• Sorted by Date • Sorted by Last Name of First Author •
Guo, Yu, Guo, Fei, Zhang, Xiaohong, Yang, Yan, Mei, Dengkui, and Ren, Xiaodong, 2025. A Two-Step Method for Enhancing Thermospheric Mass Density Empirical Model. Space Weather, 23(5):e2024SW004317, doi:10.1029/2024SW004317.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2025SpWea..2304317G,
author = {{Guo}, Yu and {Guo}, Fei and {Zhang}, Xiaohong and {Yang}, Yan and {Mei}, Dengkui and {Ren}, Xiaodong},
title = "{A Two-Step Method for Enhancing Thermospheric Mass Density Empirical Model}",
journal = {Space Weather},
keywords = {thermosphere, neutral total mass density, SWARM-C, GRACE-A, NRLMSIS 2.1 model, empirical model enhancement},
year = 2025,
month = may,
volume = {23},
number = {5},
eid = {e2024SW004317},
pages = {e2024SW004317},
abstract = "{With the rapid development of Low Earth Orbit constellations, the
importance of accurately estimating thermospheric mass density
is steadily increasing. Current empirical models still exhibit
unavoidable biases in estimating thermospheric mass density. In
this paper, we propose a novel two-step empirical model
calibration enhancement method. The enhancement coefficients are
constructed by the second-order spherical harmonic function and
the machine learning method. The daily in situ mass density
observations collected by the SWARM-C and GRACE-A satellites
between 2015 and 2017 are used to generate coefficients and test
the model. The two-step enhancement method performs well under
various conditions, including different satellites, altitudes,
and space weather scenarios. During storm periods, using
satellite observations as the references, the enhanced MSIS 2.1
model can achieve estimation error reduction of over 15\%.
During long-term testing in 2015, 2016, and 2017, the average
RMSEs of the enhanced thermospheric mass density decreased by
23.06\%, 20.33\%, and 30.95\%, respectively.}",
doi = {10.1029/2024SW004317},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025SpWea..2304317G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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