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Autor:
Nour Raouafi, Guillero Stenborg, Daniel Seaton, Haimin Wang, Jiasheng Wang, Craig DeForest, Stuart Bale, James Drake, Vadim Uritsky, Judy Karpen, C. Richard DeVore, Lakshmi Pradeep Chitta, Timothy Horbury, Louise Harra, Sofiane Bourouaine, Justin Kasper, Pankaj Kumar, Tai Phan, Alphonse Sterling, Marco Velli
Solar and stellar winds are ubiquitous flows of charged particles (i.e., electrons, protons, and heavier ions) permeating the astral spheres1. Through these winds, stars lose angular momentum, slow down their rotation as they age, shape planetary sys
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a059302c73d4ab2d0226c97fde919aac
https://doi.org/10.21203/rs.3.rs-2221227/v1
https://doi.org/10.21203/rs.3.rs-2221227/v1