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Exploring Commercial Global Navigation Satellite System (GNSS) Radio Occultation (RO) Products for Planetary Boundary Layer Studies in the ArcticCommercial radio occultation (RO) satellites that utilize the Global Navigation Satellite System (GNSS) signals are emerging as key tools for observing the polar regions, which are not covered by the second-generation Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC-2) mission. This study evaluates the value of commercial RO measurements, specifically Spire and GeoOptics, for planetary boundary layer (PBL) investigations in the Arctic, a region where favor able lower-atmospheric penetration of GNSS RO is vital for observing the persistently shallow PBL. The lower tropospheric penetration capability of both Spire and GeoOptics over the Arctic Ocean, with nearly 80% observations reaching an altitude of 500m above mean sea level, is comparable to other RO missions such as the current Meteorological Operational satellite programme (MetOp) and the discontinued COSMIC-1 missions. A seasonal cycle in RO penetration probability, with the minimum occurring during the Arctic warm season, was observed in most RO datasets TS3,except NASA-purchased Spire data. Monthly mean Arctic PBL height (PBLH) derived from Spire and GeoOptics compares well with MetOp observations and the reanalysis from Modern-Era Retrospective analysis for Research and Applications version 2 (MERRA-2). A minimum penetration threshold of 500m generally suffices for determining Arctic PBLH, although a 300m threshold improves performance of NASA-purchased Spire data. Arctic PBLH representation is influenced less by the number of observations or instrument type and more by the algorithms used for bending angle and refractivity retrievals. These findings underscore the importance of processing algorithms in achieving accurate lower atmospheric soundings and Arctic PBLH representation.
Document ID
20250002847
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
Manisha Ganeshan
(Morgan State University Baltimore, United States)
Dong L Wu ORCID
(Goddard Space Flight Center Greenbelt, United States)
Joseph Santanello
(Goddard Space Flight Center Greenbelt, United States)
Jie Gong ORCID
(Goddard Space Flight Center Greenbelt, United States)
Chi Ao
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Panagiotis Vergados
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Kevin J Nelson
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Date Acquired
March 19, 2025
Publication Date
March 24, 2025
Publication Information
Publication: Atmoshperic Measurement Techniques
Publisher: European Geosciences Union
Volume: 18
Issue: 6
Issue Publication Date: March 25, 2025
ISSN: 1867-8610
e-ISSN: 1867-8548
Subject Category
Lunar and Planetary Science and Exploration
Funding Number(s)
CONTRACT_GRANT: 80NSSC23K0385
CONTRACT_GRANT: 80NM0018D0004
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
External Peer Committee
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