Drift Rates of Major Neptunian Features between 2018 and 2021
Erandi Chavez, Erin Redwing, Imke de Pater, Ricardo Hueso, Edward M., Molter, Michael H. Wong, Carlos Alvarez, Elinor Gates, Katherine de Kleer,, Joel Aycock, Jason Mcilroy, John Pelletier, Anthony Ridenour, Agust\'in, S\'anchez-Lavega, Jose F\'elix Rojas, Terry Stickel

TL;DR
This study measures the drift rates of Neptune's cloud features from 2018 to 2021 using various telescopes, revealing stable mid-latitude regions and confirming the drift rate of a circumpolar wave consistent with past data.
Contribution
First comprehensive analysis of Neptune's cloud feature drift rates over multiple years using combined observational datasets, linking features to atmospheric wind profiles.
Findings
Features near -70° align with K' band wind profile.
Mid-latitude features show high atmospheric stability.
Circumpolar wave drift rate matches previous measurements.
Abstract
Using near-infrared observations of Neptune from the Keck and Lick Observatories, and the Hubble Space Telescope in combination with amateur datasets, we calculated the drift rates of prominent infrared-bright cloud features on Neptune between 2018 and 2021. These features had lifespans of day to 1 month and were located at mid-latitudes and near the south pole. Our observations permitted determination of drift rates via feature tracking. These drift rates were compared to three zonal wind profiles describing Neptune's atmosphere determined from features tracked in H band (1.6 ), K' band (2.1 ), and Voyager 2 data at visible wavelengths. Features near measured in the F845M filter (845nm) were particularly consistent with the K' wind profile. The southern mid-latitudes hosted multiple features whose lifespans were 1 month, providing evidence…
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