Earth's ambipolar electrostatic field and its role in ion escape to space

成果类型:
Article
署名作者:
Collinson, Glyn A.; Glocer, Alex; Pfaff, Robert; Barjatya, Aroh; Conway, Rachel; Breneman, Aaron; Clemmons, James; Eparvier, Francis; Michell, Robert; Mitchell, David; Imber, Suzie; Akbari, Hassanali; Davis, Lance; Kavanagh, Andrew; Robertson, Ellen; Swanson, Diana; Xu, Shaosui; Miller, Jacob; Cameron, Timothy; Chornay, Dennis; Uribe, Paulo; Nguyen, Long; Clayton, Robert; Graves, Nathan; Debchoudhury, Shantanab; Valentine, Henry; Ghalib, Ahmed
署名单位:
National Aeronautics & Space Administration (NASA); NASA Goddard Space Flight Center; Catholic University of America; Embry-Riddle Aeronautical University; University System Of New Hampshire; University of New Hampshire; University of Colorado System; University of Colorado Boulder; University of California System; University of California Berkeley; University of Leicester; UK Research & Innovation (UKRI); Natural Environment Research Council (NERC); NERC British Antarctic Survey; Pennsylvania Commonwealth System of Higher Education (PCSHE); Pennsylvania State University; Pennsylvania State University - University Park; National Aeronautics & Space Administration (NASA); NASA Goddard Space Flight Center; Wallops Flight Facility
刊物名称:
Nature
ISSN/ISSBN:
0028-3686
DOI:
10.1038/s41586-024-07480-3
发表日期:
2024-08-29
页码:
1021-+
关键词:
electric-fields polar wind photoelectrons ionosphere venus
摘要:
Cold plasma of ionospheric origin has recently been found to be a much larger contributor to the magnetosphere of Earth than expected(1-3). Numerous competing mechanisms have been postulated to drive ion escape to space, including heating and acceleration by wave-particle interactions(4) and a global electrostatic field between the ionosphere and space (called the ambipolar or polarization field)(5,6). Observations of heated O+ ions in the magnetosphere are consistent with resonant wave-particle interactions(7). By contrast, observations of cold supersonic H+ flowing out of the polar ionosphere(8,9) (called the polar wind) suggest the presence of an electrostatic field. Here we report the existence of a +0.55 +/- 0.09 V electric potential drop between 250 km and 768 km from a planetary electrostatic field (E-vertical bar vertical bar circle plus = 1.09 +/- 0.17 mu V m(-1)) generated exclusively by the outward pressure of ionospheric electrons. We experimentally demonstrate that the ambipolar field of Earth controls the structure of the polar ionosphere, boosting the scale height by 271%. We infer that this increases the supply of cold O+ ions to the magnetosphere by more than 3,800%, in which other mechanisms such as wave-particle interactions can heat and further accelerate them to escape velocity. The electrostatic field of Earth is strong enough by itself to drive the polar wind(9,10) and is probably the origin of the cold H+ ion population(1) that dominates much of the magnetosphere(2,3).
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