Download presentation

Presentation is loading. Please wait.

Published bySofia Alvarez Modified over 4 years ago

1
Can Vesta have a polar cap? Eleonora Ammannito INAF/IFSI - Roma CISAS - Padova CISAS-UPD

2
The model Time-dependent, unidimensional partial differential equations, expressing the conservation of energy (heat diffusion) and mass (gas diffusion), in the general form = density, = flux, Q = source term PDE's are solved numerically in discrete time steps on a discrete grid

3
The initial conditions Seasonal variation of the temperature at different latitudes on the surface of Vesta. It was condidered the equilibrium between the solar irradiance at the Vestas distance from the Sun at each latitude and the thermal emission of the body. Parametri orbitali: Parametri fisici:

4
Preliminary indications

Similar presentations

Presentation is loading. Please wait....

OK

PARTIAL DIFFERENTIAL EQUATIONS

PARTIAL DIFFERENTIAL EQUATIONS

© 2018 SlidePlayer.com Inc.

All rights reserved.

Ads by Google

Ppt on conservation of minerals Ppt on cross site scripting xss Ppt on traffic light control using image processing Figurative language for kids ppt on batteries Ppt on classical economics theories Ppt on ashwagandha plant Ppt on save water save earth Doc convert to ppt online form Ppt on conceptual art history Ppt on fibonacci numbers definition