Depleted plasma densities in the ionosphere of venus near solar minimum from parker solar probe observations of upper hybrid resonance emission. Collinson, G. A., Ramstad, R., Glocer, A., III Wilson, L., & Brosius, A. Geophysical Research Letters, 2021. Publisher: Amer Geophysical Union Type: Article tex.date-modified: 2022-04-12 11:34:54 +0100
Depleted plasma densities in the ionosphere of venus near solar minimum from parker solar probe observations of upper hybrid resonance emission [link]Paper  doi  abstract   bibtex   
On July 11, 2020, NASA's Parker Solar Probe made its third flyby of Venus. The upper hybrid resonance emission was observed below 1,100 km (a first at Venus), revealing electron densities an order of magnitude lower than at solar maximum. These observations are consistent with a substantial variation in the density and structure of the Venusian ionosphere over the Solar Cycle.
@article{Collinson2021,
	title = {Depleted plasma densities in the ionosphere of venus near solar minimum from parker solar probe observations of upper hybrid resonance emission},
	volume = {48},
	issn = {0094-8276},
	url = {https://doi.org/10.1029/2020GL092243},
	doi = {10.1029/2020GL092243},
	abstract = {On July 11, 2020, NASA's Parker Solar Probe made its third flyby of Venus. The upper hybrid resonance emission was observed below 1,100 km (a first at Venus), revealing electron densities an order of magnitude lower than at solar maximum. These observations are consistent with a substantial variation in the density and structure of the Venusian ionosphere over the Solar Cycle.},
	number = {9},
	journal = {Geophysical Research Letters},
	author = {Collinson, Glyn A. and Ramstad, Robin and Glocer, Alex and III Wilson, Lynn and Brosius, Alexandra},
	year = {2021},
	note = {Publisher: Amer Geophysical Union
Type: Article
tex.date-modified: 2022-04-12 11:34:54 +0100},
}

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