Evaluating Radio Occultation (RO) Constellation Designs Using Observing System Simulation Experiments (OSSEs) for Ionospheric Specification
Open Access
- 14 August 2024
- journal article
- research article
- Published by American Geophysical Union (AGU) in Space Weather
- Vol. 22 (8)
Abstract
Low Earth orbit (LEO) radio occultation|radio occultations (RO) constellations can provide global electron density profiles (EDPs) to better specify and forecast the ionosphere‐thermosphere (I‐T) system. To inform future RO constellation design, this study uses comprehensive Observing System Simulation Experiments (OSSEs) to assess the ionospheric specification impact of assimilating synthetic EDPs into a coupled I‐T model. These OSSEs use 10 different sets of RO constellation configurations containing 6 or 12 LEO satellites with base orbit parameter combinations of 520 or 800 km altitude, and 24° or 72° inclination. The OSSEs are performed using the Ensemble Adjustment Kalman Filter implemented in the data assimilation (DA) Research Testbed and the Thermosphere‐Ionosphere‐Electrodynamics General Circulation Model (TIEGCM). A different I‐T model is used for the nature run, the Whole Atmosphere Model‐Ionosphere Plasmasphere Electrodynamics (WAM‐IPE), to simulate the period of interest is the St. Patrick's Day storm on March 13–18, 2015. Errors from models and EDP retrieval are realistically accounted for in this study through distinct I‐T models and by retrieving synthetic EDPs through an extension Abel inversion algorithm. OSSE assessment, using multiple metrics, finds that greater EDP spatial coverage leading to improved specification at altitudes 300 km and above, with the 520 km altitude constellations performing best due to yielding the highest observation counts. A potential performance limit is suggested with two 6‐satellite constellations. Lastly, close examination of Abel inversion error impacts highlights major EDP limitations at altitudes below 200 km and dayside equatorial regions with large horizontal gradients and low electron density magnitudes.Keywords
All Related Versions
Funding Information
- National Environmental Satellite, Data, and Information Service (SUBAWD00003038)
- National Science Foundation (AGS‐1848544)
- National Aeronautics and Space Administration (80NSSC23K1631)
- National Oceanic and Atmospheric Administration
- University of Colorado Boulder
- Computational and Information Systems Laboratory
This publication has 45 references indexed in Scilit:
- Inference of Hidden States by Coupled Thermosphere‐Ionosphere Data Assimilation2021
- Data Assimilation of Ground‐Based GPS and Radio Occultation Total Electron Content for Global Ionospheric SpecificationJournal of Geophysical Research: Space Physics, 2017
- Ionospheric electron density inversion for Global Navigation Satellite Systems radio occultation using aided Abel inversionsJournal of Geophysical Research: Space Physics, 2017
- Ionospheric data assimilation with thermosphere‐ionosphere‐electrodynamics general circulation model and GPS‐TEC during geomagnetic storm conditionsJournal of Geophysical Research: Space Physics, 2016
- A new source of the midlatitude ionospheric peak density structure revealed by a new Ionosphere‐Plasmasphere modelGeophysical Research Letters, 2016
- Ionospheric data assimilation and forecasting during stormsJournal of Geophysical Research: Space Physics, 2016
- An improved inversion for FORMOSAT‐3/COSMIC ionosphere electron density profilesJournal of Geophysical Research: Space Physics, 2015
- Effects of inferring unobserved thermospheric and ionospheric state variables by using an Ensemble Kalman Filter on global ionospheric specification and forecastingJournal of Geophysical Research: Space Physics, 2014
- Space Weather Observations by GNSS Radio Occultation: From FORMOSAT‐3/COSMIC to FORMOSAT‐7/COSMIC‐2Space Weather, 2014
- A comparison of the effects of initializing different thermosphere‐ionosphere model fields on storm time plasma density forecastsJournal of Geophysical Research: Space Physics, 2013