Observations of whistler mode waves by Solar Orbiter’s RPW Low Frequency Receiver (LFR): In-flight performance and first results. Chust, T., Kretzschmar, M., Graham, D. B., Le Contel, O., Retinò, A., Alexandrova, A., Berthomier, M., Hadid, L. Z., Sahraoui, F., Jeandet, A., Leroy, P., Pellion, J., Bouzid, V., Katra, B., Piberne, R., Khotyaintsev, Y. V., Vaivads, A., Krasnoselskikh, V., Souček, J., Santolík, O., Lorfèvre, E., Plettemeier, D., Steller, M., Štverák, Š., Trávníček, P., Vecchio, A., Maksimovic, M., Bale, S. D., Horbury, T. S., O’Brien, H., Evans, V., & Angelini, V. Astronomy & Astrophysics, 656:A17, December, 2021. ![Observations of whistler mode waves by Solar Orbiter’s RPW Low Frequency Receiver (LFR): In-flight performance and first results [link]](https://bibbase.org/img/filetypes/link.svg "link")
Paper doi abstract bibtex Methods. Several case studies of whistler mode waves are presented, using all possible LFR onboard digital processing products, waveforms, spectral matrices, and basic wave parameters. Results. Here, we show that whistler mode waves can be very properly identified and characterized, along with their Doppler-shifted frequency, based on the waveform capture as well as on the LFR onboard spectral analysis. Conclusions. Despite the fact that calibrations of the electric and magnetic data still require some improvement, these first whistler observations show a good overall consistency between the RPW LFR data, indicating that many science results on these waves, as well as on other plasma waves, can be obtained by Solar Orbiter in the solar wind.
@article{chust_observations_2021,
title = {Observations of whistler mode waves by {Solar} {Orbiter}’s {RPW} {Low} {Frequency} {Receiver} ({LFR}): {In}-flight performance and first results},
volume = {656},
issn = {0004-6361, 1432-0746},
shorttitle = {Observations of whistler mode waves by {Solar} {Orbiter}’s {RPW} {Low} {Frequency} {Receiver} ({LFR})},
url = {https://www.aanda.org/10.1051/0004-6361/202140932},
doi = {10.1051/0004-6361/202140932},
abstract = {Methods. Several case studies of whistler mode waves are presented, using all possible LFR onboard digital processing products, waveforms, spectral matrices, and basic wave parameters.
Results. Here, we show that whistler mode waves can be very properly identified and characterized, along with their Doppler-shifted frequency, based on the waveform capture as well as on the LFR onboard spectral analysis.
Conclusions. Despite the fact that calibrations of the electric and magnetic data still require some improvement, these first whistler observations show a good overall consistency between the RPW LFR data, indicating that many science results on these waves, as well as on other plasma waves, can be obtained by Solar Orbiter in the solar wind.},
language = {en},
urldate = {2022-07-12},
journal = {Astronomy \& Astrophysics},
author = {Chust, T. and Kretzschmar, M. and Graham, D. B. and Le Contel, O. and Retinò, A. and Alexandrova, A. and Berthomier, M. and Hadid, L. Z. and Sahraoui, F. and Jeandet, A. and Leroy, P. and Pellion, J.-C. and Bouzid, V. and Katra, B. and Piberne, R. and Khotyaintsev, Yu. V. and Vaivads, A. and Krasnoselskikh, V. and Souček, J. and Santolík, O. and Lorfèvre, E. and Plettemeier, D. and Steller, M. and Štverák, Š. and Trávníček, P. and Vecchio, A. and Maksimovic, M. and Bale, S. D. and Horbury, T. S. and O’Brien, H. and Evans, V. and Angelini, V.},
month = dec,
year = {2021},
pages = {A17},
}
