Presentation is loading. Please wait.

Presentation is loading. Please wait.

Using the Grid for Astronomy Roy Williams, Caltech.

Similar presentations

Presentation on theme: "Using the Grid for Astronomy Roy Williams, Caltech."— Presentation transcript:

1 Using the Grid for Astronomy Roy Williams, Caltech

2 Enzo Case Study Simulated dark matter density in early universe N-body gravitational dynamics (particle-mesh method) Hydrodynamics with PPM and ZEUS finite-difference Up to 9 species of H and He Radiative cooling Uniform UV background (Haardt & Madau) Star formation and feedback Metallicity fields

3 Adaptive Mesh Refinement (AMR) multilevel grid hierarchy automatic, adaptive, recursive no limits on depth,complexity of grids C++/F77 Bryan & Norman (1998) Source: J. Shalf

4 Distributed Computing Zoo Grid Computing Also called High-Performance Computing Big clusters, Big data, Big pipes, Big centers Globus backbone, which now includes Services and Gateways Decentralized control Cluster Computing local interconnect between identical cpus Peer-to-Peer (Napster, Kazaa) Systems for sharing data without centeral server Internet Computing Screensaver cycle scavenging eg SETI@home, Einstein@home,, etcSETI@homeEinstein@home Access Grid A videoconferencing system Globus A popular software package to federate resources into a grid TeraGrid A $150M award from NSF to the Supercomputer centers (NCSA, SCSC, PSC, etc etc)

5 The World Wide Web provides seamless access to information that is stored in many millions of different geographical locations In contrast, the Grid is an emerging infrastructure that provides seamless access to computing power and data storage capacity distributed over the globe. What is the Grid?

6 Grid was coined by Ian Foster and Carl Kesselman The Grid: blueprint for a new computing infrastructure. Analogy with the electric power grid: plug-in to computing power without worrying where it comes from, like a toaster. The idea has been around under other names for a while (distributed computing, metacomputing, …). Technology is in place to realise the dream on a global scale. What is the Grid?

7 The GRID middleware: Finds convenient places for the scientists job (computing task) to be run Optimises use of the widely dispersed resources Organises efficient access to scientific data Deals with authentication to the different sites Interfaces to local site authorisation / resource allocation Runs the jobs Monitors progress Recovers from problems … and …. Tells you when the work is complete and transfers the result back! What is Middleware?

8 Grid as Federation Grid as a federation independent centers flexibility unified interface power and strength Large/small state compromise

9 Three Big Ideas of Grid Federation and Uniformity –independent management; uniform face; open standards Trust and Security –access policy; uniform authentication/authorization Distance doesnt matter –20 Mbyte/sec, global file system

10 DOE Science Grid NSF National Virtual Observatory NSF GriPhyN/iVDGL DOE Particle Physics Data Grid NSF TeraGrid DOE Earth Systems Grid NEESGrid DOH BIRN UK e-Science Grid EUROGRID DataGrid (CERN,...) EuroGrid (Unicore) DataTag (CERN,…) GridLab (Cactus Toolkit) CrossGrid (Infrastructure Components) Grid projects in the world

11 TeraGrid Wide Area Network

12 TeraGrid Components Compute hardware –Intel/Linux Clusters, Alpha SMP clusters, POWER4 cluster, … Large-scale storage systems – hundreds of terabytes for secondary storage Very high-speed network backbone – bandwidth for rich interaction and tight coupling Grid middleware – Globus, data management, … Next-generation applications

13 TeraGrid Resources ANL/ UC Indiana U NCSAORNLPSCPurdue U SDSCTACC Compute Resources 1 Tflop1 TFlop35 Tflop16 Tflop18 Tflop24 Tflop8 Tflop Online Storage20 TB6 TByte700 TByte 200 TByte 28 Tbyte1000 TByte 50 TByte Archival Storage 150 Tbyte 5000 Tbyte 2400 Tbyte 36 Tbyte7200 Tbyte 2000 Tbyte Global FS220 Tbyte 20 Tbyte220 Tbyte Data Collections Yes Visualization Yes Instruments Yes Network (Gb/s,Hub) 30 CHI 10 CHI 30 CHI 10 ATL 30 CHI 10 CHI 30 LA 10 CHI

