Titlebook: Lectures on Solar Physics; H. M. Antia,Arvind Bhatnagar,Peter Ulmschneider Book 2003 Springer-Verlag Berlin Heidelberg 2003 Chromosphere.C

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on the winning thesis of the EURON Georges Giralt award.Modeling and predicting human and vehicle motion is an active research domain.Owing to the difficulty in modeling the various factors that determine motion(e.g. internal state, perception) this is often tackled by applying machinelearning techn

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B. N. Dwivedimotion(e.g. internal state, perception) this is often tackled by applying machinelearning techniques to build a statistical model, using as input a collectionof trajectories gathered through a sensor (e.g. camera, laser scanner), and thenusing that model to predict further motion. Unfortunately, mos

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P. K. Manoharanmotion(e.g. internal state, perception) this is often tackled by applying machinelearning techniques to build a statistical model, using as input a collectionof trajectories gathered through a sensor (e.g. camera, laser scanner), and thenusing that model to predict further motion. Unfortunately, mos

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Instrumentation and Observational Techniques in Solar Astronomy,ur Sun being the nearest star, shows intricate surface details and a wide variety of dynamic phenomena. These range in size from a few kilometres to millions of kilometres and in the temporal domain from a fraction of a second to decades. In addition, the Sun displays a great variety of magnetic and

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Solar Interior and Seismology,cillations have been measured bythe ground based Global Oscillation Network Group project and the space based Michelson Doppler Imager. Each of these modes is trapped in a different region of the solar interior and hence its frequencyis sensitive to structure and dynamics in the corresponding region

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The Active and Explosive Sun,emporal scales. The most notable among these is the solar activity cycle of 11 years, or magnetic cycle of 22 years. On shorter time scales of a few seconds to several hours, spectacular explosive events occur in the solar atmosphere, such as, solar flares, prominence eruptions, and coronal mass eje

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Magnetic Flux Tubes and Activity on the Sun,fundamental aspects of magnetic activity: (a) the generation, storage and emergence of magnetic fields from the solar interior; (b) the nature of the surface magnetic fields, especially in the form of small-scale flux tubes; and (c) dynamical processes in flux tubes and heating of the magnetic chrom

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