Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Dan C. Spencer"'
Autor:
Laszlo P. Kestay, Katherine de Kleer, Ariana Echevarria, A. Trinh, Gregor Steinbrügge, Mark P. Panning, Cesare Grava, Audrey Vorburger, Constantine Tsang, Fran Bagenal, Hamish C. F. C. Hay, Gregory A. Neumann, Julie A. Rathbun, Tracy K. P. Gregg, Tanguy Bertrand, Carver J. Bierson, Christopher W. Hamilton, Imke de Pater, Rowan Huang, Krishan K. Khurana, J. I. Moses, John Noonan, James Tuttle Keane, Isamu Matsuyama, Rachel L. Klima, Lea Klaiber, Laurent G. J. Montési, Michael T. Bland, Joseph Westlake, Quentin Nénon, Elias Roussos, Laura Kerber, Rohan Sood, J. T. Keane, Christine McCarthy, Melissa A. McGrath, Sarah M. Hörst, Kandis Lea Jessup, Amanda R. Hendrix, Alfred S. McEwen, C. D. K. Harris, Marc Neveu, Tilmann Denk, Paul M. Schenk, Maurizio Pajola, Xianzhe Jia, Nicholas M. Schneider, Arielle Moullet, Lauren Jozwiak, Daniella DellaGiustina, Alice Lucchetti, Jani Radebaugh, John R. Spencer, Lori M. Feaga, Catherine Elder, Ashley Davies, Patricio Becerra, Rosaly M. C. Lopes, Doris Breuer, Amy C. Barr Mlinar, Michelle R. Kirchoff, Dan C. Spencer, Corbin L. Kling, Andréa C. G. Hughes, Kurt D. Retherford, Francis Nimmo, J. Schools, David A. Williams, Ryan S. Park, Walter S. Kiefer, Walter M. Harris, Edwin S. Kite, Ali Sulaiman, Lynnae C. Quick, Ross A. Beyer, Anne Pommier, James H. Roberts, Sarah S. Sutton, Janet Vertesi, Patricia M. Gregg, Ko Basu, Valery Lainey, Alexandra A. Ahern, Kathleen Mandt
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5b5ebb90076cb1141fdfcfd44cab0ddc
https://doi.org/10.3847/25c2cfeb.3de45b59
https://doi.org/10.3847/25c2cfeb.3de45b59
Tidal heating is expected to impart significant, non-spherically-symmetric structure to Jupiter's volcanic moon Io. A signature of spatially variable tidal heating is generally sought in observations of surface heat fluxes or volcanic activity, an ex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::094b4a0e27435203428de196da25d657
Publikováno v:
Journal of Geophysical Research: Planets
Magmatic segregation and volcanic eruptions transport tidal heat from Io's interior to its surface. Several observed eruptions appear to be extremely high temperature ($\geq$ 1600 K), suggesting either very high degrees of melting, refractory source
Autor:
'Dan C. Spencer
Publikováno v:
Richard F. Katz
Publikováno v:
Journal of Geophysical Research: Planets
Io, the most volcanically active body in the solar system, loses heat through eruptions of hot lava. Heat is supplied by tidal heating and is thought to be transferred through the mantle by magmatic segregation, a mode of transport that sets it apart