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  Poster Programme - PS9 Space simulations in laboratory: experiments, instrumentation and modelling

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Convener: Colangeli, L.
Co-Convener: Seiferlin, K., Sears, D.
Co-Sponsorship:


Author in Attendance:

Monday, 25 April 2005 08:30 - 10:00
Display Time: Monday, 25 April 2005 08:00 -
Monday, 25 April 2005 19:00
Poster Area: Hall X

Chairperson: N.N.

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X390
EGU05-A-05077;  PS9-1MO1P-0390
Richterova, I.; Nemecek, Z.; Safrankova, J.
The model and experiment of secondary emission from dust grains

X391
EGU05-A-05098;  PS9-1MO1P-0391
Pavlu, J.; Richterova, I.; Safrankova, J. ; Nemecek, Z.
Ion and electron emission from dust grains: Laboratory simulation

X392
EGU05-A-05860;  PS9-1MO1P-0392
Smythe, W. D.; Nelson, R. M.; Hapke, B. W.; Manatt, K. S.; Eddy, J.
Advances in Instrumental Techniques for Investigating Planetary Regolith Microstructure

X393
EGU05-A-06108;  PS9-1MO1P-0393
Yamada, M.; Tachibana, S.; Nagahara, H.; Ozawa, K.
Anisotropy of Mg isotopic fractionation and Mg lattice diffusion during evaporation of forsterite in vacuum

X394
EGU05-A-06517;  PS9-1MO1P-0394
Gunderson, K.; Thomas, N.; Whitby, J.
First measurements with the Physikalisches Institut Radiometric Experiment (PHIRE)

X395
EGU05-A-06932;  PS9-1MO1P-0395
Witzke, A.; Arnold, G.; Stöffler, D.
Detectibility of Ca- and Mg-sulfates in the spectra of Martian soils

X396
EGU05-A-03551;  PS9-1MO1P-0396
Ziethe, R.; Whitby, J. A.; Benz, W.
Computational Fluid Dynamics vs. Laboratory Experiments

X397
EGU05-A-03572;  PS9-1MO1P-0397
Molina, A.; Moreno, F.; Muñoz, O.; Guirado, D.; Girela, F.; López, A.; Ramos, J.L.; Costillo, L.P.
A new light scattering laboratory at the Instituto de Astrofísica de Andalucía in Granada, Spain.

X398
EGU05-A-08053;  PS9-1MO1P-0398
Cernogora, G.; Szopa, C.; Boufendi, L.; Jolly, A.
Laboratory simulation of Titan’s atmosphere chemistry by RF plasma: plasma properties determined with optical emission spectroscopy

X399
EGU05-A-10495;  PS9-1MO1P-0399
Ardalan, A.; Silavi, T.
New estimations for the radius of Geo-stationary satellite orbit based on spherical and ellipsoidal models




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