steepening in the energy spectrum) at a few PeV come from Galactic supernovae, the particles being accelerated by the shocks in the supernova remnants.A D Erlykin, A D Erlykin, A. W. Wolfendale +2 moreopenaire +6 more sources