HR: 1340h
AN: P33C-0255 [Abstracts]
TI: Preliminary Analysis of the Extremely Low Frequency Signals Detected With the PWA-HASI Instrument
During the Descent of the Huygens Probe Through the Atmosphere of Titan
AU: * Simoes, F
EM: fernando.simoes@cetp.ipsl.fr
AF: Centre d'etude des Environments Terrestre et Plan‚taires (CETP), CNRS, 4, Avenue de Neptune, Saint Maur
Cedex, F-94107
France
AU: Brown, V
P33C-0255
AF: Instituto de Astrofisica de Andalucia (IAA), CSIC, P.O. Box 3004, Granada, E-18080
Spain
AU: Chabassiere, M
P33C-0255
AF: Laboratoire de Physique et Chimie de l'Environnement (LPCE), CNRS, 3A Avenue de la Recherche
Scientifique, Cedex, Orleans, F-45071
France
AU: Falkner, P
P33C-0255
AF: Science Payload and Advanced Concepts Office, ESA/ESTEC, Keplerlaan 1, Noordwijk, 2200
Netherlands
AU: Ferri, F
P33C-0255
AF: Centro Interdipartimentale Studi ed Attivit… Spaziali 'G. Colombo', Via Venezia 15, Padova, 35131
Italy
AU: Fulchignoni, M
P33C-0255
AF: Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique (LESIA), Observatoire de Paris -
Meudon, 5, place Jules Janssen, cedex, Meudon, F-92195
France
AU: Grard, R
P33C-0255
AF: Research and Scientific Support Department (RSSD), ESA/ESTEC, Keplerlaan 1, Noordwijk, 2200
Netherlands
AU: Hamelin, M
P33C-0255
AF: Centre d'etude des Environments Terrestre et Plan‚taires (CETP), CNRS, 4, Avenue de Neptune, Saint Maur
Cedex, F-94107
France
AU: Hofe, R
P33C-0255
AF: Institut fur Weltraumforschung (IWF), Austrian Academy of Sciences, Schmiedlstrasse 6, Graz, A-8042
Austria
AU: Jernej, I
P33C-0255
AF: Institut fur Weltraumforschung (IWF), Austrian Academy of Sciences, Schmiedlstrasse 6, Graz, A-8042
Austria
AU: Lara, L
P33C-0255
AF: Instituto de Astrofisica de Andalucia (IAA), CSIC, P.O. Box 3004, Granada, E-18080
Spain
AU: Lopez-Moreno, J
P33C-0255
AF: Instituto de Astrofisica de Andalucia (IAA), CSIC, P.O. Box 3004, Granada, E-18080
Spain
AU: Molina-Cuberos, G
P33C-0255
AF: Dpto. Fisica, Facultad de Quimicas, Universidad de Murcia, Murcia, 30100
Spain
AU: Rodrigo, R
P33C-0255
AF: Instituto de Astrofisica de Andalucia (IAA), CSIC, P.O. Box 3004, Granada, E-18080
Spain
AU: Schwingenschuh, K
P33C-0255
AF: Institut fur Weltraumforschung (IWF), Austrian Academy of Sciences, Schmiedlstrasse 6, Graz, A-8042
Austria
AU: Trautner, R
P33C-0255
AF: Research and Scientific Support Department (RSSD), ESA/ESTEC, Keplerlaan 1, Noordwijk, 2200
Netherlands
AB:
The Permittivity, Waves, and Altimetry (PWA) analyzer is a subsystem of the Huygens Atmospheric Structure Instrument (HASI),
onboard the Huygens Probe. Dedicated to the study of electric phenomena, the PWA instrument measured the electric field in
the bandwidth 0-10kHz, during the descent of the Probe through the atmosphere of Titan. A distinctive electric signal is
observed at around 36Hz, which may provide information about wave activity in the atmosphere. We present several hypotheses
about the nature of this signal, related to natural phenomena taking place in the environment of Titan. It is not believed
that the emission at 36Hz is induced by other instruments, the parachutes, or the Probe body. We tentatively assume that this
signal is similar to the Schumann resonance observed on Earth, and we test the validity of the data set against the results
from a model of the resonance of Titan's ionospheric cavity.
DE: 5405 Atmospheres (0343, 1060)
DE: 5435 Ionospheres (2459)
DE: 5494 Instruments and techniques
DE: 6281 Titan
DE: 6929 Ionospheric physics (1240, 2400)
SC: Planetary Sciences [P]
MN: Fall Meeting 2005