Geoscientific Instrumentation, Methods and Data Systems
Geoscientific Instrumentation, Methods and Data Systems
GI
Articles | Volume 8, issue 2
Articles | Volume 8, issue 2
https://doi.org/10.5194/gi-8-197-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/gi-8-197-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
Articles | Volume 8, issue 2
Research article
 | Highlight paper
 | 
15 Aug 2019
Research article | Highlight paper |  | 15 Aug 2019

Multiresolution wavelet analysis applied to GRACE range-rate residuals

Saniya Behzadpour, Torsten Mayer-Gürr, Jakob Flury, Beate Klinger, and Sujata Goswami

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Cited articles

Bandikova, T. and Flury, J.: Improvement of the GRACE star camera data based on the revision of the combination method, Adv. Space Res., 54, 1818–1827, https://doi.org/10.1016/j.asr.2014.07.004, 2014. a
Bandikova, T., Flury, J., and Ko, U.-D.: Characteristics and accuracies of the GRACE inter-satellite pointing, Adv. Space Res., 50, 123–135, https://doi.org/10.1016/j.asr.2012.03.011, 2012. a, b, c
Bettadpur, S.: UTCSR Level-2 Processing Standards Document for Level-2 Product Release 0005, Tech. rep., Center for Space Research, The University of Texas at Austin, 2012. a
Carrere, L., Lyard, F., Cancet, M., and Guillot, A.: FES2014, a new tidal model on the global ocean with enhanced accuracy in shallow seas and in the Arctic region, Geophys. Res. Abstr., EGU2015-5481, EGU General Assembly 2015, Vienna, Austria, 2015. a
Dahle, C., Flechtner, F., Gruber, C., König, D., König, R., Michalak, G., and Neumayer, K.-H.: GFZ GRACE Level-2 Processing Standards Document for Level-2 Product Release 0005, https://doi.org/10.2312/gfz.b103-12020, Deutsches GeoForschungsZentrum (GFZ), 2012. a
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In this paper, we present an approach to represent underlying errors in measurements and physical models in the temporal gravity field determination using GRACE observations. This study provides an opportunity to improve the error model and the accuracy of the GRACE parameter estimation, as well as its successor GRACE Follow-On.
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