Results 191 to 200 of about 81,818 (284)

Microimaging Spectroscopy of Carbonaceous Chondrites and Comparison to the Spectral Diversity of Asteroids

open access: yesJournal of Geophysical Research: Planets, Volume 131, Issue 2, February 2026.
Abstract Primitive asteroids and carbonaceous chondrites (CCs) record the history of processes in the early solar system. Visible and shortwave infrared (VSWIR) spectroscopy of primitive asteroids and bulk‐powdered CCs has identified shared spectral features suggestive of shared parent body origins.
S. A. Parra   +2 more
wiley   +1 more source

Construction progress of WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope [PDF]

open access: bronze, 2018
Chris Benn   +73 more
openalex   +1 more source

Hydrologic Variability Drives Differential Methane Dynamics in Agricultural Reservoirs of the Northern Great Plains

open access: yesJournal of Geophysical Research: Biogeosciences, Volume 131, Issue 2, February 2026.
Abstract Climate variability can regulate aquatic methane fluxes as increasing temperatures can elevate microbial metabolic rates, including methanogenesis. It is less well known how climate‐induced variability in seasonal precipitation and runoff might affect methane concentrations and fluxes in aquatic ecosystems.
Ryan Rimas, Jackie Webb, Kerri Finlay
wiley   +1 more source

A NEW WIDE-FIELD TELESCOPE WITH A MIRROR DIAMETER OF 600 MM FOR THE TELESCOPE NETWORK OF THE ODESSA OBSERVATORY

open access: diamond, 2020
N. N. Fashchevsky   +4 more
openalex   +1 more source

SIMULTANEOUS EXOPLANET CHARACTERIZATION AND DEEP WIDE-FIELD IMAGING WITH A DIFFRACTIVE PUPIL TELESCOPE [PDF]

open access: green, 2013
Olivier Guyon   +14 more
openalex   +1 more source

Segmentation and Tracking of Eruptive Solar Phenomena With Convolutional Neural Networks

open access: yesJournal of Geophysical Research: Machine Learning and Computation, Volume 3, Issue 1, February 2026.
Abstract Solar eruptive events are complex phenomena, which most often include coronal mass ejections (CME), CME‐driven compressive and shock waves, flares, and filament eruptions. CMEs are large eruptions of magnetized plasma from the Sun's outer atmosphere or corona, that propagate outward into the interplanetary space.
Oleg Stepanyuk, Kamen Kozarev
wiley   +1 more source

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