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Laboratory Experiments for Studying the Emission of Nitrogen and Air Andreas Ulrich, Andrei Morozov Technische Universität München Fakultät für Physik E12 4th Air Fluorescence Workshop May 17-20, 2006, Prague - Pruhonice. Excitation of dense gases with low energy electron beams
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Laboratory Experiments for Studying the Emission of Nitrogen and Air Andreas Ulrich, Andrei Morozov Technische Universität München Fakultät für Physik E12 4th Air Fluorescence Workshop May 17-20, 2006, Prague - Pruhonice
Excitation of dense gases with low energy electron beams • Shape of the excited volume • Correlation of quenching rate constants k and p‘ values • Intensity ratios of N2 emission bands (experiments in Chicago and Garching) • Improvements
I) Excitation of dense gases with low energy electron beams Typical parameters: Electron energy: 15 keV Beam current: 10 μA average Pulses: 5 ns minimum Gas pressure: 0.1 – 2 bar Membrane: 300 nm SiNx
Motivation for using low energy electrons for N2 emission studies: High fluorescence yield at low energy Copied from DPG-presentation 2006: Andreas Obermeier
II) Shape of the excited volume The shape can be modelled using the program: „casino“ (P. Drouin, A. R. Couture, R. Gauvin, P. Hovington, P. Horny, H. Demers, Univ. de Sherbrooke, Quebec, Canada (2002)) This will be important for absolute emission measurements using low energy electron beams!
III) Correlation of quenching rate constants k and p‘ values Rprod. τ0 τc
The two approaches: time spectra pressure dependence Nagano et al. astro-ph/0303193 v3 26 Aug. 2003 the connection
Example: N2 2P-Band, v=0 and v=1, 337 and 316nm τ0 = 41.7ns (for both v) kq = 1.2×10-11 cm3/s and kq = 2.5×10-11 cm3/s, respectively Results in p‘ = 74.6 hPa and p‘ = 35.8 hPa, respectively (10% error) Morozov et al. Eur. Phys. J. D 33, 207 (2005) In contrast to: p‘ = 151.7 hPa and p‘ = 88.3 hPa, respectively (10% error) Nagano et al. astro-ph/0303193 v3 26 Aug. 2003 ?
Potential reasons for the discrepancy: Systematic errors ? Collisional mixing of the vibrational levels ? See: J. M. Calo and R. C. Axtmann, J. Chem. Phys. 54, 1332 (1971) C, v=0, 1 Non radiative quenching Collisional quenching of v – levels by N2 Radiative transition B, v=0, 1, etc. A model worked out by Andrei Morozov showed an increase of the p‘ value for the 337nm (v‘=0 to v=0) transition from 79.36 to 91.95 hPa using the data given in the publication by Calo and Axtmann. (I(p) modelled with and without coll. quenching of v levels and then fit using the regular formular.)
n=1 Q1p v=0 τ0 Q1p τ1 Q1dp
First test of the influence of vibrational relaxation via collisions: Classical model, new model with vibrational relaxation, data from new model fit with classical model
Intensity ratios of nitrogen emission bands Spectral response of McPherson 218. Preliminary measurements: Black: W Strip-lamp Blue: W Strip- lamp + UG11 Red: D2 Lamp
Spectral response of the „Rome“ spectrometer Measured with a calib. halogen and a Hg pen-ray lamp, respectively
Spectrum of air recorded using electron beam excitation, McPherson model 218 VUV monochromator and photon counting:
Comparison of spectra of laboratory air excited by 10 keV photons (photoelectrons) and 10 keV electrons (APS Chicago and e- beam Graching)
Comparison of spectra of laboratory air excited by 10 keV photons (photoelectrons) and 10 keV electrons (APS Chicago and e- beam Graching) Detail:
Comparison of the weakest and strongest lines analysed (Garching data):
Relative intensities of N2 emission bands: Comparison of Chicago and Garching data with literature values
Relative intensities of N2 emission bands: Comparison of Chicago and Garching data with literature values Log – scale:
Analysis of the same Garching- data, two persons independently
Improvements: We have bought a 100 W calibrated halogen lamp (LOT / Heraeus) We will borrow a new calibrated D2 from GSI-Darmstadt (Plasma physics group) Measurements of the absolute photon flux will be performed Pressure dependences should be measured for the ~10 keV electrons Acknowledgement ! Many thanks to Paolo Privitera, Hans Klages and all their coworkers for inviting me to participate in the Chicago experiment and KfA-Karlsruhe for paying for the trip. Thanks to Reiner Krücken and MLL for supporting my trip to this conference. I want to thank Jochen Wieser (TuiLaser/Coherent) for his help with the experiments and the apparatus, in particular the very stable power supply. Thank you for your attention