Lundin R, Winningham D, Barabash S, Frahm R, Holmström M, Sauvaud J-A, Fedorov A, Asamura K, Coates A J, Soobiah Y, Hsieh K C, Grande M, Koskinen H, Kallio E, Kozyra J, Woch J, Fraenz M, Brain D, Luhmann J, McKenna-Lawler S, Orsini R S, Brandt P, Wurz P
Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden.
Science. 2006 Feb 17;311(5763):980-3. doi: 10.1126/science.1122071.
Auroras are caused by accelerated charged particles precipitating along magnetic field lines into a planetary atmosphere, the auroral brightness being roughly proportional to the precipitating particle energy flux. The Analyzer of Space Plasma and Energetic Atoms experiment on the Mars Express spacecraft has made a detailed study of acceleration processes on the nightside of Mars. We observed accelerated electrons and ions in the deep nightside high-altitude region of Mars that map geographically to interface/cleft regions associated with martian crustal magnetization regions. By integrating electron and ion acceleration energy down to the upper atmosphere, we saw energy fluxes in the range of 1 to 50 milliwatts per square meter per second. These conditions are similar to those producing bright discrete auroras above Earth. Discrete auroras at Mars are therefore expected to be associated with plasma acceleration in diverging magnetic flux tubes above crustal magnetization regions, the auroras being distributed geographically in a complex pattern by the many multipole magnetic field lines extending into space.
极光由沿磁场线加速的带电粒子沉淀到行星大气层中引起,极光亮度大致与沉淀粒子的能量通量成正比。火星快车号航天器上的空间等离子体和高能原子分析仪实验对火星夜侧的加速过程进行了详细研究。我们在火星夜侧深处的高空区域观测到加速的电子和离子,这些区域在地理上对应于与火星地壳磁化区域相关的界面/裂隙区域。通过将电子和离子加速能量积分到高层大气,我们看到能量通量在每秒每平方米1至50毫瓦的范围内。这些条件与在地球上方产生明亮离散极光的条件相似。因此,预计火星上的离散极光与地壳磁化区域上方发散磁通量管中的等离子体加速有关,极光通过延伸到太空的许多多极磁场线以复杂的模式在地理上分布。