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The Mass Change Designated Observable Study: Overview and ResultsThe 2017–2027 United States National Academy of Sciences Decadal Survey (DS) for Earth Science and Applications from Space identified Mass Change (MC) as one of five Designated Observables (DOs) having the highest priority in terms of Earth observations required to advance Earth system science over the next decade. In response to this designation, NASA initiated several multi-center studies, with the goal of recommending observing system architectures for each DO for implementation within this decade. This paper provides an overview of the Mass Change Designated Observable (MCDO) Study along with key findings. The study process included: (a) generation of a Science and Applications Traceability Matrix (SATM) that maps required measurement parameters to the DS Science and Applications Objectives; (b) identification of three architecture classes relevant for measuring mass change: Precise Orbit Determination (POD), Satellite-Satellite-Tracking (SST) and Gravity Gradiometry (GG), along with variants within each architecture class; and (c) creation of a Value Framework process that considers science value, cost, risk, schedule, and partnership opportunities, to identify and recommend high value observing systems for further in-depth study. The study team recommended the implementation of an SST architecture, and identified variants that simultaneously (a) satisfy the baseline measurement parameters of the SATM; (b) maximize the probability of providing overlap with the Gravity Recovery and Climate Experiment Follow-On (GRACE-FO) mission currently in operation, accelerating science return from both missions; and (c) provide a pathway towards substantial improvements in resolution and accuracy of mass change data products relative to the program of record.
Document ID
20220012313
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
D N Wiese
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
B Bienstock
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
C Blackwood
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
J Chrone
(Langley Research Center Hampton, Virginia, United States)
B D Loomis
(Goddard Space Flight Center Greenbelt, Maryland, United States)
J Sauber
(Goddard Space Flight Center Greenbelt, Maryland, United States)
M Rodell
(Goddard Space Flight Center Greenbelt, Maryland, United States)
R Baize
(Langley Research Center Hampton, Virginia, United States)
D Bearden
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
K Case
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
S Horner
(Ames Research Center Mountain View, California, United States)
S Luthcke
(Goddard Space Flight Center Greenbelt, Maryland, United States)
J T Reager
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
M Srinivasan
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
L Tsaoussi
(National Aeronautics and Space Administration Washington D.C., District of Columbia, United States)
F Webb
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
A Whitehurst
(National Aeronautics and Space Administration Washington D.C., District of Columbia, United States)
V Zlotnicki
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Date Acquired
August 9, 2022
Publication Date
July 19, 2022
Publication Information
Publication: Earth and Space Science
Publisher: American Geophysical Union
Volume: 9
Issue: 8
Issue Publication Date: August 1, 2022
e-ISSN: 2333-5084
Subject Category
Space Sciences (General)
Funding Number(s)
WBS: 304029.01.32.02.01
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
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