Zobrazeno 1 - 10
of 26
pro vyhledávání: '"W. M. Folkner"'
Autor:
D. Durante, M. Parisi, D. Serra, M. Zannoni, V. Notaro, P. Racioppa, D. R. Buccino, G. Lari, L. Gomez Casajus, L. Iess, W. M. Folkner, G. Tommei, P. Tortora, S. J. Bolton
Publikováno v:
Geophysical Research Letters, Vol 47, Iss 4, Pp n/a-n/a (2020)
Abstract The Juno spacecraft reached the mid‐point of its nominal mission in December 2018, after completing 17 perijove passes. Ten of these were dedicated to the determination of the gravity field of the planet, with the aim of constraining its i
Externí odkaz:
https://doaj.org/article/c0f1c4ff4b5e4d0390b41189fcebfdf2
Autor:
Luciano Iess, Daniele Serra, Dustin Buccino, P. Racioppa, Paolo Tortora, Marco Zannoni, Marzia Parisi, Giacomo Lari, Scott Bolton, W. M. Folkner, Virginia Notaro, Daniele Durante, Giacomo Tommei, L. Gomez Casajus
The Juno spacecraft reached the mid‐point of its nominal mission in December 2018, after completing 17 perijove passes. Ten of these were dedicated to the determination of the gravity field of the planet, with the aim of constraining its interior s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0c0adc46d1eb9b10ac3bda52866b0b0
https://hdl.handle.net/11585/724886
https://hdl.handle.net/11585/724886
Autor:
Ravit Helled, S. M. Wahl, Steven Levin, Luciano Iess, Jonathan I. Lunine, Scott Bolton, William B. Hubbard, D. J. Stevenson, Daniel R. Reese, Daniele Durante, Tristan Guillot, Eli Galanti, Hao Cao, Yamila Miguel, Marzia Parisi, W. M. Folkner, Yohai Kaspi, John E. P. Connerney, A. Biekman, Burkhard Militzer
Publikováno v:
Nature
Nature, Nature Publishing Group, 2018, 555 (7695), pp.227-230. ⟨10.1038/nature25775⟩
Nature, 2018, 555 (7695), pp.227-230. ⟨10.1038/nature25775⟩
Nature, 555, 227-230
Nature, Nature Publishing Group, 2018, 555 (7695), pp.227-230. ⟨10.1038/nature25775⟩
Nature, 2018, 555 (7695), pp.227-230. ⟨10.1038/nature25775⟩
Nature, 555, 227-230
International audience; Jupiter’s atmosphere is rotating differentially, with zones and belts rotating at speeds that differ by up to 100 metres per second. Whether this is also true of the gas giant’s interior has been unknown1,2, limiting our a
Publikováno v:
Planetary and Space Science. 152:107-115
The International Astronomical Union (IAU) defines planet and satellite coordinate systems relative to their axis of rotation and the angle about that axis. The rotational elements of the bodies are the right ascension and declination of the rotation
Autor:
J. D. Anderson, Michael Feldman, Daniele Serra, Giacomo Tommei, M. Gregnanin, John E. P. Connerney, Sami W. Asmar, Luciano Iess, Marco Zannoni, Andrea Milani, Dustin Buccino, Daniele Durante, Paolo Tortora, Steven Levin, W. M. Folkner, L. Gomez Casajus, Ryan S. Park, Scott Bolton, Marzia Parisi
Publikováno v:
Geophysical Research Letters. 44:4694-4700
The combination of the Doppler data from the first two Juno science orbits provides an improved estimate of the gravity field of Jupiter, crucial for interior modeling of giant planets. The low-degree spherical harmonic coefficients, especially J4 an
Autor:
S A, Stern, H A, Weaver, J R, Spencer, C B, Olkin, G R, Gladstone, W M, Grundy, J M, Moore, D P, Cruikshank, H A, Elliott, W B, McKinnon, J Wm, Parker, A J, Verbiscer, L A, Young, D A, Aguilar, J M, Albers, T, Andert, J P, Andrews, F, Bagenal, M E, Banks, B A, Bauer, J A, Bauman, K E, Bechtold, C B, Beddingfield, N, Behrooz, K B, Beisser, S D, Benecchi, E, Bernardoni, R A, Beyer, S, Bhaskaran, C J, Bierson, R P, Binzel, E M, Birath, M K, Bird, D R, Boone, A F, Bowman, V J, Bray, D T, Britt, L E, Brown, M R, Buckley, M W, Buie, B J, Buratti, L M, Burke, S S, Bushman, B, Carcich, A L, Chaikin, C L, Chavez, A F, Cheng, E J, Colwell, S J, Conard, M P, Conner, C A, Conrad, J C, Cook, S B, Cooper, O S, Custodio, C M, Dalle Ore, C C, Deboy, P, Dharmavaram, R D, Dhingra, G F, Dunn, A M, Earle, A F, Egan, J, Eisig, M R, El-Maarry, C, Engelbrecht, B L, Enke, C J, Ercol, E D, Fattig, C L, Ferrell, T J, Finley, J, Firer, J, Fischetti, W M, Folkner, M N, Fosbury, G H, Fountain, J