X-ray polarimetry at INAF Paolo Soffitta IAPS/INAF (Rome, Italy) 1 IAPS/INAF : Enrico Costa, Sergio Fabiani, Fabio Muleri, Alda Rubini, Paolo Soffitta.
INTRODUCTION TO SPECTROSCOPIC METHODS OF ANALYSIS LECTURE 1 1.
Feb. 9, 2011 Fourier Transforms Polarizations. Fourier Transforms A function’s Fourier Transform is a specification of the amplitudes and phases of sinusoidals,
CHAPTER 1 Instrumental Analysis
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OPTICAL MINERALOGY Dr. AZZA RAGAB. Gamma rays (3x10 -9 m) → Radio waves (3x10 6 m) The electromagnetic spectrum (Light) -It is a form of energy, which.
THE POLARIZATION OF LIGHT The electromagnetic theory, Specifically requires that the vibrations be traverse, being therefore entirely confined to the plane.
Fluorescence Depolarization Martin Cole, Faraz Khan Physics 200 Professor Newman biolab/tpe/tutor/fpa/anis2.html.
Lecture 2 INTRODUCTION TO SPECTROMETRIC METHODS Copyright ©The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 6 An Introduction to Spectrometric Methods Spectrometric methods are a large group of analytical methods that are based on atomic and molecular.
X-ray photoelectric polarimetry with the Gas Pixel Detector Paolo Soffitta IASF-Rome/INAF Workshop on X-ray Polarimetry 2011-12-7 Tsinghua University Beijing.
Polarization in astronomy and its registration. EDIPO project. Sergey Guziy on behalf of a large collaboration (NNU, Nikolaev, Ukraine) (IAA-CSIC Granada,
