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Mostrando 621 - 640 Resultados de 962 Para Buscar '"Solar System"', tiempo de consulta: 0.24s Limitar resultados
  1. 621
    “…Hydrogen is the most abundant element in the solar system and thus one of the important candidates. …”
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    Hydrogenation of iron in the early stage of Earth's evolution
  2. 622
    “…Volatile element and compound abundances vary widely in planets and were set during the earliest stages of solar system evolution. Experiments or natural analogs approximating these early conditions are limited. …”
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    Evaporative fractionation of zinc during the first nuclear detonation
  3. 623
    “…The size and shape of this “Great Cold Spot” vary significantly with time, strongly suggesting that it is produced by an aurorally generated weather system: the first direct evidence of a long‐term thermospheric vortex in the solar system. We discuss the implications of this spot, comparing it with short‐term temperature and density variations at Earth.…”
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    The Great Cold Spot in Jupiter's upper atmosphere
  4. 624
    por Teachey, Alex, Kipping, David M.
    Publicado 2018
    “…Exomoons are the natural satellites of planets orbiting stars outside our solar system, of which there are currently no confirmed examples. …”
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    Evidence for a large exomoon orbiting Kepler-1625b
  5. 625
    por Schmieder, Martin, Kring, David A.
    Publicado 2020
    “…High-precision impact ages can be used to (1) reconstruct and quantify the impact flux in the inner Solar System and, in particular, the Earth–Moon system, thereby placing constraints on the delivery of extraterrestrial mass accreted on Earth through geologic time; (2) utilize impact ejecta as event markers in the stratigraphic record and to refine bio- and magneto-stratigraphy; (3) test models and hypotheses of synchronous double or multiple impact events in the terrestrial record; (4) assess the potential link between large impacts, mass extinctions, and diversification events in the biosphere; and (5) constrain the duration of melt sheet crystallization in large impact basins and the lifetime of hydrothermal systems in cooling impact craters, which may have served as habitats for microbial life on the early Earth and, possibly, Mars.…”
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    Earth's Impact Events Through Geologic Time: A List of Recommended Ages for Terrestrial Impact Structures and Deposits
  6. 626
    “…The behavior of ice under extreme conditions undergoes the change of intermolecular binding patterns and leads to the structural phase transitions, which are needed for modeling the convection and internal structure of the giant planets and moons of the solar system as well as H2O-rich exoplanets. Such extreme conditions limit the structural explorations in laboratory but open a door for the theoretical study. …”
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    Phase Transition of Ice at High Pressures and Low Temperatures
  7. 627
    “…At the Berkeley Space Sciences Laboratory, we are working to further expand this technology by developing analytical instruments to chemically explore our solar system. This effort requires improving the quality and reliability of glass microfabrication through quality control procedures at every stage of design and manufacture. …”
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    Fabrication of high-quality glass microfluidic devices for bioanalytical and space flight applications
  8. 628
    “…Among the celestial bodies in the Solar System, Mars currently represents the main target for the search for life beyond Earth. …”
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    Iron Ion Particle Radiation Resistance of Dried Colonies of Cryomyces antarcticus Embedded in Martian Regolith Analogues
  9. 629
