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Introduction to Pulsar Wind Nebulae
2018The ejected material by a SN explosion interacts with the surrounding environment, giving rise to a new astrophysical object known as SNR (for a review of this matter, I refer the reader to (Reynolds 2008) and to Appendix A for more information on the first evolutionary phase).
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Introduction to Pulsar Wind Nebulae
2016Pulsar Wind Nebulae are nebulae of electrons and positrons powered by a central pulsar. In this chapter I give a detailed description of star evolution, centered on the description of supernova remnants, pulsars and pulsar wind nebulae. The basic properties of pulsars are explained, together with the emission mechanisms responsible for the production ...
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Rechargeable Batteries for Grid Scale Energy Storage
Chemical Reviews, 2022Yang Jin, , Wei Chen
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Expert elicitation survey predicts 37% to 49% declines in wind energy costs by 2050
Nature Energy, 2021Ryan Wiser, Joseph Rand, Joachim Seel
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Radiative Models of Pulsar Wind Nebulae
2017Since pulsar wind nebulae (PWNe) are the product of the interaction between the magnetized, highly relativistic particle outflow powered by a neutron star’s rotational energy and its surroundings, their emission is sensitive to the properties of the central neutron star, its pulsar wind, and surroundings.
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Offshore wind competitiveness in mature markets without subsidy
Nature Energy, 2020Malte Jansen +2 more
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A global assessment of extreme wind speeds for wind energy applications
Nature Energy, 2021Sara C Pryor, Rebecca J Barthelmie
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