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Main Authors: Chen, Sihe, Adams, Danica, Fan, Siteng, Gao, Peter, Young, Eliot, Yung, Yuk
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2402.00510
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author Chen, Sihe
Adams, Danica
Fan, Siteng
Gao, Peter
Young, Eliot
Yung, Yuk
author_facet Chen, Sihe
Adams, Danica
Fan, Siteng
Gao, Peter
Young, Eliot
Yung, Yuk
contents Combining findings from New Horizons' suite of instruments reveals a bimodal haze particle distribution within Pluto's atmosphere, which haze models have not been able to reproduce. We employ the photochemical and microphysics KINAERO model to simulate seasonal cycles and their impact on the haze distribution. We find that the smaller spherical particle mode can be generated through photochemistry and coagulation, while the larger aggregate mode are formed by surface volatile deposits sublimating and subsequently lofting such particles upwards.
format Preprint
id arxiv_https___arxiv_org_abs_2402_00510
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Deciphering Pluto's Haze: How a Solar-Powered Vapor-Pressure Plume Shapes Its Bimodal Particle Size Distribution
Chen, Sihe
Adams, Danica
Fan, Siteng
Gao, Peter
Young, Eliot
Yung, Yuk
Earth and Planetary Astrophysics
Combining findings from New Horizons' suite of instruments reveals a bimodal haze particle distribution within Pluto's atmosphere, which haze models have not been able to reproduce. We employ the photochemical and microphysics KINAERO model to simulate seasonal cycles and their impact on the haze distribution. We find that the smaller spherical particle mode can be generated through photochemistry and coagulation, while the larger aggregate mode are formed by surface volatile deposits sublimating and subsequently lofting such particles upwards.
title Deciphering Pluto's Haze: How a Solar-Powered Vapor-Pressure Plume Shapes Its Bimodal Particle Size Distribution
topic Earth and Planetary Astrophysics
url https://arxiv.org/abs/2402.00510