Browsing by Author "Zweifel, Peter"
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- Some of the metrics are blocked by yourconsent settingsA Lunar Broad Band Seismometer on SELENE2 / LUNETTE missions: Focus on VBB technical improvements(2010)
;Nebut, T. ;Gagnepain-Beyneix, J. ;Lognonné, Philippe ;Kobayashi, Norihiko ;Giardini, D. ;Christensen, Ulrich R. ;Raucourt, s ;Bierwirth, M. ;Mimoun, David ;Zweifel, Peter ;Tillier, SylvainRobert, O. - Some of the metrics are blocked by yourconsent settingsLunar BroadBand Seismometer System in the Japanese lunar landing mission SELENE-2: its science goals and instrument details(2010)
;Shiraishi, Haruna ;Kobayashi, Norihiko ;Takeuchi, N. ;Murakami, H. ;Lognonné, Philippe ;Giardini, D. ;Christensen, Ulrich R. ;Okamoto, T. ;Kuge, K. ;Zhao, D. ;Mocquet, A. ;Mimoun, David ;Raucourt, s ;Nebut, T. ;Tillier, Sylvain ;Kawamura, T. ;Mance, Davor ;Zweifel, Peter ;Bierwirth, M.Yamada, I. - Some of the metrics are blocked by yourconsent settingsMOON SEIS: Design and Performances of a Very Broadband Seismometer for Future Lunar Missions(2010)
;Mimoun, David ;Lognonné, Philippe ;Giardini, D. ;Christensen, Ulrich R. ;Zweifel, Peter ;Mance, Davor ;Roll, R. ;Bierwirth, M. ;Raucourt, s ;Gagnepain-Beyneix, J. ;Tillier, SylvainNebut, T. - Some of the metrics are blocked by yourconsent settingsSEIS Experiment for the INSIGHT Mission: Towards 2018 Launch(2016)
;Verdier, Nicolas ;Lognonné, Philippe ;Banerdt, William ;Raucourt, s ;Ijpelaan, Frans ;Jerjean, L. ;Pont, Gabriel ;Sylvestre-Baron, A. ;Laudet, Philippe ;Bousquet, Pierre ;Hohhman, T. ;Umland, J. ;Bone, B. ;Hurst, Kenneth ;Giardini, D. ;Zweifel, Peter ;Bramanti, C. ;Pike, William ;Calcutt, SimonChristensen, Ulrich R.After giving an outline of the InSight mission, with a focus on SEIS activities on Mars, we will describe the SEIS instrument and its performances, and provide a status of its development at the time of the workshop. - Some of the metrics are blocked by yourconsent settingsThe ExoMars-Humbold Payload SEIS Experiment(2008)
;Mimoun, David ;Lognonné, Philippe ;Gagnepain-Beyneix, J. ;Giardini, D. ;Mance, Davor ;Zweifel, Peter ;Pike, T. ;Calcutt, Simon ;Christensen, Ulrich R. ;Roll, R. ;Berg, ArieSmit, Martijn - Some of the metrics are blocked by yourconsent settingsThe GEMS (GEophysical Monitoring Station) SEISmometer(2011)
;Lognonné, Philippe ;Banerdt, William ;Giardini, D. ;Christensen, Ulrich R. ;Pike, T. ;Mimoun, David ;Raucourt, s ;Tillier, Sylvain ;Zweifel, Peter ;Mance, Davor ;Roll, R. ;Bierwirth, M. ;Boschi, Lapo ;Garcia, R. ;Goetz, Walter ;Johnson, Chunteyell ;Kobayashi, Norihiko ;Mocquet, A. ;Panning, MarkWieczorek, Mark - Some of the metrics are blocked by yourconsent settingsThe INSIGHT SEIS VBB Experiment(2012)
;Tillier, Sylvain ;Raucourt, s ;Lognonné, Philippe ;Banerdt, William ;Mimoun, David ;Giardini, D. ;Christensen, Ulrich R. ;Pike, William ;Zweifel, Peter ;Mance, Davor ;Bierwirth, M. ;Laudet, Philippe ;Perez, R. ;Kerjean, Laurent ;Hurst, Kenneth ;Mocquet, A.Garcia, R. - Some of the metrics are blocked by yourconsent settingsThe SEIS InSight VBB Experiment(2013)
;Nebut, T. ;Lognonné, Philippe ;Banerdt, William ;Raucourt, s ;Beyneix, J. ;Dandonneau, P. ;Gabsi, Taoufik ;Robert, O. ;Tillier, Sylvain ;Hurst, Kenneth ;Mimoun, David ;Christensen, Ulrich R. ;Bierwierth, M. ;Roll, R. ;Pike, William ;Calcutt, Simon ;Giardini, D. ;Mance, Davor ;Zweifel, PeterPerez, R.Introduction: The SEIS experiment is the primary payload of the Interior Structure Investigation using Seismology and Heat Transport (InSight) mission selected by NASA in August 2012 to be the next Mars mission. The objective of the InSight SEIS experiment is the determination of the deep internal structure of Mars. In particular, geophysical parameters of first importance, such as the state (liquid/solid) and size of the core, structure of the mantle, shape of discontinui-ties and thickness of the crust will be determined by the experiment. It will measure seismic activity over a very broad frequency band, from tidal frequencies (0.05 mHz) up to high frequencies (50 Hz), to address a wide range of scientific questions, from the state of the core to the meteoritic impact rate, marsquake rate and the response of the planet to the Phobos tide. Description of the instrument: The instrument includes notably a Very Broad Band (VBB) 3 axis seis-mometer which is developed by the ';Institut du Globe de Paris' (IPGP) under the funding of CNES. The sensor assembly, which also contains a MEMS short-period seismometer, will be deployed on the Martian ground by a robotic arm from a Phoenix-type lander platform and will be protected by a wind and thermal shield. The wind and thermal shield,together with a vacuum sphere and a passive compensation system will achieve a very high protection of the VBB against temperature and pressure variations, allowing the sensor to operate in the rough Martian thermal environment while reaching a detection threshold below 10-9 ms-2 Hz-1/2 in the VBB bandwidth. Conclusion: Performance has been demonstrated with previous prototypes and the SEIS experiment of the InSight mission will therefore provide high-quality seismic signal acquisition and associated seismic information during one martian year. The delivery of the payload is planned for the end of 2014 and the launch is in March 2016 SEIS deployed on the ground next to the lander