Course detail

Geodetical Astronomy and Space Geodesy II

FAST-HE06Acad. year: 2013/2014

Dynamic of satellite orbit in gravity field - problem of two bodies.
Kepler’s laws.
Disturbed and undisturbed satellite movement.
Observation methods of tracking satellites.
Global navigational satellite systems with particular view to GPS and it‘s application.
Other techniques of satellite geodesy(SLR, satellite altimetry, DORIS, satellite Earth gravity missions).

Language of instruction

Czech

Number of ECTS credits

Mode of study

Not applicable.

Guarantor

doc. Ing. Radovan Machotka, Ph.D.

Department

Institute of Geodesy (GED)

Learning outcomes of the course unit

Introduction with spatial geodesy, particularly with satellite geodesy. Students become familiar with dynamism of satellite motion in gravitational field, with methods of terrestrial satellites tracking and results processing.

Prerequisites

Kinematics and dynamics of motion, Newton‘s motional laws, Newton‘s gravitational law, law of refraction and reflection of the light, dispersion of wave motion, methods of modulation of waves, field of dissipative forces, physical conditions in Earth‘s atmosphere.

Co-requisites

None

Planned learning activities and teaching methods

Course is composed from lectures and exercises. Practical astrogeodetic and space geodesy tasks are included in the excercises.Forms of teaching are specified in the article 7 of BUT Rules for Studies and Examinations.

Assesment methods and criteria linked to learning outcomes

Conditions for successful termination of subject are exercises attendance in accordance with BUT Rules for Studies, correct solution of all submitted individual tasks and more then a half of points from final written test.

Course curriculum

1. Problem of two bodies, Kepler’s laws.
2. Disturbed and undisturbed satellite movement.
3. Optical and electronic observation methods of tracking satellites.
4. Use of satellites for solving basic problems.
5. Basic methods of determination of position.
6. GPS – system description
7. GPS – application in surveying
8. GPS – receivers, related settlements
9. Gravitational models of the Earth
10. Radio interferometry from very long bases and it’s application (absolute and differential methods, arc method, network VLBI).

Work placements

Not applicable.

Aims

Introduction with spatial geodesy, particularly with satellite geodesy. Students become familiar with dynamism of satellite motion in gravitational field, with methods of terrestrial satellites tracking and results processing.

Specification of controlled education, way of implementation and compensation for absences

Extent and forms are specified by guarantor’s regulation updated for every academic year.

Recommended optional programme components

None

Prerequisites and corequisites

Not applicable.

Basic literature

Fixel Jan: Geodetická astronomie I a základy kosmické geodézie. VUTIUM, 2000. (CS)
MACHOTKA, R.; FIXEL, J.: GEODETICKÁ ASTRONOMIE A KOSMICKÁ GEODÉZIE II, KOSMICKÁ GEODÉZIE. VUT v Brně - studijní opora, 2007. (CS)

Recommended reading

Not applicable.

Classification of course in study plans

  • Programme N-P-C-GK Master's

    branch G , 1 year of study, summer semester, compulsory
    branch GD , 1 year of study, summer semester, compulsory

Type of course unit

 

Lecture

26 hod., optionally

Teacher / Lecturer

doc. Ing. Radovan Machotka, Ph.D.

Syllabus

1. Problem of two bodies, Kepler’s laws.
2. Disturbed and undisturbed satellite movement.
3. Optical and electronic observation methods of tracking satellites.
4. Use of satellites for solving basic problems.
5. Basic methods of determination of position.
6. GPS – system description.
7. GPS – application in surveying.
8. GPS – receivers, related settlements.
9. Satellite altimetry, satellite Earth gravity missions, Earth Gravity Models.
10. Other techniques of satellite geodesy (SLR, DORIS).

Exercise

26 hod., compulsory

Teacher / Lecturer

doc. Ing. Radovan Machotka, Ph.D.

Syllabus

Introduction. Computation of astronomical azimuth from Sun or Polaris observation, task 1.
Preparation of observation program, computer planetarium and its use, task 2.
Determination of astronomical azimuth using the Polaris - observation.
Determination of astronomical azimuth using the Polaris - repeated observation, task 3.
Ephemeris of GPS satellite computation - non disturbed motion, task 4a.
Ephemeris of GPS satellite computation - disturbed motion, task 4b.
Free time for task 4 finishing.
Networks of GNSS permanent stations.
Final test.