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11 to 20 of 2,866 Results
TROPESS CrIS CO single pixel vertical profiles: Intercomparisons with MOPITT and model comparisons for 2020 US Western wildfiresEmbargoed
Apr 30, 2024
Ming Luo, 2024, "TROPESS CrIS CO single pixel vertical profiles: Intercomparisons with MOPITT and model comparisons for 2020 US Western wildfires", https://doi.org/10.48577/jpl.MVODTB, Atmospheric Measurement Techniques, JPL Open Repository
Abstract. The new TROPESS (TRopospheric Ozone and its Precursors from Earth System Sounding) profile retrievals of Carbon Monoxide (CO) from the Cross-track Infrared Sounder (CrIS) are evaluated against Measurement of Pollution in the Troposphere (MOPITT) CO Version 9 data. Compa...
Temporal Variability of Equatorial Ionization Anomaly Crest Locations Extracted from Global Ionospheric MapsEmbargoed
Apr 30, 2024
Olga Verkhoglyadova, 2024, "Temporal Variability of Equatorial Ionization Anomaly Crest Locations Extracted from Global Ionospheric Maps", https://doi.org/10.48577/jpl.VWPE33, Space Weather, JPL Open Repository
The Equatorial Ionization Anomaly (EIA) crest location is known to vary over a variety of temporal scales. For the first time we perform a statistical survey of the temporal variation of the EIA crest location viewed globally and spanning 20 years. We extract the crest location f...
Unraveling Geologic Processes and Aqueous Alteration at Tyrrhena Terra, MarsEmbargoed
Apr 30, 2024
Joana Voigt, 2024, "Unraveling Geologic Processes and Aqueous Alteration at Tyrrhena Terra, Mars", https://doi.org/10.48577/jpl.OXSPKN, JGR: Planets, JPL Open Repository
The central eastern Tyrrhena Terra region of Mars contains abundant aqueously altered minerals including Fe/Mg-smectites, smectite/chlorite mixtures, chlorites, zeolites, and carbonates. This study relates detections of these alteration-generated materials with mafic outcrops, ge...
Day/Night Differences in Molecular Oxygen in the Martian Upper AtmosphereEmbargoed
Apr 29, 2024
Ashwin Braude, 2024, "Day/Night Differences in Molecular Oxygen in the Martian Upper Atmosphere", https://doi.org/10.48577/jpl.FBNIHU, Journal of Geophysical Research: Planets, JPL Open Repository
We use the extensive stellar occultation dataset of the Imaging Ultraviolet Spectrograph21 (IUVS) aboard the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft to22 determine the first quantification of vertical variation in O2 mole fraction separately for23 day and night...
The reduced net carbon uptake over northern hemisphere land causes the close-to-normal CO2 growth rate in 2021 La NiñaEmbargoed
Apr 29, 2024
Junjie Liu, 2024, "The reduced net carbon uptake over northern hemisphere land causes the close-to-normal CO2 growth rate in 2021 La Niña", https://doi.org/10.48577/jpl.HLPJIP, Science Advances, JPL Open Repository
La Niña climate anomalies have historically been associated with significant reductions in the atmospheric CO2 growth rate. However, the 2021 La Niña exhibited a unique near-neutral impact on the CO2 growth rate. In this study, we investigate the underlying mechanisms by employin...
Near-infrared vibrational frequencies of HCN, CN, and HNC in N2 and Ar ice matricesEmbargoed
Apr 29, 2024
Edith Fayolle, 2024, "Near-infrared vibrational frequencies of HCN, CN, and HNC in N2 and Ar ice matrices", https://doi.org/10.48577/jpl.WGLPRE, ACS Earth and Space Science, JPL Open Repository
The surfaces of cold objects in the outer Solar System, like those of Kuiper Belt objects, are often dominated by volatile ices such as nitrogen, methane, and carbon monoxide. As these icy surfaces are subjected to a variety of energetic particles and ultraviolet radiation, HCN a...
The TESS-Keck Survey XX: Mass Catalog and Data ReleaseEmbargoed
Apr 29, 2024
Catherine Clark, 2024, "The TESS-Keck Survey XX: Mass Catalog and Data Release", https://doi.org/10.48577/jpl.PBE9NW, Astronomical Journal, JPL Open Repository
The Transiting Exoplanet Survey Satellite (TESS) has discovered thousands of new worlds with TESS52 planet candidates now outnumbering the total number of confirmed planets from Kepler. Owing to53 differences in survey design, TESS continues to provide planets that are more amena...
Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3Embargoed
Apr 25, 2024
Catherine Clark, 2024, "Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3", https://doi.org/10.48577/jpl.BEQHTS, Nature, JPL Open Repository
Located at the bottom of the main-sequence, ultracool dwarf stars are widespread in the solar neighborhood. Nevertheless, their extremely low luminosity has left their planetary population largely unexplored, and only one of them, TRAPPIST- 1, has so far been found to host a tran...
Through-Ice Acoustic Communication for Ocean Worlds ExplorationEmbargoed
Apr 24, 2024
Hyeong Jae Lee, 2024, "Through-Ice Acoustic Communication for Ocean Worlds Exploration", https://doi.org/10.48577/jpl.NI8LQ5, Sensors, JPL Open Repository
Subsurface exploration of ice-covered planets and moons presents communications challenges, because of the need to communicate through several kilometers of ice. The objective of the task is to develop the capability to wirelessly communicate through ice and thus enable the appli...
Is the Radio Source Dipole from NVSS Consistent with the CMB and ΛCDM?Embargoed
Apr 24, 2024
Yun-Ting Cheng, 2024, "Is the Radio Source Dipole from NVSS Consistent with the CMB and ΛCDM?", https://doi.org/10.48577/jpl.FZNBXN, The Astrophyscial Journal, JPL Open Repository
The dipole moment in the angular distribution of the cosmic microwave background (CMB) is thought to originate from the Doppler Effect and our motion relative to the CMB frame. Observations of large-scale structure (LSS) should show a related ``kinematic dipole'' and help test th...
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