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Saturn's Cloud Structure And Temporal Evolution From Hubble Space Telescope Images.pdf

sph.etal.2005.pdf
Preview of Saturn's Cloud Structure and Temporal Evolution from Hubble Space Telescope Images
🔗 Source: web.archive.org
📊 Size: 2.31 MB
📄 Pages: 20 pages
⬇️ Downloads: 34

Summary

- Objective: Study Saturn's cloud structure and temporal evolution using Hubble Space Telescope images (1994-2003).
- Method: Analyzed calibrated WFPC2 images covering near-UV to near-IR, including the 890 nm methane band. Used a radiative transfer code to model the atmosphere.
- Findings:
- Two haze layers above a thick ammonia ice cloud.
- Upper thin haze (1-10 mbar, radii ∼0.2 µm) is persistent and shows seasonal variations in optical thickness.
- Lower thicker haze (50-100 mbar to ∼400 mbar) has strong latitudinal dependence (τ ∼20-40 at equator, τ ∼5 at pole) and shows mid-term changes (months to 1-2 years) and long-term decrease in blue single-scattering albedo.
- Significance: Understanding cloud and haze properties is crucial for atmospheric dynamics and circulation studies on Saturn.

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Description

Saturn's cloud structure and temporal evolution studied using 10 years of Hubble Space Telescope images (1994-2003).

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  • File Format: PDF
  • File Size: 2.31 MB
  • Pages: 20
  • Language: EN
  • Total Downloads: 34
  • Last Updated: 6 days ago

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