Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Leigh N. Fletcher"'
Autor:
Shawn P. Ewald, R. K. Achterberg, R. W. Schmude, Liming Li, Kevin H. Baines, Robert A. West, J. J. Fortney, G. S. Orton, Peter J. Gierasch, Agustín Sánchez-Lavega, B. Knowles, Conor A. Nixon, Santiago Pérez-Hoyos, Patrick M. Fry, A. Mallama, Ulyana A. Dyudina, Leigh N. Fletcher, Carolyn C. Porco, Xun Jiang, Amy Simon
Publikováno v:
Nature communications, vol 9, iss 1
Nature Communications, Vol 9, Iss 1, Pp 1-10 (2018)
Nature Communications
Nature Communications, Vol 9, Iss 1, Pp 1-10 (2018)
Nature Communications
The radiant energy budget and internal heat are fundamental properties of giant planets, but precise determination of these properties remains a challenge. Here, we report measurements of Jupiter’s radiant energy budget and internal heat based on C
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2497cb07f9a02143f678edf79507b97f
https://resolver.caltech.edu/CaltechAUTHORS:20180917-125104391
https://resolver.caltech.edu/CaltechAUTHORS:20180917-125104391
Autor:
Conor A. Nixon, Kevin H. Baines, Richard K. Achterberg, Andrew P. Ingersoll, Liming Li, Leigh N. Fletcher, Peter J. Gierasch, Carolyn C. Porco, Anthony D. Del Genio, Amy A. Simon-Miller, Barney J. Conrath, Ashwin Vasavada, Glenn S. Orton, Shawn P. Ewald, Xun Jiang, Robert A. West
The zonal jets on the giant planets have been thought to be stable in time1-3. A decline in the velocity of Saturn's equatorial jet has been identified, on the basis of a comparison of cloud-tracking data across two decades4, but the differences in c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d00c1534c72ddfc2a8887da23d82c6d9
https://resolver.caltech.edu/CaltechAUTHORS:20111207-143142776
https://resolver.caltech.edu/CaltechAUTHORS:20111207-143142776