Phase ratio in single-scattering dust particles: Implication to future DESTINY+ study of asteroid (3200) Phaethon
DC Field | Value | Language |
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dc.contributor.author | Evgenij Zubko | - |
dc.contributor.author | Wada, Koji | - |
dc.date.accessioned | 2024-01-18T22:00:38Z | - |
dc.date.available | 2024-01-18T22:00:38Z | - |
dc.date.created | 2023-06-27 | - |
dc.date.issued | 2023-11 | - |
dc.identifier.issn | 0019-1035 | - |
dc.identifier.uri | https://pr.ibs.re.kr/handle/8788114/14664 | - |
dc.description.abstract | The phase ratio is defined as a ratio of reflectivity of object at two different phase angles α. This light-scattering characteristic has revealed high sensitivity to physical parameters of a planetary regolith. We investigate the phase ratio of single-scattering irregularly shaped particles with different morphology by means of the discrete dipole approximation. The phase ratio defined at α = 0° and 30° appears to be highly sensitive to the imaginary part of refractive index and less sensitive to the size distribution of target particles; whereas, it is not sensitive to their real part of refractive index and irregular morphology when it attains a high level of disorder. Further, the phase ratio defined at α = 30° and 60° is almost fully insensitive to microphysics of target particles. This feature might help to enhance the scientific return from the future DESTINY+ mission to asteroid (3200) Phaethon. © 2023 Elsevier Inc. | - |
dc.language | 영어 | - |
dc.publisher | Academic Press Inc. | - |
dc.title | Phase ratio in single-scattering dust particles: Implication to future DESTINY+ study of asteroid (3200) Phaethon | - |
dc.type | Article | - |
dc.type.rims | ART | - |
dc.identifier.wosid | 001029514400001 | - |
dc.identifier.scopusid | 2-s2.0-85161668203 | - |
dc.identifier.rimsid | 81082 | - |
dc.contributor.affiliatedAuthor | Evgenij Zubko | - |
dc.identifier.doi | 10.1016/j.icarus.2023.115652 | - |
dc.identifier.bibliographicCitation | Icarus, v.404 | - |
dc.relation.isPartOf | Icarus | - |
dc.citation.title | Icarus | - |
dc.citation.volume | 404 | - |
dc.type.docType | Article | - |
dc.description.journalClass | 1 | - |
dc.description.journalClass | 1 | - |
dc.description.isOpenAccess | N | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
dc.relation.journalResearchArea | Astronomy & Astrophysics | - |
dc.relation.journalWebOfScienceCategory | Astronomy & Astrophysics | - |
dc.subject.keywordPlus | PLANETARY SURFACES | - |
dc.subject.keywordPlus | POLARIZATION | - |
dc.subject.keywordPlus | COLOR | - |
dc.subject.keywordPlus | LIGHT-SCATTERING | - |
dc.subject.keywordAuthor | Asteroid (3200) Phaethon | - |
dc.subject.keywordAuthor | DESTINY+ | - |
dc.subject.keywordAuthor | Phase ratio | - |
dc.subject.keywordAuthor | Photometry | - |
dc.subject.keywordAuthor | Regolith particles | - |