    “…Ethane is an important constituent in the atmospheres of the gas giants in our solar system. The present work describes translational spectroscopy studies of the VUV photochemistry of ethane using tuneable radiation in the wavelength range 112 ≤ λ ≤ 126 nm from a free electron laser and event-triggered, fast-framing, multi-mass imaging detection methods. …”
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    Ultraviolet photochemistry of ethane: implications for the atmospheric chemistry of the gas giants
  10. 630
    por IYE, Masanori
    Publicado 2021
    “…Selected scientific topics include studies on cosmic reionization, weak/strong gravitational lensing, cosmological parameters, primordial black holes, the dynamical/chemical evolution/interactions of galaxies, neutron star mergers, supernovae, exoplanets, proto-planetary disks, and outliers of the solar system. The last described are operational statistics, plans and a note concerning the culture-and-science issues in Hawaii.…”
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    Subaru Telescope —History, active/adaptive optics, instruments, and scientific achievements—
  11. 631
    “…As one of the most spectacular energy release events in the solar system, solar flares are generally powered by magnetic reconnection in the solar corona. …”
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    Plasma Heating Induced by Tadpole-like Downflows in the Flaring Solar Corona
  12. 632
    por Malhotra, Renu, Ito, Takashi
    Publicado 2022
    “…Many of the unusual properties of Pluto’s orbit are widely accepted as evidence for the orbital migration of the giant planets in early solar system history. However, some properties remain an enigma. …”
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    Pluto near the edge of chaos
  13. 633
    “…These results can be useful in developing a strategy for protecting reproductive health during the development of other bodies in the solar system.…”
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    Sperm of Fruit Fly Drosophila melanogaster under Space Flight
  14. 634
    “…Water bodies on Mars and the icy moons of the outer solar system are now recognized as likely being associated with high levels of salt. …”
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    The archaeal class Halobacteria and astrobiology: Knowledge gaps and research opportunities
  15. 635
    por Wang, Mingjing, Chen, Long, Chen, Huiling
    Publicado 2022
    “…Modeling solar systems necessitates the effective identification of unknown and variable photovoltaic parameters. …”
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    Multi-Strategy Learning Boosted Colony Predation Algorithm for Photovoltaic Model Parameter Identification
  16. 636
    por Lederer, C., Massimi, C., Berthoumieux, E., Colonna, N., Dressler, R., Guerrero, C., Gunsing, F., Käppeler, F., Kivel, N., Pignatari, M., Reifarth, R., Schumann, D., Wallner, A., Altstadt, S., Andriamonje, S., Andrzejewski, J., Audouin, L., Barbagallo, M., Bécares, V., Bečvář, F., Belloni, F., Berthier, B., Billowes, J., Boccone, V., Bosnar, D., Brugger, M., Calviani, M., Calviño, F., Cano-Ott, D., Carrapiço, C., Cerutti, F., Chiaveri, E., Chin, M., Cortés, G., Cortés-Giraldo, M.A., Dillmann, I., Domingo-Pardo, C., Duran, I., Dzysiuk, N., Eleftheriadis, C., Fernández-Ordóñez, M., Ferrari, A., Fraval, K., Ganesan, S., García, A.R., Giubrone, G., Gómez-Hornillos, M.B., Gonçalves, I.F., González-Romero, E., Gramegna, F., Griesmayer, E., Gurusamy, P., Harrisopulos, S., Heil, M., Ioannides, K., Jenkins, D.G., Jericha, E., Kadi, Y., Karadimos, D., Korschinek, G., Krtička, M., Kroll, J., Langer, C., Lebbos, E., Leeb, H., Leong, L.S., Losito, R., Lozano, M., Manousos, A., Marganiec, J., Marrone, S., Martinez, T., Mastinu, P.F., Mastromarco, M., Meaze, M., Mendoza, E., Mengoni, A., Milazzo, P.M., Mingrone, F., Mirea, M., Mondalaers, W., Paradela, C., Pavlik, A., Perkowski, J., Plag, R., Plompen, A., Praena, J., Quesada, J.M., Rauscher, T., Riego, A., Roman, F., Rubbia, C., Sarmento, R., Schillebeeckx, P., Schmidt, S., Tagliente, G., Tain, J.L., Tarrío, D., Tassan-Got, L., Tsinganis, A., Tlustos, L., Valenta, S., Vannini, G., Variale, V., Vaz, P., Ventura, A., Vermeulen, M.J., Versaci, R., Vlachoudis, V., Vlastou, R., Ware, T., Weigand, M., Weiß, C., Wright, T.J., Žugec, P.
