Description

The composition of planets and their volatile contents are intimately connected to the structure and evolution of their parent protoplanetary disks. The transport of momentum and volatiles is often parameterized

The composition of planets and their volatile contents are intimately connected to the structure and evolution of their parent protoplanetary disks. The transport of momentum and volatiles is often parameterized by a turbulent viscosity parameter $\alpha$, which is usually assumed to be spatially and temporally uniform across the disk.

5.42 MB application/pdf

Download count: 0

Details

Contributors
Date Created
  • 2018
Resource Type
  • Text
  • Collections this item is in
    Note
    • Partial requirement for: Ph.D., Arizona State University, 2018
      Note type
      thesis
    • Includes bibliographical references (pages 160-167)
      Note type
      bibliography
    • Field of study: Astrophysics

    Citation and reuse

    Statement of Responsibility

    by Anusha Kalyaan

    Machine-readable links