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Lyman-alpha Detecto...
Lyman-alpha Detector Designed for Rocket Measurements of the Direct Solar Radiation at 121.5 nm
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Guineva, V (författare)
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Witt, Georg (författare)
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- Gumbel, Jörg (författare)
- Stockholms universitet,Meteorologiska institutionen (MISU)
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visa fler...
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- Khaplanov, Mikhail (författare)
- Stockholms universitet,Meteorologiska institutionen (MISU)
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Werner, R (författare)
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- Hedin, Jonas (författare)
- Stockholms universitet,Meteorologiska institutionen (MISU)
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Neichev, S (författare)
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Kirov, B (författare)
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Bankov, L (författare)
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Gramatikov, P (författare)
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Tashev, V (författare)
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Popov, M (författare)
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Hauglund, K (författare)
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Hansen, G (författare)
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Ilstad, J (författare)
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Wold, H (författare)
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visa färre...
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(creator_code:org_t)
- 2007
- 2007
- Engelska.
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Ingår i: Bulgarian Journal of Physics. - 1310-0157 .- 1314-2666. ; 34:2, s. 116-127
- Relaterad länk:
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https://urn.kb.se/re...
Abstract
Ämnesord
Stäng
- Rocket measurements of the direct Lyman-alpha radiation penetrating 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 circumstance, 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 Lyman-alpha extinction in the atmosphere is a measure for the column density of the oxygen molecules, the atmospheric temperature profile can be calculated thereof. The detector of solar Lyman-alpha radiation was manufactured in the Stara Zagora Department of the Solar-Terrestrial Influences Laboratory (STIL). Its basic part is an ionization chamber, filled in with NO. A 60 V power supply is applied to the chamber. The produced photoelectric current from the sensor is fed to a 2-channels amplifier, providing an analog signal. The characteristics of the Lyman-alpha detector were studied. It passed successfully all tests and the results showed that the instrument could be used in rocket experiments to measure the Lyman-alpha flux. From the measurements of the detector, the Lyman-alpha vertical profile can be obtained. The forthcoming scientific data analysis will include radiative transfer simulations, O2 density, atmospheric power and temperature profiles retrieval as well as comparison with other parameters, measured near the polar summer mesopause and study of the processes in this region.
Ämnesord
- NATURVETENSKAP -- Geovetenskap och miljövetenskap -- Meteorologi och atmosfärforskning (hsv//swe)
- NATURAL SCIENCES -- Earth and Related Environmental Sciences -- Meteorology and Atmospheric Sciences (hsv//eng)
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- Av författaren/redakt...
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Guineva, V
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Witt, Georg
-
Gumbel, Jörg
-
Khaplanov, Mikha ...
-
Werner, R
-
Hedin, Jonas
-
visa fler...
-
Neichev, S
-
Kirov, B
-
Bankov, L
-
Gramatikov, P
-
Tashev, V
-
Popov, M
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Hauglund, K
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Hansen, G
-
Ilstad, J
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Wold, H
-
visa färre...
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Stockholms universitet