A combined rocket-borne and ground-based study of the sodium layer and charged dust in the upper mesosphere

被引:30
作者
Plane, John M. C. [1 ]
Saunders, Russell W.
Hedin, Jonas
Stegman, Jacek
Khaplanov, Misha
Gumbel, Jorg
Lynch, Kristina A.
Bracikowski, Phillip J.
Gelinas, Lynette J.
Friedrich, Martin
Blindheim, Sandra
Gausa, Michael
Williams, Bifford P.
机构
[1] Univ Leeds, Sch Chem, Leeds LS2 9JT, W Yorkshire, England
[2] Stockholm Univ, MISU, Stockholm, Sweden
[3] Dartmouth Coll, Dept Phys, Hanover, NH USA
[4] Aerosp Corp, Los Angeles, CA 90009 USA
[5] Graz Univ Technol, Graz, Austria
[6] GATS Inc, Boulder, CO USA
基金
欧洲研究理事会; 美国国家科学基金会;
关键词
Na layer; Charged dust; Meteoric smoke; Meteoric ablation; METEORIC SMOKE PARTICLES; ELECTRON-DENSITY; ATOMIC OXYGEN; NA LAYER; CHEMISTRY; TEMPERATURE; MODEL; O-2; CO2; CONSTRAINTS;
D O I
10.1016/j.jastp.2013.11.008
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The Hotel Payload 2 rocket was launched on January 31st 2008 at 20.14 LT from the Andoya Rocket Range in northern Norway (69.31 degrees N, 16.01 degrees E). Measurements in the 75-105 km region of atomic O, negatively-charged dust, positive ions and electrons with a suite of instruments on the payload were complemented by lidar measurements of atomic Na and temperature from the nearby ALOMAR observatory. The payload passed within 2.58 km of the lidar at an altitude of 90 km. A series of coupled models is used to explore the observations, leading to two significant conclusions. First, the atomic Na layer and the vertical profiles of negatively-charged dust (assumed to be meteoric smoke particles), electrons and positive ions, can be modelled using a self-consistent meteoric input flux. Second, electronic structure calculations and Rice-Ramsperger-Kassel-Markus theory are used to show that even small Fe-Mg-silicates are able to attach electrons rapidly and form stable negatively-charged particles, compared with electron attachment to O-2 and O-3. This explains the substantial electron depletion between 80 and 90 km, where the presence of atomic O at concentrations in excess of 10(10) cm(-3) prevents the formation of stable negative ions. (C) 2013 Elsevier Ltd. All rights reserved.
引用
收藏
页码:151 / 160
页数:10
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