Javascript must be enabled to continue!
Brownian Noise and Temperature Sensitivity of Long-Period Lunar Seismometers
View through CrossRef
ABSTRACT
As long-period ground motion holds the key to understanding the interior of the Earth’s Moon, reducing long-period noise sources will be an essential area of focus in the design of future lunar seismometers. For the proposed Lunar Geophysical Network (LGN), the International Lunar Network (ILN) Science Definition Team specifies that an LGN enabling seismometer will need to be more sensitive than any previous seismometer at frequencies below 1 Hz. In an effort toward lowering the seismometer noise floor for lunar geophysical missions, we evaluate the 1/f Brownian noise and the temperature sensitivity of a seismometer. Temperature sensitivity of a seismometer is related to an important component of the seismometer output noise that is proportional to the temperature noise in the environment. The implications of the ILN requirement are presented in the context of the state-of-the-art InSight Seismic Experiment for Interior Structure (SEIS) Very Broad Band (VBB) planetary seismometer. Brownian noise due to internal friction was estimated for future lunar operation after accounting for the rebalance of the product of mass and distance to the center of gravity of the pendulum for the SEIS-VBB sensor. We find that Brownian noise could be a limiting factor in meeting the ILN requirement for lunar seismometers. Further, we have developed a formalism to understand the temperature sensitivity of a seismometer, relating it quantitatively to the local gravity, the thermoelastic coefficient of the spring, change in center of gravity, and the coefficient of thermal expansion of the mechanical structures. We found that in general the temperature sensitivity of a seismometer is proportional to the local gravity, and so the temperature sensitivity can be reduced when operating on a planetary body with lower gravity. Our Brownian noise and temperature sensitivity models will be useful in the design of the next generation of planetary seismometers.
Seismological Society of America (SSA)
Title: Brownian Noise and Temperature Sensitivity of Long-Period Lunar Seismometers
Description:
ABSTRACT
As long-period ground motion holds the key to understanding the interior of the Earth’s Moon, reducing long-period noise sources will be an essential area of focus in the design of future lunar seismometers.
For the proposed Lunar Geophysical Network (LGN), the International Lunar Network (ILN) Science Definition Team specifies that an LGN enabling seismometer will need to be more sensitive than any previous seismometer at frequencies below 1 Hz.
In an effort toward lowering the seismometer noise floor for lunar geophysical missions, we evaluate the 1/f Brownian noise and the temperature sensitivity of a seismometer.
Temperature sensitivity of a seismometer is related to an important component of the seismometer output noise that is proportional to the temperature noise in the environment.
The implications of the ILN requirement are presented in the context of the state-of-the-art InSight Seismic Experiment for Interior Structure (SEIS) Very Broad Band (VBB) planetary seismometer.
Brownian noise due to internal friction was estimated for future lunar operation after accounting for the rebalance of the product of mass and distance to the center of gravity of the pendulum for the SEIS-VBB sensor.
We find that Brownian noise could be a limiting factor in meeting the ILN requirement for lunar seismometers.
Further, we have developed a formalism to understand the temperature sensitivity of a seismometer, relating it quantitatively to the local gravity, the thermoelastic coefficient of the spring, change in center of gravity, and the coefficient of thermal expansion of the mechanical structures.
We found that in general the temperature sensitivity of a seismometer is proportional to the local gravity, and so the temperature sensitivity can be reduced when operating on a planetary body with lower gravity.
Our Brownian noise and temperature sensitivity models will be useful in the design of the next generation of planetary seismometers.
Related Results
The Planet Explorer: Navigating Planetary Sample Data in Spatial Dimensions
The Planet Explorer: Navigating Planetary Sample Data in Spatial Dimensions
Introduction:  Renewed interest in a human return to the Moon has revived the importance of past Apollo missions. Both manned and robotic missions to the Moon provided det...
Lunar glass
Lunar glass
Lunar glass, a significant component of lunar soil, is produced by non-equilibrium processes on the moon, such as volcanic eruptions, meteorite impacts, solar wind, and cosmic radi...
Hunt for Lunar-Originated Asteroid Population from Earth Flybys
Hunt for Lunar-Originated Asteroid Population from Earth Flybys
. IntroductionNear-Earth asteroids (NEAs) have been thought to originate from the main asteroid belt between Mars and Jupiter. However, recent research has revealed the existence o...
New Economy in space: Cis-lunar economic circle and analogue simulations in China to the 2061 Horizon
New Economy in space: Cis-lunar economic circle and analogue simulations in China to the 2061 Horizon
    The Moon is sometimes also called the "eighth continent" of the Earth. Determining how to utilize cis-lunar orbital infrastructures and lunar resources to car...
AstroLEAP: A Surface Package to Monitor the Near-Surface Lunar Environment
AstroLEAP: A Surface Package to Monitor the Near-Surface Lunar Environment
Introduction: The lunar surface has become a major target for a number of Space Agencies and private stakeholders with a number of commercial and institutional missions under prepa...
Mechanism of suppressing noise intensity of squeezed state enhancement
Mechanism of suppressing noise intensity of squeezed state enhancement
This research focuses on advanced noise suppression technologies for high-precision measurement systems, particularly addressing the limitations of classical noise reducing approac...
Walking Wheel Design for Lunar Rove-Rand and Its Application Simulation Based on Virtual Lunar Environment
Walking Wheel Design for Lunar Rove-Rand and Its Application Simulation Based on Virtual Lunar Environment
The lunar rover design is the key problem of planet exploration. It is extraordinarily important for researchers to fully understand the lunar terrain and propose the reasonable lu...
Temperature sensitivity analysis on mass-spring potential with electrostatic frequency reduction for lunar seismometers
Temperature sensitivity analysis on mass-spring potential with electrostatic frequency reduction for lunar seismometers
A broadband seismometer has been identified as an important scientific instrument that can be deployed on the surface of Earth’s Moon in the near future. To achieve the goals of th...

