TY - JOUR
T1 - A Quarter Century of Wind Spacecraft Discoveries
AU - Wilson, Lynn B.
AU - Brosius, Alexandra L.
AU - Gopalswamy, Natchimuthuk
AU - Nieves-Chinchilla, Teresa
AU - Szabo, Adam
AU - Hurley, Kevin
AU - Phan, Tai
AU - Kasper, Justin C.
AU - Lugaz, Noé
AU - Richardson, Ian G.
AU - Chen, Christopher H.K.
AU - Verscharen, Daniel
AU - Wicks, Robert T.
AU - TenBarge, Jason M.
N1 - Publisher Copyright:
© 2021. The Authors. This article has been contributed to by US Government employees and their work is in the public domain in the USA.
PY - 2021/6
Y1 - 2021/6
N2 - The Wind spacecraft, launched on November 1, 1994, is a critical element in NASA’s Heliophysics System Observatory (HSO)—a fleet of spacecraft created to understand the dynamics of the Sun-Earth system. The combination of its longevity (>25 years in service), its diverse complement of instrumentation, and high resolution and accurate measurements has led to it becoming the “standard candle” of solar wind measurements. Wind has over 55 selectable public data products with over ∼1,100 total data variables (including OMNI data products) on SPDF/CDAWeb alone. These data have led to paradigm shifting results in studies of statistical solar wind trends, magnetic reconnection, large-scale solar wind structures, kinetic physics, electromagnetic turbulence, the Van Allen radiation belts, coronal mass ejection topology, interplanetary and interstellar dust, the lunar wake, solar radio bursts, solar energetic particles, and extreme astrophysical phenomena such as gamma-ray bursts. This review introduces the mission and instrument suites then discusses examples of the contributions by Wind to these scientific topics that emphasize its importance to both the fields of heliophysics and astrophysics.
AB - The Wind spacecraft, launched on November 1, 1994, is a critical element in NASA’s Heliophysics System Observatory (HSO)—a fleet of spacecraft created to understand the dynamics of the Sun-Earth system. The combination of its longevity (>25 years in service), its diverse complement of instrumentation, and high resolution and accurate measurements has led to it becoming the “standard candle” of solar wind measurements. Wind has over 55 selectable public data products with over ∼1,100 total data variables (including OMNI data products) on SPDF/CDAWeb alone. These data have led to paradigm shifting results in studies of statistical solar wind trends, magnetic reconnection, large-scale solar wind structures, kinetic physics, electromagnetic turbulence, the Van Allen radiation belts, coronal mass ejection topology, interplanetary and interstellar dust, the lunar wake, solar radio bursts, solar energetic particles, and extreme astrophysical phenomena such as gamma-ray bursts. This review introduces the mission and instrument suites then discusses examples of the contributions by Wind to these scientific topics that emphasize its importance to both the fields of heliophysics and astrophysics.
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U2 - 10.1029/2020RG000714
DO - 10.1029/2020RG000714
M3 - Review article
AN - SCOPUS:85108623764
SN - 8755-1209
VL - 59
JO - Reviews of Geophysics
JF - Reviews of Geophysics
IS - 2
M1 - e2020RG000714
ER -