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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Format: | Article |
Language: | English |
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MDPI AG
2022-02-01
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Series: | Remote Sensing |
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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 |
collection | DOAJ |
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. |
first_indexed | 2024-03-09T21:07:51Z |
format | Article |
id | doaj.art-13a2723b82834340bd8b46e1ea287fa3 |
institution | Directory Open Access Journal |
issn | 2072-4292 |
language | English |
last_indexed | 2024-03-09T21:07:51Z |
publishDate | 2022-02-01 |
publisher | MDPI AG |
record_format | Article |
series | Remote Sensing |
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 AT peterlbender improvednextgenerationgravitymission |