Mesospheric observations by a forward scattering meteor radar basic setup

Author:

Madkour Waleed,Yamamoto Masa-yuki

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference16 articles.

1. Baggaley, W.J.: The interpretation of overdense radio meteor echo duration characteristics. Bull. Astron. Inst. Czechoslov. 30, 184–189 (1979)

2. Baggaley, W.J., Cummack, C.H.: Meteor train ion chemistry. J. Atmos. Terr. Phys. 36, 1759 (1974)

3. Carbognani, A., De Meyere, M., Foschini, L., Steyaert, C.: On the meteor height from forward scatter radio observations. Astron. Astrophys. 361, 293 (2001)

4. Ceplecha, Z., Borovička, J., Elford, W.G., ReVelle, D.O., Hawkes, R.L., Porubčan, V., Šimek, M.: Meteor phenomena and bodies. Space Sci. Rev. 84(3–4), 327–471 (1998)

5. Davis, J.A., Greenhow, J.S., Hall, J.E.: The effect of attachment on radio echo observations of meteors. Proc. R. Soc. Lond. Ser. A, Math. Phys. Sci. 253(1272), 130–139 (1959)

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