Polar lightning and decadal-scale cloud variability on Jupiter

被引:47
作者
Baines, Kevin H.
Simon-Miller, Amy A.
Orton, Glenn S.
Weaver, Harold A.
Lunsford, Allen
Momary, Thomas W.
Spencer, John
Cheng, Andrew F.
Reuter, Dennis C.
Jennings, Donald E.
Gladstone, G. R.
Moore, Jeffrey
Stern, S. Alan
Young, Leslie A.
Throop, Henry
Yanamandra-Fisher, Padma
Fisher, Brendan M.
Hora, Joseph
Ressler, Michael E.
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[4] SW Res Inst, Boulder, CO 80302 USA
[5] SW Res Inst, San Antonio, TX 78238 USA
[6] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[7] NASA Headquarters, Sci Mission Directorate, Washington, DC 20546 USA
[8] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
D O I
10.1126/science.1147912
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Although lightning has been seen on other planets, including Jupiter, polar lightning has been known only on Earth. Optical observations from the New Horizons spacecraft have identified lightning at high latitudes above Jupiter up to 80 degrees N and 74 degrees S. Lightning rates and optical powers were similar at each pole, and the mean optical flux is comparable to that at nonpolar latitudes, which is consistent with the notion that internal heat is the main driver of convection. Both near-infrared and ground-based 5-micrometer thermal imagery reveal that cloud cover has thinned substantially since the 2000 Cassini flyby, particularly in the turbulent wake of the Great Red Spot and in the southern half of the equatorial region, demonstrating that vertical dynamical processes are time-varying on seasonal scales at mid-and low latitudes on Jupiter.
引用
收藏
页码:226 / 229
页数:4
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