14 The TeraGrid Vision Distributing the resources is better than putting them at one site Build new, extensible, grid-based infrastructure –New hardware, new networks, new software, new practices, new policies Leverage homogeneity –Run single job across entire TeraGrid –Move executables between sites Catch-phrase: Open, Deep and Wide –Open to US science community –Heroic computing possible by programming Unix –Easy to use through science gateways

15 TeraGrid Allocations Policies Any US researcher can request an allocation –

16 Wide Variety of Usage Scenarios Tightly coupled simulation jobs storing vast amounts of data, performing visualization remotely as well as making data available through online collections (ENZO) Thousands of independent jobs using data from a distributed data collection (NVO) Science Gateways – "not a Unix prompt"! –from web browser with security –SOAP client for scripting –from application eg IRAF, IDL

17 Running jobs

18 Account Security Username/Password –weak security, too many holes –deprecated in many places SSH keys –put public key on remote machine –serves as single sign-on X.509 Certificates –Proves identity –Flexible

19 Ways to Submit a Job 1. Directly to PBS Batch Scheduler –Simple, scripts are portable among PBS TeraGrid clusters 2. Globus common batch script syntax –Scripts are portable among other grids using Globus 3. Condor-G = Condor + Globus 4. Use a science gateway, eg Nesssi specific tasks, easy to use

20 PBS Batch Submission Single executables to be on a single remote machine –login to a head node, submit to queue Direct, interactive execution –mpirun –np 16./a.out Through a batch job manager –qsub my_script where my_script describes executable location, runtime duration, redirection of stdout/err, mpirun specification… ssh –qsub –v "FILE=f544" –qstat or showq –ls *.dat –pbs.out, pbs.err files

21 Remote submission Through globus –globusrun -r [some-teragrid-head- node] -f my_rsl_script where my_rsl_script describes the same details as in the qsub my_script! Through Condor-G –condor_submit my_condor_script where my_condor_script describes the same details as the globus my_rsl_script!

22 Condor-G A Grid-enabled version of Condor that provides robust job management for Globus clients. –Robust replacement for globusrun –Provides extensive fault-tolerance –Can provide scheduling across multiple Globus sites –Brings Condors job management features to Globus jobs

23 Condor DAGMan Manages workflow interdependencies Each task is a Condor description file A DAG file controls the order in which the Condor files are run

24 Cluster Supercomputer 100s of nodes purged /scratch parallel file system /home (backed-up) login node job submission and queueing (Condor, PBS,..) user metadata node parallel I/O global file system

25 MPI parallel programming Each node runs same program first finds its number (rank) and the number of coordinating nodes (size) Laplace solver example Algorithm: Each value becomes average of neighbor values node 0node 1 Parallel: Run algorithm with ghost points Use messages to exchange ghost points Serial: for each point, compute average remember boundary conditions

26 Globus Security Single-sign-on, certificate handling, CAS, MyProxy Execution Management Remote jobs: GRAM and Condor-G Data Management GridFTP, reliable FT, 3rd party FT Information Services aggregating information from federated grid resources Common Runtime Components web services through GT4 The following is a personal opinion, it is NOT the position of the NVO: Globus is a complex and difficult installation Globus needs frequent maintenance and updates Globus is monolithic (all or nothing)

27 Data storage

28 Typical types of HPC storage needs TypeTypical size Use Aggregate BW Tolerance for Latency Requirements 11-10TBHome filesyste m A lot of small files, high metadata rates, interactive use. 2 (optional) 100s GB (per CPU) Local scratch space High bandwidth data cache. 310- 100TB Global filesyste m High aggregate bandwidth. Concurrent access to data. Moderate latency tolerated. 4100TB- PB Archival Storage Large storage pools with low cost. Used for long term storage of results.

