HPSS Performance study

Under:

Introduction

HPSS is software that manages petabytes of data on disk and robotic tape libraries. We will discuss in this section our observations as per the efficiency of accessing files in STAR as per a snapshot of the 2006 situation. It is clear that IO opptimizations has several components amongst which:
  • Access pattern optimization (request ordering, ...)
  • Optimization based on tape drive and technology capabilities
  • Miscellaneous technology considerations
    (cards, interface, firmware and driver, RAID, disks, ...)
  • HPSS disk cache optimizations
  • COS and/or PVR optimization
However, several trend have already been the object of past research and we will point to some of those and compare to our situation rather than debating the obvious. Wewill try to keep a focus on measurements in our environment.

Tape drive and technology capabilities

A starting point would be to discuss the capabilities of the technologies involved and their maximum performance and limitations. In STAR, two technologies remain as per 1006/10:
  • the 994B drives
  • the LTO-3 drives

Access pattern optimization (request ordering, ...)

A first simple and immediate consideration is to minimize tape mount and dismount operations, causing latencies and therefore performance drops. Since we use the DataCarousel for most restore operations, let's summarize its features.

Phi meson spin alignment wrt production plane / Global polarization of Lambda hyperons

Spin Alignment of vector mesons (K*, phi) in Au+Au collisions

TEA BREAK

3-particle correlations

3-particle correlations : Is there a Mach cone ?

Low- and intermediate-pT azimuthal di-hadron correlations

Phi analysis in CuCu collisions

Speaker : Xinghua and Bedanga


Talk time : 18:00, Duration : 00:30

Recent multiplicity results from PMD

K* analysis in Au+Au collisions

TEA BREAK

Properties of particle production at large transverse momentum in Au+Au and Cu+Cu collisions at RHIC

Yields and elliptic flow of d(dbar) and He3 (He3bar) in Au+Au collisions at sqrt_s = 200 GeV

A measurement of the centrality dependence of the N(Omega)/N(Phi ratios and Phi anisotropic flow

AOB

Speaker : All ( All )


Talk time : 15:00, Duration : 00:10

IRMIS progress

Speaker : Jiro Fujita ( Creighton )


Talk time : 14:50, Duration : 00:10

SDAS enclave reminder (for this year)

Speaker : Jerome Lauret ( BNL )


Talk time : 14:30, Duration : 00:10

Opened discussion - BNL domain and SMS / operational needs & requirements

Speaker : All ( All )


Talk time : 14:40, Duration : 00:10