- Docente: Tiziano Maestri
- Credits: 6
- SSD: FIS/06
- Language: Italian
- Teaching Mode: Traditional lectures
- Campus: Bologna
- Corso: First cycle degree programme (L) in Astronomy (cod. 8004)
Learning outcomes
At the end of the course the Student is able to analyze the planetary atmospheres as physical systems. He learns the phenomenology and equations governing the fundamental physical processes occurring in the planetary atmospheres. The Student is able to interpret simplemodels ofgreenhouse effect and to link climatic patterns with orbital parameters of Planets.
Course contents
1) Origin and composition of the Solar System
Theories on the origin of the solar system. Main physical laws
governing its configuration. The planets: active and inactive
surfaces, internal structures. Satellites and rings. Minor bodies
of the solar system: nanoplanets, asteorids, comets, meteorits.
Transneptunian objects.
2) Main characteristics of the Earth and Planets
atmosphereComposition and chemical evolution. Mass
escape mechanisms (Jeans Escape). Mean thermal structure. The
Stratosphere and the role of the Ozone layer. Thermal vertical
profile of internal and external planets.
3) Thermodynamics of the Atmosphere
Air parcel concept. The gas laws applied to the real atmospheres.
Hydrostatic balance and hypsometric equation. Dry air: adiabatic
processes and lapse rate. Diabatic processes and diabatic
stratification.
4) Hydrostatic Stability Buoyancy force and
vertical velocities. Static stability and the Brunt Vaisala
frequency. Categories of static stability for dry air and
convection. Auto-convective gradient.
5) Water Vapour and Condensed Phase in the
Atmosphere Water vapour saturation pressure and phase
changes. Adiabatic lapse rate for saturated air (pseudo-adiabats).
Condensed states in atmospheric planets: clouds.
6) Fundamentals of Radiative Transfer
Electromagnetic spectrum. Solid angle and main radiometric
quantities. Black body radiance and its fundamental
laws.Kirchhoff's law. The differential equation of the
radiative transfer for absorbing and emitting
processes.Schwarzschild's solution for a plane parallel
atmosphere.
7) The Sun The structure. Luminosity and
measure of the Solar Constant. The solar spectrum. Sun radiation
and atmospheric particles and gas interaction.
8) Radiative Equilibrium and emission temperature of a
Planet Albedo. Basic model for a planet in radiative
balance. Emission temperature and variation of the solar constant
and of the spherical albedo. Mean surface temperature and emission
temperature.
9) Greenhouse Effect Greenhouse 1-d model.
Greenhouse parameter. The Venus case and the Sandstrom theorem.
Radiative equilibrium in a plane parallel and grey
atmosphere.Runaway green-house effect (Venus, Earth and
Mars). Time radiative constants.
10) Basic of atmospheric dynamics Basic
equations. General circulation in the Earth atmosphere. Cases
analysis: circulation on Venus, diurnal winds on Mars and
convective processes on Jupiter.
11) Simple Climatic Models 0-d models and
feedback processes. Energy balance 1-d climatic models:
Budyko-Sellers.Milankovitch theory: orbital parameters and
climatic patterns. Experimental data and glacial eras.
Readings/Bibliography
T. Maestri. Planetary Atmospheres. Available directly from the
teacher.
C. Bartolini, M. Benelli, L. Solmi: DVD-ROM "Viaggio nel Sistema Solare" (2011) available at the Astronomy Dep.
John M. Wallace and Peter V. Hobbs. Atmospheric Science: An Introductory Survey Academic Press, 1997.
Joseph W. Chamberlain and Donald M. Hunten. Theory of Planetary Atmospheres: An Introduction to Their Physics and Chemistry Aca- demic Press, 1987.
D. L. Hartmann. Global Physical Climatology Academic Press, 1994.
Murry L. Salby Fundamentals of Atmospheric Physics Academic Press, 1996.
Teaching methods
The teacher will discuss the program content by using the
blackboard and by exploiting the video projector. Simple exercises
will be solved during the classes.
Assessment methods
Oral test and discussion of a brief research paper (prepared by the student) which analyze a specific topic.
Teaching tools
The following items will be available to the Students:
* Lectures notes (on paper and/or electronics).
* Scientific articles useful to the investigation of specific
research lines.
* Software algorithms for the numerical solution of specific
problems.
* Materials on dvd
* Bibliography and references
Office hours
See the website of Tiziano Maestri