Roles and Responsibilities for Team Leaders and Co-team leaders The definition of the initial science program for LCLS has been developed through an open process. Letters of intent were solicited from the breadth of the scientific community. These proposals for full instruments, technologies and science were evaluated by the LCLS Science Advisory Committee. The SAC saw all of high quality and felt that the science could be categorized into five thrust areas: pump-probe studies, coherent imaging, high energy density science, nano-scale dynamics, and atomic, molecular and optical science. They further suggested that team leaders be named for each thrust area and that they are the official pint of contact for each thrust area. SAC further suggested the addition of co-team leaders to supplement the expertise of the team leaders to ensure that the breadth of the science in the five thrust areas was well represented. Responsibilities of the team leader:

1) Definition and choices of the initial science program in their thrust areas. 2) Define the ‘physics requirements’ for the thrusts. This definition results in a

physics requirements document that is the control document that defines the performance metrics for the instrument. It should be noted that these requirements will quite naturally be developed collaboratively with the LUSI instrument scientists.

3) The team leader acts as the official point of contact between the team and the LUSI project.

Co-team leaders assist the team leader in carrying out these responsibilities.

LCLS – the Initial Scientific Teams and Thrusts

• AMO science Lou Dimauro Nora Berrah

• Coherent scattering of Brian Stephenson Karl Ludwignanoscale fluctuationsGerhard Grübel

• Diffraction studies of Kelly GaffneyDavid Reisstimulated dynamicsJörgen Larsson

(pump-probe) T. Tschentscher

Anders Nilsson• Nano-particle and single Janos Hajdu

Henry Chapmanmolecule (non-periodic) John Miaoimaging Jan Lüning

• High energy Dick Lee Phil Heimanndensity science

t=0

t=

Aluminum plasma

10-4 10-2 1102 10 4

classical plasma

dense plasma

high density matter

G =1

Density (g/cm-3)

G =10

G =100

team leader co-team leader(s)

LUSI and LCLS Science

LCLS – the Initial Scientific Teams and Thrusts

• AMO science Lou Dimauro Nora Berrah

• Coherent scattering of Brian Stephenson Karl Ludwignanoscale fluctuationsGerhard Grübel

• Diffraction studies of Kelly GaffneyDavid Reisstimulated dynamicsJörgen Larsson

(pump-probe) T. Tschentscher

Anders Nilsson• Nano-particle and single Janos Hajdu

Henry Chapmanmolecule (non-periodic) John Miaoimaging Jan Lüning

• High energy Dick Lee Phil Heimanndensity science

t=0

t=

Aluminum plasma

10-4 10-2 1102 10 4

classical plasma

dense plasma

high density matter

G =1

Density (g/cm-3)

G =10

G =100

team leader co-team leader(s)

LUSI and LCLS Science