Add to ORKGSeismic experiments on future Mars exploration missions, and the instrumentation required for their performances are reported. Advances in microcomputer techniques of which have made feasible the processing of data prior to transmission to earth are discussed along with experience with the Viking hardware and software as related to future experiments. Sensor techniques are briefly mentioned
By the end of 2018, 42 years after the landing of the two Viking seismometers on Mars, InSight will ...
A seismic network on Mars should have enough stations (e.g., 24) to characterize the seismicity of t...
We carried out three geophysical experiments in Mars analog environments in order to better understa...
Efforts were made to determine the seismicity of Mars as well as define its internal structure by de...
A three-axis short-period seismometer has been operating on the surface of Mars in the Utopia Planit...
Little is known of the internal structure or composition of Mars or the present rates and characteri...
By the end of 2018, 42 years after the landing of the two Viking seismometers on Mars, InSight will ...
It is proposed to soft-land three seismometers in the Utopia-Elysium region and three or more radio ...
A three-axis short-period seismometer is now operating on Mars in the Utopia Planitia region. The no...
Following a brief overview of the mission concepts for a Mars Global Network Mission as of the time ...
By the end of 2018, 42 years after the landing of the two Viking seismometers on Mars, InSight will ...
International audienceBy the end of 2018, 42 years after the landing of the two Viking seismometers ...
By the end of 2018, 42 years after the landing of the two Viking seismometers on Mars, InSight will ...
A seismic network on Mars should have enough stations (e.g., 24) to characterize the seismicity of t...
We carried out three geophysical experiments in Mars analog environments in order to better understa...
Efforts were made to determine the seismicity of Mars as well as define its internal structure by de...
A three-axis short-period seismometer has been operating on the surface of Mars in the Utopia Planit...
Little is known of the internal structure or composition of Mars or the present rates and characteri...
By the end of 2018, 42 years after the landing of the two Viking seismometers on Mars, InSight will ...
It is proposed to soft-land three seismometers in the Utopia-Elysium region and three or more radio ...
A three-axis short-period seismometer is now operating on Mars in the Utopia Planitia region. The no...
Following a brief overview of the mission concepts for a Mars Global Network Mission as of the time ...
By the end of 2018, 42 years after the landing of the two Viking seismometers on Mars, InSight will ...
International audienceBy the end of 2018, 42 years after the landing of the two Viking seismometers ...
By the end of 2018, 42 years after the landing of the two Viking seismometers on Mars, InSight will ...
A seismic network on Mars should have enough stations (e.g., 24) to characterize the seismicity of t...
We carried out three geophysical experiments in Mars analog environments in order to better understa...