Description of Individual Course Units
Course Unit CodeCourse Unit TitleType of Course UnitYear of StudySemesterNumber of ECTS Credits
9101015352018Cromospheric Activity IElective118
Level of Course Unit
Second Cycle
Objectives of the Course
Under solar-stellar relation, from x-ray to radio region, identifying and describing the cool spots as a magnetic activity pattern, which is originated by magnetic structures.
Name of Lecturer(s)
Doç. Dr. Hasan Ali DAL
Learning Outcomes
1- Considering the basic physical processes, to be able to obtain the mathematical results in the areas of astrophysics.
2- Getting some relations between the physical interactions and the radiation processes, to get some knowledge about astrophysical processes and stellar evolutions.
Mode of Delivery
Face to Face
Prerequisites and co-requisities
Recommended Optional Programme Components
None
Course Contents
- The stars exhibitng spot activity in the HR Diagram - The discussions on the dynamo and its processes about spot activity. - The discussions on the photometrical patterns of spot activity. - The observing technicof the photometrical patterns of spot activity. - To dertermination of the photometrical patterns of spot activity - The discussions on the spectral patterns of spot activity. - The observing technicof the spectral patterns of spot activity. - To dertermination of the spectral patterns of spot activity
Weekly Detailed Course Contents
WeekTheoreticalPracticeLaboratory
1Spot activity in the HR Diagram
2Dynamo and its processes1
3Photometrical patterns of spot activity
4Photometrical patterns of spot activity1
5Observing technicof the photometrical patterns of spot activity
6Observing technicof the photometrical patterns of spot activity2
7Dertermination of the photometrical patterns of spot activity
8Dertermination of the photometrical patterns of spot activity2
9First Exam
10Spectral patterns of spot activity
11Spectral patterns of spot activity2
12Observing technicof the spectral patterns of spot activity
13Observing technicof the spectral patterns of spot activity2
14Dertermination of the spectral patterns of spot activity
15Dertermination of the spectral patterns of spot activity2
16Final Exam
Recommended or Required Reading
- Solar Type Activity in Main Sequence Stars (Gershberg, R. E. 2005, Solar-Type Activity in Main-Secauence Stars, New York: Springer Press) - Solar and Stellar Magnetic Activity (Zwaan, S., 2003, Solar and Stellar Magnetic Activity, New York, Cambridge Press)
Planned Learning Activities and Teaching Methods
Activities are given in detail in the section of "Assessment Methods and Criteria" and "Workload Calculation"
Assessment Methods and Criteria
Term (or Year) Learning ActivitiesQuantityWeight
SUM0
End Of Term (or Year) Learning ActivitiesQuantityWeight
SUM0
SUM0
Language of Instruction
Turkish
Work Placement(s)
None
Workload Calculation
ActivitiesNumberTime (hours)Total Work Load (hours)
Midterm Examination133
Final Examination133
Attending Lectures14342
Seminar24896
Individual Study for Homework Problems23060
Individual Study for Mid term Examination14848
Individual Study for Final Examination14848
TOTAL WORKLOAD (hours)300
Contribution of Learning Outcomes to Programme Outcomes
PO
1
PO
2
PO
3
PO
4
PO
5
PO
6
PO
7
PO
8
PO
9
PO
10
PO
11
LO1 543545  4 
LO2           
* Contribution Level : 1 Very low 2 Low 3 Medium 4 High 5 Very High
 
Ege University, Bornova - İzmir / TURKEY • Phone: +90 232 311 10 10 • e-mail: intrec@mail.ege.edu.tr