XLDB CONFERENCE WELCOME. James Williams September 11, 2012

Similar documents
Office of Science Perspective

SLAC National Accelerator Laboratory. Persis S. Drell Director August 30, 2010

Katsushi Arisaka University of California, Los Angeles Department of Physics and Astronomy

Astronomy of the Next Decade: From Photons to Petabytes. R. Chris Smith AURA Observatory in Chile CTIO/Gemini/SOAR/LSST

Welcome to DESY. What is DESY and what kind of research is done here?

The SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry Breaking Gell-Mann Okubo Mass Formulae Quark-Mo

A few words by Arie Bodek - University of Rochester

Basic Energy Sciences Update and Current Status of Facilities

Most of Modern Physics today is concerned with the extremes of matter:

Direct-Current Accelerator

Jefferson Lab Status. Stuart Henderson Laboratory Director. April 26, 2018

Laboratory for Nuclear Science

Most of Modern Physics today is concerned with the extremes of matter:

6-8 February 2017 Hotel do Mar Sesimbra. Hands on Neutrinos

Elementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016

An end-to-end simulation framework for the Large Synoptic Survey Telescope Andrew Connolly University of Washington

Neutrino Physics: an Introduction

Evidence for the Strong Interaction

The Large Synoptic Survey Telescope

An Introduction to Particle Physics

High Energy Physics. QuarkNet summer workshop June 24-28, 2013

Particle Physics A short History

Honorary Doctorate Ceremony for Jonathan Dorfan, 6 July 2009

EIC Science. Rik Yoshida, EIC-Center at Jefferson Lab Abhay Deshpande, Center for Frontiers in Nuclear Physics, BNL and Stony Brook

A Brief History of Particle Physics

Par$cles. Ma#er is made of atoms. Atoms are made of leptons and quarks. Leptons. Quarks. atom nucleus nucleon quark m m m m

Rick Ebert & Joseph Mazzarella For the NED Team. Big Data Task Force NASA, Ames Research Center 2016 September 28-30

Professor Emmanuel Tsesmelis CERN Directorate Office Department of Physics, University of Oxford

Introduction to Particle Accelerators & CESR-C

From Supercomputers to GPUs

Lecture 25: Cosmology: The end of the Universe, Dark Matter, and Dark Energy. Astronomy 111 Wednesday November 29, 2017

W-Bosons as a Microscope for the Observation of Quarks and Anti-Quarks Inside the Proton M. Grosse Perdekamp University of Illinois, Urbana Champaign

IoP Masterclass. The Physics of Flavour at the Large Hadron Collider. Tim Gershon University of Warwick March 30th 2011

The Discovery of the Higgs Boson: one step closer to understanding the beginning of the Universe

Charmed Mesons GEORGE HODGKINSON AND BETHANY SLINGSBY

Introduction to Particle Accelerators

Finish up our overview of small and large

v = H o d Hubble s Law: Distant galaxies move away fastest Velocity (v) is proportional to Distance (d):

Director s s Report. Jonathan Dorfan DOE High Energy Physics Review June 14, 2005

The Effects of Nuclear Weapons

Y2 Neutrino Physics (spring term 2017)

QCD and deep inelastic scattering

LSST, Euclid, and WFIRST

Neutrino Physics. Kam-Biu Luk. Tsinghua University and University of California, Berkeley and Lawrence Berkeley National Laboratory

the quest for certainty

M. Cobal, PIF 2006/7. Quarks

IoP Masterclass. The Physics of Flavour at the Large Hadron Collider. Tim Gershon University of Warwick April

M. Cobal, PIF 2006/7. Quarks

Engines of Discovery

Particle Accelerators for Research and for Medicine

Particle Accelerators for Research and for Medicine

W-Bosons as a Microscope for the Observation of Quarks and Anti-Quarks Inside the Proton M. Grosse Perdekamp University of Illinois, Urbana Champaign

Island Universes. Up to 1920 s, many thought that Milky Way encompassed entire universe.

Quarks and Their Discovery

A Brief History of Modern Physics

Quarks and the Cosmos

I. Antoniadis CERN. IAS CERN Novice Workshop, NTU, 7 Feb 2014

Accelerators. Acceleration mechanism always electromagnetic Start with what s available: e - or p Significant differences between accelerators of

Introduction to me, High-Energy Physics and research at Belle

A brief history of neutrino. From neutrinos to cosmic sources, DK&ER

Section 4 : Accelerators

IoP Masterclass B PHYSICS. Tim Gershon University of Warwick March 18 th 2009

Neutrino vs antineutrino. Lepton number

Scientific Data Flood. Large Science Project. Pipeline

REALIZING EINSTEIN S DREAM. Exploring Our Mysterious Universe

Applications of scattering theory! From the structure of the proton! to protein structure!

Status of Managing Chemical Inventories Utilizing Radio Frequency Identification at Department of Energy Facilities

The first 400,000 years

Discovery of c, b and t quarks and quarkonia Marco Schramm

Lecture 6-4 momentum transfer and the kinematics of two body scattering

RESOLUTION DISTANCE DISTANCE

An Assessment of U.S.-Based Electron-Ion Collider Science

Data Intensive Computing meets High Performance Computing

The Large Hadron Collider, and New Avenues in Elementary Particle Physics. Gerard t Hooft, Public Lecture, IPMU Tokyo, April 16, 2015

Cosmic Background Radiation

Teaching Assistant Shared responsibility for labs, discussion sections, exams, homework assignments, and grades for an introductory physics class.

