PPT-Polarimetric shapes of spectral lines in solar observations

Egidio Landi DeglInnocenti Dipartimento di Fisica e Astronomia Università di Firenze Italia Banja Koviljaca May 1317 2013 9th Serbian Conference on Spectral Line Shapes in Astrophysics Line shapes I. quadrature. observations. Janusz Nicewicz. Introduction. ESA Model. Observations. Results. Conclusions . Introduction. . Mean distance 1AU. Mass . 1.9891×10. 30.  kg. Mean diameter 1,392,684 km. Fabry-Pérot. interferometers. Alex A. Takeda . Aug. 18, 2010. Mentor . Dr. Alexander . Kutyrev. Zodiacal light. Sunlight scattered by dust particles in the solar system. Affects measurements of near-infrared extragalactic background light (EBL). Robert Minchin. Spectral Lines. What is a Spectral Line?. Types of Spectral Line. Molecular Transitions. Linewidths. Reference Frames. When a Coconut falls…. Bang!. h. Energy released = . mgh. When an electron falls…. The First Step in Quantitative Spectral Analysis. Richard Gray. Appalachian State University. MK Spectral Classification: 1943 – 2013. 70 years of contributions to stellar astronomy. Discovery of the spiral structure of the Galaxy (Morgan, . Units: 1 nanometer= 10. -9. meters!. . Different. . wavelengths . correspond. . to. . different. . colors!. If you pass white light through a prism, it separates into its component colors.. R. Element of Art. Element of Art. An element of art is a basic visual symbol that an artist uses to create visual art. These elements include: colour, line, shape, form, space and texture. It is through a blending of these elements that you are able to see the work as the artist meant you to see it.. to purpose, consistency in character, the agreement . of . all the elements in a work of art.. . The principle of harmony. The trees, the house,. . and the sky are all in harmony, but the beauty of the picture is marred by the presence of the unrelated objects in the foreground. . Mark Weber, Joseph . Pagaran. , Stefan Noël, . Klaus . Bramstedt. , and John P. Burrows. weber@uni-bremen.de. TOSCA Workshop, Berlin, 14-16 April 2012. Motivation. x. SCIAMACHY . observes. SSI in UV/. Ellen Howell (Arecibo Observatory) and Amy Lovell (Agnes Scott College). Hyakutake. Comets: where do they come from?. Icy bodies ejected during giant planet formation. Remnants of early solar system. 1. Outline. Introduction. Scope . Weather Radar. Polarimetric Weather Radar . Operation. Case Study. POLDIRAD. Analysis: Benefits of Polarimetric Weather Radar. Rain Rate estimates. Errors. Conclusion. Properties of Shapes. Number of sides. Number of angles. Number of lines of symmetry. Regular or irregular. Right Angles. Parallel lines. Shapes. Quadrilaterals. Triangles. Polygons. Key Words. Regular Shapes. in vivo. measurements. Angelo Pierangelo. 1. Jérémy . Vizet. 1. , . Jean . Rehbinder. 1. , . Stanislas . Deby. 1. , . Stéphane . Roussel. 1. , . Tatiana . Novikova. 1. , . Ranya. Soufan. 2. , . Catherine . Ken Phillips. Scientific Associate, Natural History Museum, and Honorary . Prof.. , QUB. 1. Solar Corona: Physical Properties. Solar corona has very . high temperatures:. . 10. 6. K – 2. ×10. 6. Rachel Hetlyn, Boston University. August 1, 2012. What is SOLARIS?. Climate Absolute Radiance and Refractivity Observatory (CLARREO). Calibration Demonstrator System (CDS). Thermal control of attenuators.