Lyman-alpha Detector Designed for Rocket Measurements of the Direct Solar Radiation at 121.5 nm

• Main Authors: V. Guineva, G. Witt, J. Gumbel, M. Khaplanov, R. Werner, J. Hedin, S. Neichev, B. Kirov, L. Bankov, P. Gramatikov, V. Tashev, M. Popov, K. Hauglund, G. Hansen, J. Ilstad, H. Wold
• Other Authors: The Pennsylvania State University CiteSeerX Archives
• Format: Text
• Language: English
• Published: 2007
• Subjects: Andøya; Norway
• Online Access: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.555.3096; http://www.bjp-bg.com/papers/bjp2007_2_116-127.pdf

Abstract. Rocket measurements of the direct Lyman-alpha radiation penetrat-ing in the atmosphere were planned during the HotPay I rocket experiment, June 2006, Project ASLAF (Attenuation of the Solar Lyman-Alpha Flux), Andøya Rocket Range (ARR), Norway. The basic goal of ASLAF project was the study of the processes in the summer mesosphere and thermosphere (up to 110 km), at high latitudes using the Lyman-alpha measurements. The resonance transition 2P-2S of the atomic hydrogen (Lyman-alpha emission) is the strongest and most conspicuous feature in the solar EUV spectrum. Due to the favorable circum-stance, that the Lyman-alpha wavelength (121.5 nm) coincides with a minimum of the O2 absorption spectrum, the direct Lyman-alpha radiation penetrates well in the mesosphere. The Lyman-alpha radiation is the basic agent of the NO molecules ionization, thus generating the ionospheric D-layer, and of the water vapour photolysis, being one of the main H2O loss processes. The Lyman-alpha radiation transfer depends on the resonance scattering from the hydrogen atoms in the atmosphere and on the O2 absorption. Since the