PPT-Probing CO freeze-out and desorption in protoplanetary disks

Chunhua Qi HarvardSmithsonian CfA Qi et al 2008 Qi et al in prep Image credit Bill Saxton NRAO Star Formation Stages Sketch of the physical and chemical structure of a 15 Myr old protoplanetary disk around a Sunlike star. 1 CD6 SE Fig 1 CD XT SE Fig 1 CD8 SE Fig 1 CD ransport brPage 3br 325 1015 Reading 325 325 Fig 3 17 59 57 Fig 2 1 1 1 brPage 4br Cyrus CD 6 SE 2 CD 8 SE 2 CD XT SE 2 CD T TRANSPORT User Instructions 1 IMPORTANT Read before operating this equipme brPage 1br OUT 12 OUT 34 OUT 56 OUT 7 OUT KICK SNARE OM OM HI GAN UKELELE ZITHER BANJO ELEC GTR OUST GTR OH R OH L OWBELL GAN HI VO AL BASS DIRE BASS MP SOFT S N R SOFT S N L AN G S NTH THERE 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. Done by : Alaa Al-Harran. What is Deep Freeze ?. Deep Freeze, by . Faronics. , is an application available for the Microsoft Windows, Mac OS X, and SUSE Linux operating systems which allows system administrators to protect the core operating system and configuration files on a workstation or server by restoring a computer back to its original configuration each time the computer restarts.. 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. RAID (Redundant Arrays of Independent Disks). Disk . organization technique that manages a large number of disks, providing a view of a single disk of. High capacity and high speed up using multiple disk in parallel. 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. 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. Share of sales hasn’t been taken away from other types, as voucher sites tend to overwrite each other (50-60% on average for . key publishers. . on programme). Conversion rate however has dropped considerably. Sahil. Singla. . (Carnegie Mellon University). Joint . Work (. Partly) With . ANUPAM GUPTA . and . VISWANATH NAGARAJAN. (2. nd. Feb, 2018). Combinatorial Optimization. Given a . Finite . Universe. Matthew . Marcinkowski. Group Meeting. June 27, . 2016. Adsorption and Desorption. E. ads. E. ads. Non-activated, non-dissociative adsorption. Activated, dissociative process.. Adsorption and Desorption. Two main types: Magnetic and Optical. Random access to memory. The hardware must be controlled by driver software called the “controller” in order to be used. Hard Disks, RAID, and Error Handling. Don Porter. Portions courtesy Emmett . Witchel. 1. Quick Recap. CPU Scheduling. Balance competing concerns with heuristics. What were some goals?. No perfect solution. Today: Block device scheduling. Background. EPPR 15-05 Slide 5, India proposal to delete Need for FFD for Grade A.. EPPR 15-13 Japan Proposal slide 7 on FFD requirement for Grade A. Discussion during EPPR 15 on this point and need for more data from India..