Results 81 to 90 of about 55,109 (308)

Realizing Ultrahigh Dielectric Constant With Ultrawide Temperature Stability in Dual‐Phase BNT‐BST Ceramics by SPS Sintering

Rare Metals, EarlyView.
ABSTRACT Ceramic capacitors are critical components in advanced electronic devices, primarily due to their multi‐functionalities in energy/information storage and conversion. However, poor temperature stability remains a long‐standing challenge for practical applications, especially at extremely high‐ or low‐temperature conditions (e.g., > 200°C or ...
Zhi‐Peng Li, Dong‐Xu Li, Zong‐Yang Shen, You Zhang, Jia‐Mou Wu, Yan Li, Wen‐Qin Luo, Chao‐Feng Wu   +7 more
wiley   +1 more source

Spectroscopic observations of the planets Final report [PDF]

Spectroscopic observations of Jupiter, Venus, and Mars ...
Owen, T.
core   +1 more source

Jupiter as an exoplanet: UV to NIR transmission spectrum reveals hazes, a Na layer and possibly stratospheric H2O-ice clouds [PDF]

, 2015
Currently, the analysis of transmission spectra is the most successful technique to probe the chemical composition of exoplanet atmospheres. But the accuracy of these measurements is constrained by observational limitations and the diversity of possible ...
Garcia-Melendo, E., Gonzalez-Merino, B, Lopez-Puertas, M., Montañes-Rodriguez, P., Palle, E.   +4 more
core   +3 more sources

Evaluating land–sea linkages using land cover change and coral reef monitoring data: A case study from northeastern Puerto Rico

Remote Sensing in Ecology and Conservation, EarlyView.
Land cover change that leads to increased nutrient and sediment runoff is an important driver of change in coral reef ecosystems. In this study, we combined satellite remote sensing and field monitoring to assess concomitant changes in watershed land cover and coral cover in northeastern Puerto Rico in 2000–2015.
Pirta Palola, Sasha Hills, Simon J. Pittman, Edwin A. Hernández‐Delgado, Antoine Collin, Lisa M. Wedding   +5 more
wiley   +1 more source

A Carbon-rich Atmosphere on a Windy Pulsar Planet

The Astrophysical Journal Letters
A handful of enigmatic Jupiter-mass objects have been discovered orbiting pulsars. One such object, PSR J2322–2650b, uniquely resembles a hot-Jupiter exoplanet, due to its minimum density of 1.8 g cm ^−3 and its ∼1900 K equilibrium temperature.
Michael Zhang, Maya Beleznay, Timothy D. Brandt, Roger W. Romani, Peter Gao, Hayley Beltz, Matthew Bailes, Matthew C. Nixon, Jacob L. Bean, Thaddeus D. Komacek, Brandon P. Coy, Guangwei Fu, Rafael Luque, Daniel J. Reardon, Emma Carli, Ryan M. Shannon, Jonathan J. Fortney, Anjali A. A. Piette, M. Coleman Miller, Jean-Michel Desert   +19 more
doaj   +1 more source

Jupiter: As a planet [PDF]

The planet Jupiter, its planetary mass and atmosphere, radio waves emitted from Jupiter, thermal radiation, internal structure of Jupiter, and the possibility of life on Jupiter are discussed.

core   +1 more source

Molecular tracers of planet formation in the atmospheres of hot Jupiters [PDF]

, 2021
Richard Hobbs, Oliver Shorttle, Nikku Madhusudhan   +2 more
openalex   +1 more source

Substitution of Ti by Nb in Maraging Steel: Effects on Strengthening Mechanisms and Crystallographic Behavior

steel research international, EarlyView.
This work demonstrates that replacing Ti with Nb in maraging steel forms nanoscale Nb–Mo particles along boundaries, strengthening the alloy without relying on Ti phases. Heat‐treatment tuning promotes uniform crystal orientation and balanced grain boundaries, enabling strong yet ductile behavior.
Mohamad Masoumi, Manoel José, Gerardo Jesus Aracena Pérez, Isabel Ferreira Barros, Marcos Natan da Silva Lima, Geronimo Perez, Samuel Lucas Santos Medeiros, Pedro Henrique Pinheiro Lima, Luís Flávio Gaspar Herculano, Maria Vittoria Moraschini Reis, Sérgio Souto Maior Tavares, Farina Alexandre Bellegard, Fridman Daniel Pallos, Miloslav Béreš, Hamilton Ferreira Gomes de Abreu   +14 more
wiley   +1 more source

Transport properties in the atmosphere of Jupiter [PDF]

The computer program used to obtain transport properties for the Hulburt-Hirschfelder potential was tested. Transport properties for the C-C interaction were calculated.
Biolsi, L., Jr.
core   +1 more source

Comparing Atmospheric Cloud Models of Jupiter

, 2023
Comparing Atmospheric Cloud Models of Jupiter- can we reduce the degeneracy of the problem? Using new techniques we are able to test previous models and develop new a new model through constraining properties of Jupiter’s atmosphere before undertaking full retrievals. This reduces some of the degeneracy of the problem allowing us to be more confident
Alexander, C, Irwin, P
openaire   +1 more source