During the first 35 close Titan flybys the Radio and Plasma Wave Science instrument (RPWS) aboard the CASSINI orbiter did not observe radio signals possibly associated with lightning in the atmosphere of Titan [Fischer et al., 2007, Geophys. Res. Lett., 34, L22104). The electric field sensors of the HUYGENS PWA instrument (permittivity, waves and altimetry) observed smooth variations as well as impulsive events varying with altitude during the descent of the probe in the atmosphere of Titan. While a part of the low frequency signals was explained as externally driven Schumann resonances, there is still a debate on the origin of the impulsive events. In order to differentiate natural atmospheric discharges from sources on the parachute or th...
International audienceDuring the Cassini-Huygens probe mission at Titan on 14th January 2005, The Hu...
The Huygens Atmospheric Structure Instrument (HASI) is a multi sensor package which has been designe...
International audienceAfter the confirmed absence of any detectable lightning activity in Titan’s at...
During the first 35 close Titan flybys the Radio and Plasma Wave Science instrument (RPWS) aboard th...
International audienceThis study presents an approximate model for the atypical Schumann resonance i...
After a preliminary analysis of the low-frequency data collected with the electric antenna of the Pe...
International audienceThe low-frequency data collected with the antenna of the Permittivity, Wave an...
The permittivity, waves and altimetry (PWA) instrument was designed for the investigation of the ele...
International audienceThe descent of the Huygens Probe through the atmosphere of Titan provided info...
International audienceWe report on the nondetection of radio emissions associated with possible ligh...
International audienceExtremely Low Frequency (ELF) electric field signals recorded by the Huygens p...
International audienceAfter five years of thorough analysis of data from the Huygens Probe that desc...
International audienceDuring the Cassini-Huygens probe mission at Titan on 14th January 2005, The Hu...
The Huygens Atmospheric Structure Instrument (HASI) is a multi sensor package which has been designe...
International audienceAfter the confirmed absence of any detectable lightning activity in Titan’s at...
During the first 35 close Titan flybys the Radio and Plasma Wave Science instrument (RPWS) aboard th...
International audienceThis study presents an approximate model for the atypical Schumann resonance i...
After a preliminary analysis of the low-frequency data collected with the electric antenna of the Pe...
International audienceThe low-frequency data collected with the antenna of the Permittivity, Wave an...
The permittivity, waves and altimetry (PWA) instrument was designed for the investigation of the ele...
International audienceThe descent of the Huygens Probe through the atmosphere of Titan provided info...
International audienceWe report on the nondetection of radio emissions associated with possible ligh...
International audienceExtremely Low Frequency (ELF) electric field signals recorded by the Huygens p...
International audienceAfter five years of thorough analysis of data from the Huygens Probe that desc...
International audienceDuring the Cassini-Huygens probe mission at Titan on 14th January 2005, The Hu...
The Huygens Atmospheric Structure Instrument (HASI) is a multi sensor package which has been designe...
International audienceAfter the confirmed absence of any detectable lightning activity in Titan’s at...