Statistical study of electron density turbulence and ion-cyclotron waves in the inner heliosphere: Solar Orbiter observations. Carbone, F., Sorriso-Valvo, L., Khotyaintsev, Y. V., Steinvall, K., Vecchio, A., Telloni, D., Yordanova, E., Graham, D. B., Edberg, N. J. T., Eriksson, A. I., Johansson, E. P. G., Vásconez, C. L., Maksimovic, M., Bruno, R., D’Amicis, R., Bale, S. D., Chust, T., Krasnoselskikh, V., Kretzschmar, M., Lorfèvre, E., Plettemeier, D., Souček, J., Steller, M., Štverák, Š., Trávníček, P., Vaivads, A., Horbury, T. S., O’Brien, H., Angelini, V., & Evans, V. Astronomy & Astrophysics, 656:A16, December, 2021.
Statistical study of electron density turbulence and ion-cyclotron waves in the inner heliosphere: Solar Orbiter observations [link]Paper  doi  abstract   bibtex   
Context. The recently released spacecraft potential measured by the RPW instrument on board Solar Orbiter has been used to estimate the solar wind electron density in the inner heliosphere. Aims. The measurement of the solar wind’s electron density, taken in June 2020, has been analysed to obtain a thorough characterization of the turbulence and intermittency properties of the fluctuations. Magnetic field data have been used to describe the presence of ion-scale waves.
@article{carbone_statistical_2021,
	title = {Statistical study of electron density turbulence and ion-cyclotron waves in the inner heliosphere: {Solar} {Orbiter} observations},
	volume = {656},
	issn = {0004-6361, 1432-0746},
	shorttitle = {Statistical study of electron density turbulence and ion-cyclotron waves in the inner heliosphere},
	url = {https://www.aanda.org/10.1051/0004-6361/202140931},
	doi = {10.1051/0004-6361/202140931},
	abstract = {Context. The recently released spacecraft potential measured by the RPW instrument on board Solar Orbiter has been used to estimate the solar wind electron density in the inner heliosphere. Aims. The measurement of the solar wind’s electron density, taken in June 2020, has been analysed to obtain a thorough characterization of the turbulence and intermittency properties of the fluctuations. Magnetic field data have been used to describe the presence of ion-scale waves.},
	language = {en},
	urldate = {2022-07-12},
	journal = {Astronomy \& Astrophysics},
	author = {Carbone, F. and Sorriso-Valvo, L. and Khotyaintsev, Yu. V. and Steinvall, K. and Vecchio, A. and Telloni, D. and Yordanova, E. and Graham, D. B. and Edberg, N. J. T. and Eriksson, A. I. and Johansson, E. P. G. and Vásconez, C. L. and Maksimovic, M. and Bruno, R. and D’Amicis, R. and Bale, S. D. and Chust, T. and Krasnoselskikh, V. and Kretzschmar, M. and Lorfèvre, E. and Plettemeier, D. and Souček, J. and Steller, M. and Štverák, Š. and Trávníček, P. and Vaivads, A. and Horbury, T. S. and O’Brien, H. and Angelini, V. and Evans, V.},
	month = dec,
	year = {2021},
	pages = {A16},
}

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