Errors From Asymmetric Emission Rate in Spaceborne, Limb Sounding Doppler Interferometry: A Correction Algorithm With Application to ICON/MIGHTI
Abstract The Michelson Interferometer for Global High‐resolution Thermospheric Imaging (MIGHTI) on NASA's Ionospheric Connection Explorer (ICON) mission is designed to measure the neutral wind and temperature between 90 and ∼300 km altitude. Using the Doppler Asymmetric Spatial Heterodyne (DASH...
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doaj-f6b3bfd5638d4d8b84fa964144a238262020-11-25T03:10:07ZengAmerican Geophysical Union (AGU)Earth and Space Science2333-50842020-10-01710n/an/a10.1029/2020EA001164Errors From Asymmetric Emission Rate in Spaceborne, Limb Sounding Doppler Interferometry: A Correction Algorithm With Application to ICON/MIGHTIYen‐Jung J. Wu0Brian J. Harding1Colin C. Triplett2Jonathan J. Makela3Kenneth D. Marr4Christoph R. Englert5John M. Harlander6Thomas J. Immel7Space Sciences Laboratory University of California Berkeley CA USASpace Sciences Laboratory University of California Berkeley CA USASpace Sciences Laboratory University of California Berkeley CA USADepartment of Electrical and Computer Engineering University of Illinois at Urbana‐Champaign Urbana IL USASpace Science Division U.S. Naval Research Laboratory Washington DC USASpace Science Division U.S. Naval Research Laboratory Washington DC USASpace Systems Research Corporation Alexandria VA USASpace Sciences Laboratory University of California Berkeley CA USAAbstract The Michelson Interferometer for Global High‐resolution Thermospheric Imaging (MIGHTI) on NASA's Ionospheric Connection Explorer (ICON) mission is designed to measure the neutral wind and temperature between 90 and ∼300 km altitude. Using the Doppler Asymmetric Spatial Heterodyne (DASH) spectroscopy technique, observations from MIGHTI can be used to derive thermospheric winds by measuring Doppler shifts of the atomic oxygen red line (630.0 nm) and green line (557.7 nm). Harding et al. (2017, https://doi.org/10.1007/s11214‐017‐0359‐3) (Harding17) describe the wind retrieval algorithm in detail and point out the large uncertainties that result near the solar terminators and equatorial arcs, regions of large spatial gradients in airglow volume emission rates (VER). The uncertainties originate from the assumption of a constant VER at every given altitude, resulting in errors where the assumption is not valid when limb sounders, such as MIGHTI, observe regions with significant VER gradients. In this work, we introduce a new wind retrieval algorithm (Wu20) with the ability to account for VER that is asymmetric along the line of sight with respect to the tangent point. Using the predicted ICON orbit and simulated global VER variation, the greatest impact of the symmetric airglow assumption to the ICON vector wind product is found within 30° from the terminator when the spacecraft is in the dayside, causing an error of at least 10 m/s. The new algorithm developed in this study reduces the error near the terminator by a factor of 10. Although Wu20 improves the accuracy of the retrievals, it loses precision by 75% compared to Harding17.https://doi.org/10.1029/2020EA001164Dopper interferometryasymmetric ionosphereneutral wind retrievalIonospheric Connection Explorer |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Yen‐Jung J. Wu Brian J. Harding Colin C. Triplett Jonathan J. Makela Kenneth D. Marr Christoph R. Englert John M. Harlander Thomas J. Immel |
spellingShingle |
Yen‐Jung J. Wu Brian J. Harding Colin C. Triplett Jonathan J. Makela Kenneth D. Marr Christoph R. Englert John M. Harlander Thomas J. Immel Errors From Asymmetric Emission Rate in Spaceborne, Limb Sounding Doppler Interferometry: A Correction Algorithm With Application to ICON/MIGHTI Earth and Space Science Dopper interferometry asymmetric ionosphere neutral wind retrieval Ionospheric Connection Explorer |
author_facet |
Yen‐Jung J. Wu Brian J. Harding Colin C. Triplett Jonathan J. Makela Kenneth D. Marr Christoph R. Englert John M. Harlander Thomas J. Immel |
author_sort |
Yen‐Jung J. Wu |
title |
Errors From Asymmetric Emission Rate in Spaceborne, Limb Sounding Doppler Interferometry: A Correction Algorithm With Application to ICON/MIGHTI |
title_short |
Errors From Asymmetric Emission Rate in Spaceborne, Limb Sounding Doppler Interferometry: A Correction Algorithm With Application to ICON/MIGHTI |
title_full |
Errors From Asymmetric Emission Rate in Spaceborne, Limb Sounding Doppler Interferometry: A Correction Algorithm With Application to ICON/MIGHTI |
title_fullStr |
Errors From Asymmetric Emission Rate in Spaceborne, Limb Sounding Doppler Interferometry: A Correction Algorithm With Application to ICON/MIGHTI |
title_full_unstemmed |
Errors From Asymmetric Emission Rate in Spaceborne, Limb Sounding Doppler Interferometry: A Correction Algorithm With Application to ICON/MIGHTI |
title_sort |
errors from asymmetric emission rate in spaceborne, limb sounding doppler interferometry: a correction algorithm with application to icon/mighti |
publisher |
American Geophysical Union (AGU) |
series |
Earth and Space Science |
issn |
2333-5084 |
publishDate |
2020-10-01 |
description |
Abstract The Michelson Interferometer for Global High‐resolution Thermospheric Imaging (MIGHTI) on NASA's Ionospheric Connection Explorer (ICON) mission is designed to measure the neutral wind and temperature between 90 and ∼300 km altitude. Using the Doppler Asymmetric Spatial Heterodyne (DASH) spectroscopy technique, observations from MIGHTI can be used to derive thermospheric winds by measuring Doppler shifts of the atomic oxygen red line (630.0 nm) and green line (557.7 nm). Harding et al. (2017, https://doi.org/10.1007/s11214‐017‐0359‐3) (Harding17) describe the wind retrieval algorithm in detail and point out the large uncertainties that result near the solar terminators and equatorial arcs, regions of large spatial gradients in airglow volume emission rates (VER). The uncertainties originate from the assumption of a constant VER at every given altitude, resulting in errors where the assumption is not valid when limb sounders, such as MIGHTI, observe regions with significant VER gradients. In this work, we introduce a new wind retrieval algorithm (Wu20) with the ability to account for VER that is asymmetric along the line of sight with respect to the tangent point. Using the predicted ICON orbit and simulated global VER variation, the greatest impact of the symmetric airglow assumption to the ICON vector wind product is found within 30° from the terminator when the spacecraft is in the dayside, causing an error of at least 10 m/s. The new algorithm developed in this study reduces the error near the terminator by a factor of 10. Although Wu20 improves the accuracy of the retrievals, it loses precision by 75% compared to Harding17. |
topic |
Dopper interferometry asymmetric ionosphere neutral wind retrieval Ionospheric Connection Explorer |
url |
https://doi.org/10.1029/2020EA001164 |
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