Characteristics of Fe ablation trails observed during the 1998 Leonid meteor shower

被引:22
作者
Chu, XZ
Pan, WL
Papen, G
Gardner, CS
Swenson, G
Jenniskens, P
机构
[1] Univ Illinois, Dept Elect & Comp Engn, Urbana, IL 61801 USA
[2] NASA, Ames Res Ctr, SETI Inst, Moffett Field, CA 94035 USA
关键词
D O I
10.1029/1999GL010756
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Eighteen Fe ablation trails were observed during the 17/18 Nov 1998 Leonid meteor shower with an airborne Fe lidar aboard the NSF/NCAR Electra aircraft over Okinawa. The average altitude of the 18 trails from the high velocity (72 km/s) Leonid meteors, 95.67+/-0.93 km, is approximately 6.7 km higher than previously observed for slower (similar to 30 km/s) sporadic meteors. This height difference is consistent with the assumption that meteors ablate when atmospheric drag reaches a critical threshold. The average age of the Fe trails, determined by a diffusion model, is 10.1 min. The youngest ages were observed below 92 km and above 98 km where chemistry and diffusion dominate, respectively. The average abundance of the trails is 10% of the abundance of the background Fe layer. Observations suggest that the 1998 Leonid shower did not have a significant impact on the abundance of the background Fe layer.
引用
收藏
页码:1807 / 1810
页数:4
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