29 Disk Farms (datawulf) Large files striped over disks Management node for file creation, access, ls, etc etc Homogeneous Disk Farm (= parallel file system) parallel file system metadata node parallel I/O

30 Parallel File System Large files are striped –very fast parallel access Medium files are distributed –Stripes do not all start the same place Small files choke the PFS manager –Either containerize –or use blobs in a database not a file system anymore: pool of 10 8 blobs with lnames

31 Storage Resource Broker (SRB) Single logical namespace while accessing distributed archival storage resources Effectively infinite storage Data replication Parallel Transfers Interfaces: command-line, API, SOAP, web/portal.

32 Storage Resource Broker (SRB): Virtual Resources, Replication NCSA SDSC workstation SRB Client (cmdline, or API) hpss-sdscsfs-tape-sdschpss-caltech …

33 Storage Resource Broker (SRB): Virtual Resources, Replication Browser SOAP client Command-line.... casjobs at JHU tape at sdsc myDisk Similar to VOSpace concept certificate File may be replicated File comes with metadata... may be customized

34 Containerizing Shared metadata Easier for bulk movement container file in container

35 Data intensive computing with NVO services

36 Two Key Ideas for Fault- Tolerance Transactions No partial completion -- either all or nothing –eg copy to a tmp filename, then mv to correct file name Idempotent Acting as if done only once, even if used multiple times Can run the script repeatedly until finished

37 DPOSS flattening 2650 x 1.1 Gbyte files Cropping borders Quadratic fit and subtract Virtual data SourceTarget

38 Driving the Queues for f in os.listdir(inputDirectory): # if the file exists, with the right size and age, then we keep it ofile = outputDirectory +"/"+ f if os.path.exists(ofile): osize = os.path.getsize(ofile) if osize != 1109404800: print " -- wrong target size, remaking", osize else: time_tgt = filetime(ofile) time_src = filetime(file) if time_tgt < time_src: print(" -- target too old or nonexistant, making") else: print " -- already have target file " continue cmd = "qsub -v \"FILE=" + f +"\"" print " -- submitting batch job: ", cmd os.system(cmd) Here is the driver that makes and submits jobs

39 PBS script #!/bin/sh #PBS -N dposs #PBS -V #PBS -l nodes=1 #PBS -l walltime=1:00:00 cd /home/roy/dposs-flat/flat./flat \ -infile /pvfs/mydata/source/${FILE}.fits \ -outfile /pvfs/mydata/target/${FILE}.fits \ -chop 0 0 1500 23552 \ -chop 0 0 23552 1500 \ -chop 0 22052 23552 23552 \ -chop 22052 0 23552 23552 \ -chop 18052 0 23552 4000 A PBS script. Can do "qsub –v "FILE=f345"

40 GET services from Python import urllib hyperatlasURL = self.hyperatlasServer + "/getChart?atlas=" + atlas \ + "&RA=" + str(center1) + "&Dec=" + str(center2) stream = urllib.urlopen(hyperatlasURL) # result is a tab-separated line, so use split() to tokenize tokens = stream.readline().split('\t') print "Using page ", tokens[0], " of atlas ", atlas self.scale = float(tokens[1]) self.CTYPE1 = tokens[2] self.CTYPE2 = tokens[3] rval1 = float(tokens[4]) rval2 = float(tokens[5]) This code uses a service to find the best hyperatlas page for a given sky location

