PPT-Processes in Protoplanetary Disks

Phil Armitage Colorado Processes in Protoplanetary Disks Disk structure Disk evolution Turbulence Episodic accretion Single particle evolution Ice lines and persistent radial structure Transient structures in disks. All Fujifilm floppy disk manufacturing plants worldwide have been awarded ISO9002 certification your assurance of stringent quality control at every step of the production process And Fujifilm floppy disks have been successfully tested beyond 30 mil Protoplanetary. Disks. Colette Salyk. National Optical Astronomy Observatory. Credit: JPL-Caltech/T. Pyle (SSC). Credit: NASA. ?. Why studying . protoplanetary. . disks is important for understanding habitability. Packaging samples for irradiation. Overview. Care must be taken while packaging groundmass and mineral separates to prevent loss of sample and cross-contamination of adjacent samples.. Because the geometric position of samples and standards is critical, labelling throughout the process is important.. Lecture by C.P. Dullemond. Institute for Theoretical Astrophysics. Heidelberg University. Image . Credit. : NASA. The Big Questions. After C. Mordasini. > 10 billion galaxies in the Universe. 100 billion stars in each. to Achieve . Temporal Coverage of Objects and . Its Surveillance . Application. You-. Chiun. Wang, Yung-Fu Chen, and Yu-. Chee. Tseng. IEEE TRANSACTIONS ON MOBILE . COMPUTING 2011. Outline. . Introduction. - High-R Spectroscopy -. TMT science & instrument workshop. 　. Oct. 16-17, 2013 @ Tokyo. Hideko Nomura. . (Tokyo Tech.). Matthew J. Richter (UC Davis). §1 Introduction. From protoplanetary disk to planets. a. nd stellar multiplicity. Insights from recent surveys. Gaspard . Duchêne. (UC Berkeley, Obs. Grenoble). © NASA/JPL/Caltech. Planets in multiple systems?. © . LucasFilm. Ltd.. They must exist!. Phil Armitage. Colorado. Processes in Protoplanetary Disks. Disk structure. Disk evolution. Turbulence. Episodic accretion. Single particle evolution. Ice lines and persistent radial structure. Transient structures in disks. ASHIMA KALRA . . Hard disks.. . Floppy disks.. . CD ROMs.. . DVDs.. . INDEX. ….. Floppy Disks. The first floppy disks were 8 Inches in diameter.They hold upto 256 KB.. The next generation were 5.25 inches in diameter.It Could hold up to 1.44 MB.It is a standard one.. and RAID. Outline. Disks. Disk scheduling algorithms. Redundancy in storage . systems, RAID. 2. Disk Geometry. Disks have multiple platters. Each platter has . an arm and a head for accessing data. The arms for the different platters move together. Ofir Weisse. EECS 582 – W16. 1. About the paper. Published in 1988. Summarized existing technologies. EECS 582 – W16. 2. Motivation – What’s In the Box? . (That we call a computer). EECS 582 – W16. Phil Armitage. Colorado. Motivation. What can we directly observe?. Dust. m. m-mm. Gas – . emission &. kinematics. (CO other. molecules, . H. 2. hard). Limited. direct . time . dependence. Evolution. Insights from recent surveys. Gaspard . Duchêne. (UC Berkeley, Obs. Grenoble). © NASA/JPL/Caltech. Planets in multiple systems?. © . LucasFilm. Ltd.. They must exist!. Planets in multiple systems!. Reads and writes are equally fast.. Arrays of these disks are used to provide highly reliable storage.. Increasingly popular as they are fast and do not contain moving parts.. Magnetic Disks.. . What is a magnetic disk and how it works.