Results 11 to 20 of about 1,598,590 (349)
A Review of the Theory of Galactic Winds Driven by Stellar Feedback [PDF]
Galaxies, 2018 Galactic winds from star-forming galaxies are crucial to the process of galaxy formation and evolution, regulating star formation, shaping the stellar mass function and the mass-metallicity relation, and enriching the intergalactic medium with metals ...
Dong Zhang
exaly +2 more sources
, 2005 Galactic winds are the primary mechanism by which energy and metals are recycled in galaxies and are deposited into the intergalactic medium. New observations are revealing the ubiquity of this process, particularly at high redshift.
Bland-Hawthorn, J. +2 more
core +4 more sources
Tropical Cyclone Winds from WindSat, AMSR2, and SMAP: Comparison with the HWRF Model
Remote Sensing, 2021 A new data set of tropical cyclone winds (‘TC-winds’) through rain as observed by the WindSat and AMSR2 microwave radiometers has been developed by making use of a linear combination of C- and X-band frequency channels.
Andrew Manaster +2 more
exaly +3 more sources
The Winds and Currents Mission Concept
Frontiers in Marine Science, 2019 The Winds and Currents Mission (WaCM) is a proposed approach to meet the need identified by the NRC Decadal Survey for the simultaneous measurements of ocean vector winds and currents. WaCM features a Ka-band pencil-beam Doppler scatterometer able to map
Ernesto Rodriguez +2 more
exaly +2 more sources
Stellar Winds on the Main-Sequence II: the Evolution of Rotation and Winds [PDF]
, 2015 Aims: We study the evolution of stellar rotation and wind properties for low-mass main-sequence stars. Our aim is to use rotational evolution models to constrain the mass loss rates in stellar winds and to predict how their properties evolve with time on
Brott, I. +3 more
core +2 more sources
The SILCC project: III. Regulation of star formation and outflows by stellar winds and supernovae [PDF]
, 2016 We study the impact of stellar winds and supernovae on the multi-phase interstellar medium using three-dimensional hydrodynamical simulations carried out with FLASH.
Baczynski, C. +11 more
core +4 more sources
Simulations of disk galaxies with cosmic ray driven galactic winds [PDF]
, 2013 We present results from high-resolution hydrodynamic simulations of isolated SMC- and Milky Way-sized galaxies that include a model for feedback from galactic cosmic rays (CRs). We find that CRs are naturally able to drive winds with mass loading factors
Agertz, Oscar +3 more
core +2 more sources
Improving the Accuracy of the Cross-Calibrated Multi-Platform (CCMP) Ocean Vector Winds
Remote Sensing, 2022 The Cross-Calibrated Multi-Platform (CCMP) Ocean vector wind analysis is a level-4 product that uses a variational method to combine satellite retrievals of ocean winds with a background wind field from a numerical weather prediction (NWP) model.
C. Mears +4 more
semanticscholar +1 more source
Widespread decline in winds delayed autumn foliar senescence over high latitudes
Proceedings of the National Academy of Sciences of the United States of America, 2021 Significance Decline in winds over past decades were observed over high northern latitudes (>50°), yet its influence on the date of autumn leaf senescence (DFS) remains unknown.
Chaoyang Wu +11 more
semanticscholar +1 more source
Zonas cardinales y orientación entre los qomléʔk (tobas del oeste de Formosa, Argentina)
Journal de la Société des Américanistes, 2021 This paper analyzes the different ways in which the Tobas of Western Formosa, Qomléʔk, also known as Tobas de Sombrero Negro, refer to cardinal zones and their contexts of use.
María Belén Carpio +1 more
doaj +1 more source