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Welcome to the Synchrotron Radiation Course

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Presentation on theme: "Welcome to the Synchrotron Radiation Course"— Presentation transcript:

1 Welcome to the Synchrotron Radiation Course

2 Synchrotron Radiation 2011, preliminary plan (up-dated on Studentportalen):
Introduction, history, sources of electromagnetic radiation, accelerating charged particles at high speed. Basic ideas 1: Properties of synchrotron radiation: angular distribution, energy distribution, power, brilliance, polarization, time structure, coherence. Basic ideas 2 Insertion devices: Wigglers and Undulators MAX-lab user meeting    Reports from the user meeting  Optical properties in the soft X-ray range. Absorption-Reflection-Transmission Beamlines and monochromators Free electron lasers xxxxx: Laborations at MAX-lab xxxx Lab presentations, suggested applications xxxx Presentations by experts in various fields xxxxx Dissertations The examination includes handed-in solved problems, performing a laboratory work. In addition, you will write a beamtime proposal, which you must defend in a ‘dissertation’, and you will also act as opponent on one occasion. These dissertations will take place during December.and the beginning of next year. We use Attwood: ‘Soft X-ray and Extreme Ultraviolet Radiation’, and lecture notes.

3 Links to info about synchrotron radiation: David Attwood and guest speakers lecture on his book: News, information, and educational materials about the world’s synchrotron and free electron laser light source facilities: Short history of synchrotron radiation:

4 The cyclotron… as seen by…
…the inventor …the user …the governmental funding agency Catoons by David Judd and Ron MacKenzie, LBNL1966

5 Phys. Rev. 71, 829–830 (1947)

6 Phys. Rev. 91, 1577 (1953)

7 Synchrotron Radiation Around the Globe
From Altarelli and Salam, Europhysics News (2004) Vol. 35 No. 2

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10 Geometry and Electronic Structure
Properties in terms of how electrons and nuclei move

11 Slide from a presentation by Jo Stöhr, Stanford
Today Lasers X-rays Ultrafast Slide from a presentation by Jo Stöhr, Stanford

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