Results 171 to 180 of about 741 (254)
Abstract A polar cap patch was observed to exit the polar cap to become a blob as it entered the auroral oval on the nightside of the Earth under moderately quiet geomagnetic conditions (Kp = 3−). Auroral particle precipitation led to an increase in the electron density of the blob.
S. J. Maguire +9 more
wiley +1 more source
First Coincident Radar and Optical Observations of a Meteor Radio Afterglow
Abstract It has been hypothesized that Meteor Radio Afterglows (MRAs) occur due to resonant transition radiation (RTR) where suprathermal electrons emit as they pass through electron density inhomogeneities in a turbulent plasma. Meteor trails are thought to produce suprathermal electrons through anion oxidation, which can be identified through meteor ...
K. S. Obenberger +15 more
wiley +1 more source
Current understanding of electroautotrophy and its relevance in astrobiology-related research. [PDF]
Wang Q, Lau Vetter MCY.
europepmc +1 more source
Abstract In forced ocean general circulation models (OGCMs), regional sea‐level interannual variability arises from internal ocean dynamics and external forcings, among which freshwater fluxes from Greenland and rivers are typically prescribed as a seasonal climatology rather than with their full variability.
S. Tajouri +4 more
wiley +1 more source
On detecting and characterizing planetary oceans in the solar system using a distance-based ensemble modelling approach: application to the Uranus system. [PDF]
Cochrane CJ +4 more
europepmc +1 more source
Abstract Anthropogenic nitrogen emissions and deposition have substantially increased seawater nitrate concentrations in the western North Pacific. However, their influence on net community production (NCP)—a primary driver of organic carbon export from the euphotic zone—remains one of the least constrained components governing oceanic CO2 uptake ...
Minji Hong +4 more
wiley +1 more source
The origin of complex crater formation during high-speed impacts. [PDF]
Celebi HF +6 more
europepmc +1 more source
Early Solar Wind and Dynamo Magnetic Field Topology Predictions for (16) Psyche and Other Asteroids
Abstract Asteroid (16) Psyche is a metal‐rich body that might record an ancient coherent magnetization if some relict crust or mantle is preserved. Herein, we use magnetohydrodynamic simulations to predict (16) Psyche's field topology for several distinct pathways: (i) an early solar wind‐induced magnetization imparted after a larger body was impacted,
Atma Anand +3 more
wiley +1 more source
Pollution resistance of Saturn's ring particles during micrometeoroid impact. [PDF]
Hyodo R, Genda H, Madeira G.
europepmc +1 more source
Exploring the Interior Structure of (16) Psyche Through Basin‐Scale Collisions
Abstract Asteroid (16) Psyche, the largest member of the M/X‐type asteroids, may be the leftover core of a differentiated planetesimal. As such (16) Psyche will be explored in detail by NASA's discovery‐class Psyche mission in 2029. This will be the first mission to orbit a metal‐rich asteroid, or any asteroid in the 100–500 km size range.
Namya Baijal +7 more
wiley +1 more source

