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    المساهمون: Particle Physics and Astrophysics, Space Physics Research Group, Department of Physics

    وصف الملف: application/pdf

    العلاقة: Parker Solar Probe was designed, built, and is now operated by the Johns Hopkins Applied Physics Laboratory as part of NASA's Living with a Star (LWS) program (contract NNN06AA01C). Support from the LWS management and technical team has played a critical role in the success of the Parker Solar Probe mission. The work has been supported by the Finnish Centre of Excellence in Research on Sustainable Space (FORESAIL; grant No. 336807). This is a project under the Academy of Finland, and this research has been supported by the European Research Council (SolMAG; grant No. 724391) as well as Academy of Finland project SWATCH (343581). Open access is funded by Helsinki University Library. I.C.J., M.P., and S.D.B. acknowledge support from the International Space Science Institute (ISSI) in Bern, through ISSI International Team project No. 557, Beam-Plasma Interaction in the Solar Wind and the Generation of Type III Radio Bursts. I.C.J. also acknowledges support from the ISSI visiting scientist program. The authors would also like to thank Dr. V. V. Krasnoselskikh for the active discussions on the topic of parametric decay instability and radio generation mechanisms.; Sishtla , C P , Jebaraj , I C , Pomoell , J , Magyar , N , Pulupa , M , Kilpua , E & Bale , S D 2023 , ' The Effect of the Parametric Decay Instability on the Morphology of Coronal Type III Radio Bursts ' , Astrophysical Journal Letters , vol. 959 , no. 2 , L33 . https://doi.org/10.3847/2041-8213/ad137eTest; ORCID: /0000-0002-4489-8073/work/150688168; ORCID: /0000-0003-1175-7124/work/150705655; ORCID: /0000-0003-4236-768X/work/150780379; http://hdl.handle.net/10138/569711Test; fe53c935-9213-4d14-b8c0-0aa42e0680fd; 85181693880; 001131993200001

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