On the formation of a sharp layer of metallic constituents at sunrise in the lower thermosphere

Springer Science and Business Media LLC - Tập 90 - Trang 141-146 - 1981
J S Shirke1, R Sridharan1, S P Gupta1, A D Danilov2, A A Pokhunkov2, V K Semenov2, V A Verfolomeev2
1Physical Research Laboratory, Ahmedabad, India
2Institute of Applied Geophysics, Moscow, USSR

Tóm tắt

Results are presented of two instrumented rocket experiments performed from an equatorial station, one at night and the other shortly after sunrise. The ion neutral composition as well as electron density and the amplitude of plasma irregularities were monitored. During the latter flight, a sharp layer of ionisation with its lower boundary at 100 km was observed. The layer had a half width close to 1 km and a peak electron density of 5·6× 104cm−3. Large amplitude of plasma irregularities, noticed on the negative gradient portion of the layer indicates a downward direction of the polarisation electric field during the observations. The resulting downward drift of photoions as they are produced at sunrise followed by the local decrease of the drift is suggested to be the cause of the layer formation at that altitude. The long lasting nature of such layers once identified on ionograms indicates that they are constituted of metallic ions possibly of micrometeoritic origin deposited overnight in the lower thermosphere. The required photoionisation rate of production of the metallic ions at sunris eis about 2 cm−3 sec−1.

Tài liệu tham khảo

Aikin A C and Goldberg R A 1973J. Geophys. Res. 78 734 Ananda Rao, Raghavendra Rao B R and Reddy C R 1977J. Geophys. Res. 82 1510 Anderson J G and Barth C A 1971J Geophys. Res. 76 3723 Balsley B B and Woodman R F 1969J. Atmos. Terr. Phys. 31 865 Danilov A D, Pokhunkov A A, Semenov V K, Vorfolomeev V A, Shirke J S, Sridharan ReGupta S P and Pradhan S N 1980Adv. Space Exploration Vol. 7 Low latitude Aeronomi, Processes P. 111 Hawkins G S 1956Mon. Not. R. Astron. Soc. 116 103 Istomin V G 1963Space Res. 3 209 Johannessen A and Krankowsky D 1972J. Geophys. Res. 77 2888 Lebedinets V N and Shushkova V B 1970Planet. Space Sci. 18 1653, 1659 Narcisi R S and Bailey A D 1965J. Geophys. Res. 70 3687 Narcisi R S 1968Space Res. 8 360 Prakash S and Pandey R 1979Proc. Indian Acad. Sci. (Earth Planet. Sci.) 88 229 Reid G C 1968J. Geophys. Res. 73 1627 Satya Prakash, Gupta S P and Subbaraya B H 1969Rad. Sci. 4 791 Satya Prakash and Subbaraya B H 1967Rev. Sci. Instrum. 38 1132 Shirke J S and Sridharan R 1967Proc. Indian Acad. Sci. (Earth Planet. Sci.) 88 219 Swider W Jr 1909Planet. Space Sci. 17 1233 Woodman R F 1979J. Geophys. Res. 75 6249 Young J M, Johnson C Y and Holmes J C 1967J. Geophys. Res. 72 1473 Zbinden P A, Hidalgo M A, Eberhardt P and Geiss J 1975Planet. Space Sci. 23 1621