    Publicado 2014
    “…These results provide fundamental constraints on $s$-process production of heavier species, especially the production of Cu in massive stars, which serve as the dominant source of Cu in the solar system.…”
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    $^{62}$Ni($n,\gamma$) and $^{63}$Ni($n,\gamma$) cross sections measured at n_TOF/CERN
  17. 637
    por Aghanim, N, Armitage-Caplan, C, Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Banday, A J, Barreiro, R B, Battaner, E, Benabed, K, Benoît, A, Benoit-Lévy, A, Bernard, J -P, Bersanelli, M, Bielewicz, P, Bobin, J, Bock, J J, Bonaldi, A, Bonavera, L, Bond, J R, Borrill, J, Bouchet, F R, Bridges, M, Bucher, M, Burigana, C, Butler, R C, Cappellini, B, Cardoso, J -F, Catalano, A, Chamballu, A, Chen, X, Chiang, L -Y, Christensen, P R, Church, S, Colombi, S, Colombo, L P L, Crill, B P, Curto, A, Cuttaia, F, Danese, L, Davies, R D, Davis, R J, de Bernardis, P, de Rosa, A, de Zotti, G, Delabrouille, J, Dickinson, C, Diego, J M, Dole, H, Donzelli, S, Doré, O, Douspis, M, Dupac, X, Efstathiou, G, Enßlin, T A, Eriksen, H K, Finelli, F, Forni, O, Frailis, M, Franceschi, E, Gaier, T C, Galeotta, S, Ganga, K, Giard, M, Giardino, G, Giraud-Héraud, Y, Gjerløw, E, González-Nuevo, J, Górski, K M, Gratton, S, Gregorio, A, Gruppuso, A, Hansen, F K, Hanson, D, Harrison, D, Henrot-Versillé, S, Hernández-Monteagudo, C, Herranz, D, Hildebrandt, S R, Hivon, E, Hobson, M, Holmes, W A, Hornstrup, A, Hovest, W, Huffenberger, K M, Jaffe, T R, Jaffe, A H, Jewell, J, Jones, W C, Juvela, M, Kangaslahti, P, Keihänen, E, Keskitalo, R, Kisner, T S, Knoche, J, Knox, L, Kunz, M, Kurki-Suonio, H, Lagache, G, Lähteenmäki, A, Lamarre, J -M, Lasenby, A, Laureijs, R J, Lawrence, C R, Leach, S, Leahy, J P, Leonardi, R, Lesgourgues, J, Liguori, M, Lilje, P B, Linden-Vørnle, M, López-Caniego, M, Lubin, P M, Macías-Pérez, J F, Maino, D, Mandolesi, N, Maris, M, Marshall, D J, Martin, P G, Martínez-González, E, Masi, S, Matarrese, S, Matthai, F, Mazzotta, P, Meinhold, P R, Melchiorri, A, Mendes, L, Mennella, A, Migliaccio, M, Mitra, S, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Moss, A, Munshi, D, Naselsky, P, Natoli, P, Netterfield, C B, Nørgaard-Nielsen, H U, Novikov, D, Novikov, I, O'Dwyer, I J, Osborne, S, Paci, F, Pagano, L, Paladini, R, Paoletti, D, Partridge, B, Pasian, F, Patanchon, G, Pearson, D, Peel, M, Perdereau, O, Perotto, L, Perrotta, F, Pierpaoli, E, Pietrobon, D, Plaszczynski, S, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poutanen, T, Pratt, G W, Prézeau, G, Prunet, S, Puget, J -L, Rachen, J P, Rebolo, R, Reinecke, M, Remazeilles, M, Ricciardi, S, Riller, T, Rocha, G, Rosset, C, Rossetti, M, Roudier, G, Rubiño-Martín, J A, Rusholme, B, Sandri, M, Santos, D, Scott, D, Seiffert, M D, Shellard, E P S, Spencer, L D, Starck, J -L, Stolyarov, V, Stompor, R, Sureau, F, Sutton, D, Suur-Uski, A -S, Sygnet, J -F, Tauber, J A, Tavagnacco, D, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Tucci, M, Tuovinen, J, Türler, M, Umana, G, Valenziano, L, Valiviita, J, Van Tent, B, Varis, J, Vielva, P, Villa, F, Vittorio, N, Wade, L A, Wandelt, B D, Watson, R, Wilkinson, A, Yvon, D, Zacchei, A, Zonca, A
    Publicado 2013
    “…Our calibration is based on a combination of the Orbital Dipole plus the Solar Dipole, caused respectively by the motion of the Planck spacecraft with respect to the Sun and by motion of the Solar System with respect to the CMB rest frame. The latter provides a signal of a few mK with the same spectrum as the CMB anisotropies and is visible throughout the mission. …”
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    Planck 2013 results. V. LFI calibration
  18. 638
    por Thagard, Paul
    Publicado 1992
    Libro
    Conceptual revolutions /
  19. 639
    por Beech, Martin
    Publicado 2009
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    Terraforming: The Creating of Habitable Worlds
  20. 640
    por Cooke, Antony
    Publicado 2009
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    Make Time for the Stars
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