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Despite the fact that calibrations of the electric and magnetic data still require some improvement, these first whistler observations show a good overall consistency between the RPW LFR data, indicating that many science results on these waves, as well as on other plasma waves, can be obtained by Solar Orbiter in the solar wind.","language":"en","urldate":"2022-07-12","journal":"Astronomy & Astrophysics","author":[{"propositions":[],"lastnames":["Chust"],"firstnames":["T."],"suffixes":[]},{"propositions":[],"lastnames":["Kretzschmar"],"firstnames":["M."],"suffixes":[]},{"propositions":[],"lastnames":["Graham"],"firstnames":["D.","B."],"suffixes":[]},{"propositions":[],"lastnames":["Le","Contel"],"firstnames":["O."],"suffixes":[]},{"propositions":[],"lastnames":["Retinò"],"firstnames":["A."],"suffixes":[]},{"propositions":[],"lastnames":["Alexandrova"],"firstnames":["A."],"suffixes":[]},{"propositions":[],"lastnames":["Berthomier"],"firstnames":["M."],"suffixes":[]},{"propositions":[],"lastnames":["Hadid"],"firstnames":["L.","Z."],"suffixes":[]},{"propositions":[],"lastnames":["Sahraoui"],"firstnames":["F."],"suffixes":[]},{"propositions":[],"lastnames":["Jeandet"],"firstnames":["A."],"suffixes":[]},{"propositions":[],"lastnames":["Leroy"],"firstnames":["P."],"suffixes":[]},{"propositions":[],"lastnames":["Pellion"],"firstnames":["J.-C."],"suffixes":[]},{"propositions":[],"lastnames":["Bouzid"],"firstnames":["V."],"suffixes":[]},{"propositions":[],"lastnames":["Katra"],"firstnames":["B."],"suffixes":[]},{"propositions":[],"lastnames":["Piberne"],"firstnames":["R."],"suffixes":[]},{"propositions":[],"lastnames":["Khotyaintsev"],"firstnames":["Yu.","V."],"suffixes":[]},{"propositions":[],"lastnames":["Vaivads"],"firstnames":["A."],"suffixes":[]},{"propositions":[],"lastnames":["Krasnoselskikh"],"firstnames":["V."],"suffixes":[]},{"propositions":[],"lastnames":["Souček"],"firstnames":["J."],"suffixes":[]},{"propositions":[],"lastnames":["Santolík"],"firstnames":["O."],"suffixes":[]},{"propositions":[],"lastnames":["Lorfèvre"],"firstnames":["E."],"suffixes":[]},{"propositions":[],"lastnames":["Plettemeier"],"firstnames":["D."],"suffixes":[]},{"propositions":[],"lastnames":["Steller"],"firstnames":["M."],"suffixes":[]},{"propositions":[],"lastnames":["Štverák"],"firstnames":["Š."],"suffixes":[]},{"propositions":[],"lastnames":["Trávníček"],"firstnames":["P."],"suffixes":[]},{"propositions":[],"lastnames":["Vecchio"],"firstnames":["A."],"suffixes":[]},{"propositions":[],"lastnames":["Maksimovic"],"firstnames":["M."],"suffixes":[]},{"propositions":[],"lastnames":["Bale"],"firstnames":["S.","D."],"suffixes":[]},{"propositions":[],"lastnames":["Horbury"],"firstnames":["T.","S."],"suffixes":[]},{"propositions":[],"lastnames":["O’Brien"],"firstnames":["H."],"suffixes":[]},{"propositions":[],"lastnames":["Evans"],"firstnames":["V."],"suffixes":[]},{"propositions":[],"lastnames":["Angelini"],"firstnames":["V."],"suffixes":[]}],"month":"December","year":"2021","pages":"A17","bibtex":"@article{chust_observations_2021,\n\ttitle = {Observations of whistler mode waves by {Solar} {Orbiter}’s {RPW} {Low} {Frequency} {Receiver} ({LFR}): {In}-flight performance and first results},\n\tvolume = {656},\n\tissn = {0004-6361, 1432-0746},\n\tshorttitle = {Observations of whistler mode waves by {Solar} {Orbiter}’s {RPW} {Low} {Frequency} {Receiver} ({LFR})},\n\turl = {https://www.aanda.org/10.1051/0004-6361/202140932},\n\tdoi = {10.1051/0004-6361/202140932},\n\tabstract = {Methods. 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