758 citations
- Max Planck Institute for Solar System ResearchDE39 papers
- Stanford UniversityUS22 papers
- University College LondonGB13 papers
- University of California, BerkeleyUS12 papers
- University of GrazAT12 papers
- Lockheed Martin (United States)US11 papers
- Nagoya UniversityJP11 papers
- Goddard Space Flight CenterUS10 papers
- Monash UniversityAU10 papers
- Max Planck SocietyDE9 papers
- The University of SydneyAU9 papers
- Centre National de la Recherche ScientifiqueFR8 papers
160 papers
The Localized 12-hour Wave Over Alaska: Leveraging Meridional Wind Measurements From the Sodium Lidar
Sophie R. Phillips, Katrina Bossert, Komal Kumari +3
The 12-h wave in meridional winds in the mesosphere and lower thermosphere (MLT) during the solar minimum 2018-2019 Arctic winter is investigated using sodium lidar observations at…
Toward a Universal Framework for the Internal Gravity Wave Spectrum
Leticia Fabre-Lima, Jeffrey Early, Miles A. Sundermeyer
The Garrett-Munk (GM) spectrum has long provided a canonical model of the oceanic internal gravity wave field. However, it relies on hydrostatic assumptions and idealized stratific…
Magnetic flux systems involved in the May 2024 solar energetic events from AR 13664 inferred through coronal dimmings
Amaia Razquin, Karin Dissauer, Astrid M. Veronig +1
Coronal dimmings are transient depletions of coronal plasma observed in extreme ultraviolet and soft X-rays, interpreted as low-corona signatures of coronal mass ejections (CMEs).…
Calibrating Mid-Infrared Emission Features As Diagnostics of Star Formation in Infrared-Luminous Galaxies via Radiative Transfer Modeling
L. Robinson, D. Farrah, A. Efstathiou +13
Luminous infrared galaxies are key sites of obscured stellar mass assembly at z > 0.5. Their star formation rates (SFRs) are often estimated using the luminosities of the 6.2 micro…
Benchmarking atmospheric circulation variability in an AI emulator, ACE2, and a hybrid model, NeuralGCM
Ian Baxter, Hamid Pahlavan, Pedram Hassanzadeh +2
Physics-based atmosphere-land models with prescribed sea surface temperature have notable successes but also biases in their ability to represent atmospheric variability compared t…
Structure and Dynamics of the Sun's Interior Revealed by Helioseismic and Magnetic Imager
Alexander Kosovichev, Sarbani Basu, Yuto Bekki +43
High-resolution helioseismology observations with the Helioseismic and Magnetic Imager (HMI) onboard Solar Dynamics Observatory (SDO) provide a unique three-dimensional view of the…