An Improved Next Generation Gravity Mission

There is an opportunity to make a major reduction in the acceleration noise level for the first Next Generation Gravity Mission by replacing the accelerometers used on the GRACE Follow-On Mission by a highly simplified version of the Gravitational Reference Sensors flown very successfully on the LIS...

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Main Author: Peter L. Bender
Format: Article
Language:English
Published: MDPI AG 2022-02-01
Series:Remote Sensing
Subjects:
Online Access:https://www.mdpi.com/2072-4292/14/4/948
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author Peter L. Bender
author_facet Peter L. Bender
author_sort Peter L. Bender
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description There is an opportunity to make a major reduction in the acceleration noise level for the first Next Generation Gravity Mission by replacing the accelerometers used on the GRACE Follow-On Mission by a highly simplified version of the Gravitational Reference Sensors flown very successfully on the LISA Pathfinder mission of ESA. The reduced measurement noise level can make possible much-improved measurements of the short-period and short-wavelength variations in the geopotential. This would be particularly from the along-track analysis of the results, which can permit repeat measurements about half a day apart along ground tracks within 200 km of each other over a substantial part of the globe. Such a mission would permit considerably improved testing of geophysical models for the geopotential variations due to changes in the Earth’s mass distribution.
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spelling doaj.art-13a2723b82834340bd8b46e1ea287fa32023-11-23T21:54:38ZengMDPI AGRemote Sensing2072-42922022-02-0114494810.3390/rs14040948An Improved Next Generation Gravity MissionPeter L. Bender0JILA, University of Colorado, Boulder, CO 80309-0440, USAThere is an opportunity to make a major reduction in the acceleration noise level for the first Next Generation Gravity Mission by replacing the accelerometers used on the GRACE Follow-On Mission by a highly simplified version of the Gravitational Reference Sensors flown very successfully on the LISA Pathfinder mission of ESA. The reduced measurement noise level can make possible much-improved measurements of the short-period and short-wavelength variations in the geopotential. This would be particularly from the along-track analysis of the results, which can permit repeat measurements about half a day apart along ground tracks within 200 km of each other over a substantial part of the globe. Such a mission would permit considerably improved testing of geophysical models for the geopotential variations due to changes in the Earth’s mass distribution.https://www.mdpi.com/2072-4292/14/4/948rapid earth mass variationsshort wavelength earth mass variationssimplified gravitational reference sensors
spellingShingle Peter L. Bender
An Improved Next Generation Gravity Mission
Remote Sensing
rapid earth mass variations
short wavelength earth mass variations
simplified gravitational reference sensors
title An Improved Next Generation Gravity Mission
title_full An Improved Next Generation Gravity Mission
title_fullStr An Improved Next Generation Gravity Mission
title_full_unstemmed An Improved Next Generation Gravity Mission
title_short An Improved Next Generation Gravity Mission
title_sort improved next generation gravity mission
topic rapid earth mass variations
short wavelength earth mass variations
simplified gravitational reference sensors
url https://www.mdpi.com/2072-4292/14/4/948
work_keys_str_mv AT peterlbender animprovednextgenerationgravitymission
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