M, Freeze, L, Gabasova, L S, Glaze, J L, Green, G A, Griffith, Y, Guo, M, Hahn, D W, Hals, D P, Hamilton, S A, Hamilton, J J, Hanley, A, Harch, K A, Harmon, H M, Hart, J, Hayes, C B, Hersman, M E, Hill, T A, Hill, J D, Hofgartner, M E, Holdridge, M, Horányi, A, Hosadurga, A D, Howard, C J A, Howett, S E, Jaskulek, D E, Jennings, J R, Jensen, M R, Jones, H K, Kang, D J, Katz, D E, Kaufmann, J J, Kavelaars, J T, Keane, G P, Keleher, M, Kinczyk, M C, Kochte, P, Kollmann, S M, Krimigis, G L, Kruizinga, D Y, Kusnierkiewicz, M S, Lahr, T R, Lauer, G B, Lawrence, J E, Lee, E J, Lessac-Chenen, I R, Linscott, C M, Lisse, A W, Lunsford, D M, Mages, V A, Mallder, N P, Martin, B H, May, D J, McComas, R L, McNutt, D S, Mehoke, T S, Mehoke, D S, Nelson, H D, Nguyen, J I, Núñez, A C, Ocampo, W M, Owen, G K, Oxton, A H, Parker, M, Pätzold, J Y, Pelgrift, F J, Pelletier, J P, Pineau, M R, Piquette, S B, Porter, S, Protopapa, E, Quirico, J A, Redfern, A L, Regiec, H J, Reitsema, D C, Reuter, D C, Richardson, J E, Riedel, M A, Ritterbush, S J, Robbins, D J, Rodgers, G D, Rogers, D M, Rose, P E, Rosendall, K D, Runyon, M G, Ryschkewitsch, M M, Saina, M J, Salinas, P M, Schenk, J R, Scherrer, W R, Schlei, B, Schmitt, D J, Schultz, D C, Schurr, F, Scipioni, R L, Sepan, R G, Shelton, M R, Showalter, M, Simon, K N, Singer, E W, Stahlheber, D R, Stanbridge, J A, Stansberry, A J, Steffl, D F, Strobel, M M, Stothoff, T, Stryk, J R, Stuart, M E, Summers, M B, Tapley, A, Taylor, H W, Taylor, R M, Tedford, H B, Throop, L S, Turner, O M, Umurhan, J, Van Eck, D, Velez, M H, Versteeg, M A, Vincent, R W, Webbert, S E, Weidner, G E, Weigle, J R, Wendel, O L, White, K E, Whittenburg, B G, Williams, K E, Williams, S P, Williams, H L, Winters, A M, Zangari, T H, Zurbuchen
Publikováno v:
Science (New York, N.Y.). 364(6441)
The Kuiper Belt is a distant region of the outer Solar System. On 1 January 2019, the New Horizons spacecraft flew close to (486958) 2014 MU
Autor:
S. M. Wahl, Jonathan I. Lunine, L. Gomez Casajus, Burkhard Militzer, Ryan S. Park, Andrea Milani, Dustin Buccino, William B. Hubbard, Paolo Tortora, Luciano Iess, Steven Levin, Marzia Parisi, Ravit Helled, Daniele Durante, Eli Galanti, Yamila Miguel, W. M. Folkner, Marco Zannoni, Scott Bolton, John D. Anderson, Daniele Serra, D. J. Stevenson, P. Racioppa, Tristan Guillot, Yohai Kaspi, Hao Cao, John E. P. Connerney
Publikováno v:
Nature
Nature, Nature Publishing Group, 2018, 555 (7695), pp.220-222. ⟨10.1038/nature25776⟩
Nature, Nature Publishing Group, 2018, 555 (7695), pp.220-222. ⟨10.1038/nature25776⟩
The gravity harmonics of a fluid, rotating planet can be decomposed into static components arising from solid-body rotation and dynamic components arising from flows. In the absence of internal dynamics, the gravity field is axially and hemispherical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0526681ebda67ed530b877795e0c8947
https://hal.univ-cotedazur.fr/hal-02528883
https://hal.univ-cotedazur.fr/hal-02528883
Autor:
S. Bhaskaran, W. M. Folkner, T. Joseph W. Lazio, J. A. Ellis, Curt Cutler, Michele Vallisneri, Ryan S. Park, Stephen Taylor, Todd A. Ely
In-spiraling supermassive black holes should emit gravitational waves, which would produce characteristic distortions in the time of arrival residuals from millisecond pulsars. Multiple national and regional consortia have constructed pulsar timing a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7822260d4fe627f4f0413c8d1b3600f5
Autor:
D. Serra, W. M. Folkner, L. Iess, J. D. Anderson, S. W. Asmar, D. R. Buccino, D. Durante, L. Gomez Casajus, M. Gregnanin, A. Milani, M. Parisi, G. Tommei, P. Tortora, M. Zannoni
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4094::4c014cfa64ce2564229f6e5ad563c7cd
http://hdl.handle.net/11585/613987
http://hdl.handle.net/11585/613987
Publikováno v:
Physical Review D. 89
The modified Newtonian dynamics (MOND) is an attempt to modify the gravitation theory to solve the dark matter problem. This phenomenology is very successful at the galactic level. The main effect produced by MOND in the Solar System is called the ex