Upper‐Atmosphere Mass Density Variations From CASSIOPE Precise Orbits
Abstract Thermospheric mass density (TMD) measurements are invaluable to accurately estimate and predict the position and velocity of orbiting objects in Low Earth Orbit (LEO). Existing observational methods and predictive models have some problems (e.g., accuracy, resolution, coverage, cost, etc.)...
Saved in:
Main Authors: | Andrés Calabia, Shuanggen Jin |
---|---|
Format: | Article |
Language: | English |
Published: |
Wiley
2021-04-01
|
Series: | Space Weather |
Subjects: | |
Online Access: | https://doi.org/10.1029/2020SW002645 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Capabilities for Probing of Upper Atmosphere Density Variations and Seismic-Orbital Effects Using Small-Size Spacecraft
by: A. V. Tertyshnikov
Published: (2020-12-01) -
Assessing Thermospheric Neutral Density Models Using GEODYN's Precision Orbit Determination
by: Z. C. Waldron, et al.
Published: (2024-02-01) -
Comparisons and Analyses of Thermospheric Mass Densities Derived from Global Navigation Satellite System–Precise Orbit Determination and an Ionization Gauge–Orbital Neutral Atmospheric Detector Onboard a Spherical Satellite at 520 km Altitude
by: Yujiao Jin, et al.
Published: (2024-12-01) -
The Determination of Satellite Orbital Decay From POD Data During Geomagnetic Storms
by: Ruoxi Li, et al.
Published: (2021-04-01) -
Estimating Satellite Orbital Drag During Historical Magnetic Superstorms
by: Denny M. Oliveira, et al.
Published: (2020-11-01)