Inside the Atom. Say Thanks to the Authors Click (No sign in required)

Introduction. Read: Ch 1 of M&S

INTERACTIONS. The science of matter, space and time. High-Energy Physics

Leptons and Weak interactions

Higgs particle discovery and measurements - a breakthrough in physics

Summer Students 2003

Introduction to Synchrotron Light Sources

F. TASNÁDI LINKÖPING UNIVERSITY THEORETICAL PHYSICS NEUTRINO OSCILLATIONS & MASS

Particle physics today. Giulia Zanderighi (CERN & University of Oxford)

Prof. Emmanuel Tsesmelis Deputy Head of International Relations CERN

Astronomy 113. Dr. Joseph E. Pesce, Ph.D. The Big Bang & Matter. Olber s Paradox. Cosmology. Olber s Paradox. Assumptions 4/20/18

Astronomy 113. Dr. Joseph E. Pesce, Ph.D Joseph E. Pesce, Ph.D.

Ryan Stillwell Paper: /10/2014. Neutrino Astronomy. A hidden universe. Prepared by: Ryan Stillwell. Tutor: Patrick Bowman

(AD/BP-OP-BD/BPS) ESS

The Science Missions of Columbia

Elementary (?) Particles

Introduction a la Physique des Saveur Lourdes. JRJC 2013 Yasmine Amhis LAL - Orsay

Chapter Outline. The Ultimate Structure of Matter. The Library. Of What is the Universe Made? Reductionism. The Building Blocks of Matter

Jim s early days: Brookhaven, Princeton, and the CP Discovery. September 30, 2016 Stewart Smithx

Big Bang Planck Era. This theory: cosmological model of the universe that is best supported by several aspects of scientific evidence and observation

Particle Physics and Astrophysics Program at SLAC. David B. MacFarlane Associate Laboratory Directory for PPA SLUO AGM on Nov 10, 2011

The Big Bang Theory. Rachel Fludd and Matthijs Hoekstra

The Ultimate Structure of Matter

Sample file. Solar System. Author: Tina Griep. Understanding Science Series

Transcription:

XLDB CONFERENCE WELCOME James Williams September 11, 2012

2

Welcome! LINAC: Linear Accelerator It has driven SLAC science for 50 years 3

Department of Energy Office of Science National Laboratories Pacific Northwest Lawrence Berkeley National SLAC National Accelerator Idaho National Lawrence Livermore National Sandia National Laboratories National Renewable Energy Fermi National Accelerator Ames National Los Alamos National Argonne National National Energy Technology Brookhaven National Princeton Plasma Physics Thomas Jefferson National Accelerator Facility Oak Ridge National Savannah River National National Nuclear Security Administration Lab Office of Energy Efficiency and Renewable Energy Lab Office of Environmental Management Lab Office of Fossil Energy Lab Office of Nuclear Energy, Science and Technology Lab Office of Science Lab 4

Stanford University DOE pays Stanford $1 per year to lease 426 acres of land 240 Universities worldwide use our resources 5

1,600 Employees from 36 Countries -205 Postdocs and Grad Students ; 3,100 Facility Users & Visiting Scientists 142 Buildings 1,000 Scientific Papers published each year in peer-reviewed journals 6 Scientists awarded the Nobel Prize for work done at SLAC 1 st North American Website $400,000,000 Budget (10% of this goes for energy consumption) Jan 26, 2012 6

Hold Slide for Nobels Nobel Prizes Physics, 1976 Pioneering experimental contributions to lepton physics. Burton Richter Samuel C.C. Ting Richard E. Taylor Jerome I. Friedman Henry W. Kendall Physics, 1990 Deep inelastic scattering of electrons on protons and bound neutrons Essential for the development of the quark model Physics, 1995 Discovery of the tau lepton Chemistry, 2006 Studies of the molecular basis of eukaryotic transcription Martin L. Perl Frederick Reines Roger Kornberg Yoichiro Nambu, Makoto Kobayashi, Toshihide Maskawa Physics, 2008 Theory of broken symmetries later observed by BaBar Ada Yonath Chemistry, 2009 Studies of the structure and function of the ribosome, foundation studies at SSRL 7

Our Mission Today Our programs explore the ultimate structure and dynamics of matter and the properties of energy, space and time - at the smallest and largest scales, in the fastest processes and at the highest energies - through robust scientific programs, excellent accelerator based user facilities and valuable partnerships. Build and operate world leading Photon Science Facilities-LCLS (LINAC Coherent Light Source) and SSRL (Stanford Synchrotron Radiation Lightsource) Perform world leading science at these facilities Maintain our position as the premier accelerator laboratory Strategic programs in particle physics, particle astrophysics and cosmology 8

What happened from actualizing this mission Production: 1999-2008 ~5 PB raw data 1 PB database (in 2002) http://www-public.slac.stanford.edu/babar/ BABAR is a particle physics experiment designed to study some of the most fundamental questions about the universe by exploring its basic constituents - elementary particles.

What will happen from actualizing this mission Operations: 2022-2031 50+ PB images 45 PB database Image metadata consisting of 700 million rows An object catalog with 20 billion rows each with 200+ attributes 30+ trillion object detections Alert count: 2 million / night 3.2 gigapixel image every 15 sec Complex n-point correlations, including near neighbor searches at petascale http://lsst.org/lsst/about/technology The LSST is a new kind of telescope. With a light-gathering power among the largest in the world, it can detect faint objects with short exposures.

Goals for the XLDB Conference

Exchange Information Identify trends, commonalities and major roadblocks related to building extremely large data stores

Bridges Bridge the gap between users trying to build extremely large data stores and solution providers worldwide

Development & Growth Facilitate development and growth of practical technologies for extremely large data stores

PRACTICAL SOLUTIONS: Our Recipe for XLDB Events Ingredients Big science Data-intensive industries Vendors Academia Directions 1. Mix together 2. Repeat yearly