41 VOTable parser in Python import urllib import xml.dom.minidom stream = urllib.urlopen(SIAP_URL) doc = xml.dom.minidom.parse(stream) #Make a dictionary for the columns col_ucd_dict = {} for XML_TABLE in doc.getElementsByTagName("TABLE"): for XML_FIELD in XML_TABLE.getElementsByTagName("FIELD"): col_ucd = XML_FIELD.getAttribute("ucd") col_ucd_dict[col_title] = col_counter urlColumn = col_ucd_dict["VOX:Image_AccessReference"] formatColumn = col_ucd_dict["VOX:Image_Format"] raColumn = col_ucd_dict["POS_EQ_RA_MAIN"] deColumn = col_ucd_dict["POS_EQ_DEC_MAIN"] From a SIAP URL, we get the XML, and extract the columns that have the image references, image format, and image RA/Dec

42 VOTable parser in Python import xml.dom.minidom table=[] for XML_TABLE in doc.getElementsByTagName("TABLE"): for XML_DATA in XML_TABLE.getElementsByTagName("DATA"): for XML_TABLEDATA in XML_DATA.getElementsByTagName("TABLEDATA"): for XML_TR in XML_TABLEDATA.getElementsByTagName("TR"): row=[] for XML_TD in XML_TR.getElementsByTagName("TD"): data = "" for child in XML_TD.childNodes: data += row.append(data) table.append(row) Table is a list of rows, and each row is a list of table cells

43 Science Gateways

44 Grid Impediments Learn Globus Learn MPI Learn PBS Port code to Itanium Get certificate Get logged in Wait 3 months for account Write proposal and now do some science....

45 A better way: Graduated Security for Science Gateways Web form - anonymous some science.... Register - logging and reporting more science.... Authenticate X.509 - browser or cmd line big-iron computing.... Write proposal - own account power user

46 2MASS Mosaicking portal An NVO-Teragrid project Caltech IPAC

47 Three Types of Science Gateways Web-based Portals –User interacts with community-deployed web interface. –Runs community-deployed codes –Service requests forwarded to grid resources Scripted service call –User writes code to submit and monitor jobs Grid-enabled applications –Application programs on users' machines (eg IRAF) –Also runs program on grid resource

48 Nesssi: Secure Web services for astronimy client certificate repository nesssi web portal nesssi node web form SOAP http queue fetch proxy select user account sandbox storage open http certificate policies

49 nesssiServer. dpossMosaic.mosaic ( -ra 49.1 -dec 60.1 -rawidth 0.5 -decwidth 0.5 -filt f -bgcorr 0) Mosaic service

50 ( -bandpass z1 -ra 170.08 -dec 13.275 -rawidth 1.0 -decwidth 1.0 ) Coadd service

51 Cutout Service, "-surveys PQ:gr,PQ:gi,PQ:z1,PQ:z2,SDSS:r,SDSS:i,SDSS:z,2MASS:k,2MASS:h -size 64)

52 cutouts from Palomar-Quest, SDSS, 2MASS of sources from Veron quasar catalog

53 Amazon Grid (who will pay?)

54 Amazon Grid Simple Storage Service Write, read, and delete. Each object has a unique, developer-assigned key. Authentication mechanisms. Objects can be private or public. Rights can be granted to specific users. REST and SOAP interfaces Default download protocol is HTTP. BitTorrent(TM) also available.

55 Amazon Grid Elastic Compute Cloud Create an Amazon Machine Image (AMI) containing your applications, libraries, data and associated configuration settings. Upload the AMI into Amazon Simple Storage Service. Configure security and network access. Start, terminate, and monitor as many instances of your AMI as needed. Pay for the instance hours and bandwidth that you actually consume. $0.10 per instance-hour consumed $0.20 per GB of data transferred outside of Amazon $0.15 per GB-Month of Amazon S3 storage

56 Amazon Grid Simple Queue Service Move data between distributed application components performing different tasks, without losing messages or requiring each component to be always available. Unlimited number of queues, unlimited number of messages. New messages can be added at any time. A computer can check a queue at any time for messages waiting to be read. REST, SOAP and query interfaces. The queue creator determines which other users can write to or read from the queue.

Download ppt "Using the Grid for Astronomy Roy Williams, Caltech."

Similar presentations

Ads by Google