Observations of co-existing rising and falling tone emissions of electromagnetic ion cyclotron waves

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dc.contributor.author Ojha, Biswajit
dc.contributor.author Omura, Yoshiharu
dc.contributor.author Singh, Satyavir
dc.contributor.author Lakhina, Gurbax S.
dc.date.accessioned 2024-06-10T10:54:31Z
dc.date.available 2024-06-10T10:54:31Z
dc.date.issued 2024
dc.identifier.citation Earth Planets Space, 76, 81 (2024). https://doi.org/10.1186/s40623-024-02027-2 en_US
dc.identifier.uri http://library.iigm.res.in:8080/xmlui/handle/123456789/2031
dc.description.abstract We report observations of co-existing rising and falling tone emissions of electromagnetic ion cyclotron (EMIC) waves by THEMIS E spacecraft. The investigation of these fne structures of the EMIC waves is essential from the point of view of understanding the connection between the proton holes and the proton hills in velocity phase-space. The wave packets of rising and falling tones are tracked by Poynting vector analysis, where we observe that the rising tones are propagating northward and the falling tones are propagating southward. The nonlinear wave growth theory supports our observations. We propose a model where the proton velocity distribution function evolves through the formation of proton holes on the negative side of the distribution function and mirrored resonant protons forming proton hills on the positive side of the distribution function, allowing us to observe the co-existing rising and falling tone EMIC waves. en_US
dc.language.iso en en_US
dc.subject Fine structures of rising and falling tone EMIC waves en_US
dc.subject EMIC waves en_US
dc.subject Nonlinear evolution of the velocity distribution function en_US
dc.title Observations of co-existing rising and falling tone emissions of electromagnetic ion cyclotron waves en_US
dc.type Article en_US


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