Results 111 to 120 of about 21,286 (216)
ABSTRACT Following the largest known Phanerozoic extinction, the end‐Permian mass extinction, the Early Triassic is often considered an interval of slow biotic recovery. During this time, the minor Smithian‐Spathian extinction occurred, further delaying the biotic recovery of this epoch.
Sean M. Newby +3 more
wiley +1 more source
Utilizing T-Line Mesh for Periumbilical Hernia Repair: Evaluation of Short-term Outcomes
Background:. Abdominal periumbilical hernias are prevalent within the adult population. When symptomatic, quality of life may be affected. This case series of 10 patients evaluates the short-term outcomes of using the T-Line mesh in periumbilical hernia ...
Charles Lu, DO +5 more
doaj +1 more source
Abstract Dust, sea salt, and anthropogenic and biogenic particles in total atmospheric deposition are sources of essential elements that can significantly impact biogeochemical cycles in the Atlantic Ocean and in islands of the Caribbean region. This unique 41‐month data set records direct sampling of total atmospheric deposition from March 2015 to ...
Yangjunjie Xu‐Yang +6 more
wiley +1 more source
Neptune Atmospheric Retrograde Orbiter – A Mission to Neptune and Its Moons [PDF]
The Neptune Atmospheric Retrograde Orbiter (NEPARO) mission concept foresees a large-scale interplanetary science mission to the outer solar system, namely Neptune with its system of rings and moons.
Bonny, Robin Frédéric
core
Tsunami inundation maps for Neptune, Lane County, Oregon
plate 1. Local source (Cascadia Subduction Zone) tsunami inundation map Neptune, Oregon -- plate 2. Distance source (Alaska-Aleutian Subduction Zone) tsunami inundation map Neptune, OregonThis archived document is maintained by the Oregon State Library ...
core
katelinbdonaldson/KHIs-at-Uranus-and-Neptune: KHIs at Uranus and Neptune
<p>This repository includes the scripts used to create analytic model to produce the results in the paper "Characterizing the solar wind-magnetosphere viscous interaction at Uranus and Neptune".</p> <p>The MATLAB code is split
katelinbdonaldson
core +1 more source
Reassessing planetary composition: Evidence of rock-dominated envelopes in Uranus and Neptune
Although Uranus and Neptune are commonly classified as ice giants, their exact compositions remain poorly constrained. Recent studies of outer Solar System bodies challenge the traditional view that these planets are primarily ice-dominated, suggesting ...
Ramirez Vanesa +2 more
doaj +1 more source
Bulk composition of the transiting hot Neptune around GJ 436
International audienceThe hot Neptune orbiting around GJ 436 is a unique example of an intermediate mass planet. Its close-in orbit suggests that the planet has undergone migration and its study is fundamental to understand planet formation and evolution.
Mordasini, C. +11 more
core +1 more source
Different Inhomogeneous Evolutionary Histories for Uranus and Neptune
We present updated nonadiabatic and inhomogeneous evolution models for Uranus and Neptune, employing an interior composition of methane, ammonia, water, and rocks.
Roberto Tejada Arevalo
doaj +1 more source

