Assimilation of GNSS Measurements for Estimation of High‐Latitude Convection Processes

Abstract Geomagnetic storms produce significant electrodynamics at midlatitudes. Strong ion convection can affect thermospheric neutral wind motion. The converse is also true, such that both fields and winds can drive ionospheric plasma movement. This work adjusts a background modeled high‐latitude...

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Main Authors: Daniel S. Miladinovich, Seebany Datta‐Barua, Aurora López Rubio, Shun‐Rong Zhang, Gary S. Bust
Format: Article
Language:English
Published: Wiley 2020-07-01
Series:Space Weather
Subjects:
Online Access:https://doi.org/10.1029/2019SW002409
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author Daniel S. Miladinovich
Seebany Datta‐Barua
Aurora López Rubio
Shun‐Rong Zhang
Gary S. Bust
author_facet Daniel S. Miladinovich
Seebany Datta‐Barua
Aurora López Rubio
Shun‐Rong Zhang
Gary S. Bust
author_sort Daniel S. Miladinovich
collection DOAJ
description Abstract Geomagnetic storms produce significant electrodynamics at midlatitudes. Strong ion convection can affect thermospheric neutral wind motion. The converse is also true, such that both fields and winds can drive ionospheric plasma movement. This work adjusts a background modeled high‐latitude electrostatic potential to estimate the storm time electric field based on data‐derived plasma densities and measurements of neutral wind. Electron densities are derived from global navigation satellite system (GNSS) total electron content measurements using Ionospheric Data Assimilation Four‐Dimensional (IDA4D). These are input to Estimating Model Parameters from Ionospheric Reverse Engineering (EMPIRE) to estimate electric potential corrections to the background Weimer 2000 potential model. The EMPIRE basis functions for electric potential are spherical harmonics in dipole magnetic colatitude and longitude, enforced to be constant along a magnetic field line. For the 17 March 2015 storm, EMPIRE electric potential produces westward zonal ion drifts that more closely agree with incoherent scatter radar (ISR) measurements made at Millstone Hill than the background Weimer 2000 model alone, when electric potential and meridional neutral winds are both corrected. Additionally ingesting northward line‐of‐sight neutral wind measurements from a Fabry‐Perot interferometer at Millstone Hill makes little difference in the agreement between zonal ion drift predictions and measurements. Estimation of only electric potential reduces the agreement between the assimilated prediction of the field‐perpendicular zonal drifts and ISR measurements significantly.
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spelling doaj-art-ec337473fc594dcb978e3cd7ac3de2072025-01-14T16:27:11ZengWileySpace Weather1542-73902020-07-01188n/an/a10.1029/2019SW002409Assimilation of GNSS Measurements for Estimation of High‐Latitude Convection ProcessesDaniel S. Miladinovich0Seebany Datta‐Barua1Aurora López Rubio2Shun‐Rong Zhang3Gary S. Bust4Mechanical, Materials, and Aerospace Engineering Illinois Institute of Technology Chicago IL USAMechanical, Materials, and Aerospace Engineering Illinois Institute of Technology Chicago IL USAMechanical, Materials, and Aerospace Engineering Illinois Institute of Technology Chicago IL USAHaystack Observatory Massachusetts Institute of Technology Cambridge MA USAJohn Hopkins University Applied Physics Laboratory Laurel MD USAAbstract Geomagnetic storms produce significant electrodynamics at midlatitudes. Strong ion convection can affect thermospheric neutral wind motion. The converse is also true, such that both fields and winds can drive ionospheric plasma movement. This work adjusts a background modeled high‐latitude electrostatic potential to estimate the storm time electric field based on data‐derived plasma densities and measurements of neutral wind. Electron densities are derived from global navigation satellite system (GNSS) total electron content measurements using Ionospheric Data Assimilation Four‐Dimensional (IDA4D). These are input to Estimating Model Parameters from Ionospheric Reverse Engineering (EMPIRE) to estimate electric potential corrections to the background Weimer 2000 potential model. The EMPIRE basis functions for electric potential are spherical harmonics in dipole magnetic colatitude and longitude, enforced to be constant along a magnetic field line. For the 17 March 2015 storm, EMPIRE electric potential produces westward zonal ion drifts that more closely agree with incoherent scatter radar (ISR) measurements made at Millstone Hill than the background Weimer 2000 model alone, when electric potential and meridional neutral winds are both corrected. Additionally ingesting northward line‐of‐sight neutral wind measurements from a Fabry‐Perot interferometer at Millstone Hill makes little difference in the agreement between zonal ion drift predictions and measurements. Estimation of only electric potential reduces the agreement between the assimilated prediction of the field‐perpendicular zonal drifts and ISR measurements significantly.https://doi.org/10.1029/2019SW002409data assimilationsubauroral polarization streamelectrodynamicsionospherethermospherecoupling
spellingShingle Daniel S. Miladinovich
Seebany Datta‐Barua
Aurora López Rubio
Shun‐Rong Zhang
Gary S. Bust
Assimilation of GNSS Measurements for Estimation of High‐Latitude Convection Processes
Space Weather
data assimilation
subauroral polarization stream
electrodynamics
ionosphere
thermosphere
coupling
title Assimilation of GNSS Measurements for Estimation of High‐Latitude Convection Processes
title_full Assimilation of GNSS Measurements for Estimation of High‐Latitude Convection Processes
title_fullStr Assimilation of GNSS Measurements for Estimation of High‐Latitude Convection Processes
title_full_unstemmed Assimilation of GNSS Measurements for Estimation of High‐Latitude Convection Processes
title_short Assimilation of GNSS Measurements for Estimation of High‐Latitude Convection Processes
title_sort assimilation of gnss measurements for estimation of high latitude convection processes
topic data assimilation
subauroral polarization stream
electrodynamics
ionosphere
thermosphere
coupling
url https://doi.org/10.1029/2019SW002409
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