Stanford Synchrotron Radiation Project (SSRP)

X-ray science at SLAC began with the Stanford Synchrotron Radiation Project (SSRP). SLAC's SPEAR ring was built with one tangential port to allow synchrotron radiation to come out. Without the foresight of the ring designers to do this, SSRP would probably never have come into existence.

A successful pilot project at SPEAR led to the National Science Foundation funding the SSRP which began operations in May 1974, 8 months ahead of schedule. SSRP was the first synchrotron radiation laboratory on a multi-GeV electron storage ring that was set up as a national facility to provide access to a broad spectral range -- including hard x-rays -- to a large number of users. Although limited by parasitic operation on the SPEAR colliding-beam program, research done at SSRP revolutionized x-ray science, leading to the funding of dedicated multi-GeV facilities in the US and abroad, the so-called second generation light sources

At the start, five experimental stations shared radiation from one bending magnet tangential exit port that was part of the initial construction of the SPEAR colliding-beam storage ring. What is now the Stanford Synchrotron Radiation Lightsource (SSRL) has blossomed from a small adjunct to the SPEAR particle physics program into a vital part of SLAC National Accelerator Laboratory.

Selected Timeline

1968

Bill Spicer (Stanford University) memorandum of June 18, 1968, making a very early request that Pief Panofsky consider the possibility of using "cyclotron" (later called synchrotron) radiation from the planned SLAC storage ring for solid state studies

1972

Decision is made to start a pilot project to use the synchrotron radiation at SPEAR. In January, the Center for Materials Research (CMR) at Stanford provides funds to install an ultra-high vacuum valve on a tangential port. A beryllium window assembly and other front-end components are later added to this tangential port without venting the storage-ring vacuum system. The CMR also funds the design and cost estimate for a one-port three-station facility at SPEAR. A supplementary proposal is submitted to the National Science Foundation in November to cover the costs for the pilot project, which was focused on high-resolution X-ray photoemission spectroscopy. A proposal to build and operate the facility is submitted to the NSF by PI Sebastian Doniach. Another proposal for a synchrotron facility at the Cambridge Electron Accelerator (CEA)is submitted by William Paul, Karl Strauch, and Herman Winick at Harvard University. A review committee established by the NSF makes site visits to both SLAC and the CEA and decides in favor of the SLAC proposal.

1973

Stanford Synchrotron Radiation Project (SSRP) started by Sebastian Doniach (Director) and William Spicer (Consulting Director) with funding from the National Science Foundation; the US Navy’s Michelson Lab at China Lake, California; Xerox Corporation; and Bell Telephone Laboratory. Herman Winick from the CEA joins SSRP as Associate Director.

5/1974

SSRP begins operations (8 months ahead of schedule) with 5 experimental stations sharing a beamline.

10/24-25/1974

First SSRP Users Group meeting

11/1974

The November Revolution takes center stage: On November 8th the first sharp resonance is discovered at SPEAR, beam energy required is 1.5 GeV, no x-ray experiments are possible at this beam energy, UV experiments continue. On November 11th, SSRP is given a prime shift, "experimenters [are] very happy." On November 20th a second sharp resonance is observed, beam energy required is 1.85 GeV, better for SSRP than November 8th, but still not much x-ray flux.

1975

National Science Foundation funds a second main beam line and a general expansion of laboratory facilities at SSRP.

Brian Kinkaid, who played a major role in the development of the SSRP EXAFS facility, completes his Ph.D., the first to be awarded for work done at SSRP.

1976

Cullie Sparks of the Oak Ridge National Laboratory led the team that did the search for superheavy elements at SSRP in 1976. The synchrotron radiation experiments definitively showed that the claims for the presence of superheavy elements in some minerals were inaccurate.

5/1976

A second beam line with 4 additional synchrotron radiation experimental stations begins operating at SPEAR

12/1976

SSRP user community numbers almost 200 scientists from 52 different institutions, with 138 active research proposals. NSF approves SSRP expansion proposal, including new experimental hall, new beam lines, and a wiggler magnet.

4/1977

SSRP Wiggler Workshop: A three-day workshop on the subject of Wiggler magnets is held at SLAC on March 21-23, 1977, and is attended by about 60 scientists from 17 laboratories around the world.

9/1/1977

SSRP becomes Stanford Synchrotron Radiation Laboratory (SSRL)

1973-1977

SSRP Photo Gallery

SSRP construction
Photograph taken on September 20, 1973 showing the SPEAR ring, Pilot Project alcove and outdoor hutch which housed the Ultra-High Vacuum (UHV) photoemission chamber. Data collection continued as the construction of the first Stanford Synchrotron Radiation Project (SSRP) building proceeded with the experimenters negotiating around the concrete forms and relying on plastic sheets to protect the hutch and the UHV chamber from rain.  (SLAC)
SSRP drawing, April 1974
April 1974 drawing of plans for the first Stanford Synchrotron Radiation Project (SSRP) beam lines, showing how 11.5 mrad of horizontal divergence from a SPEAR bending magnet was shared by five simultaneously operational experimental stations, each with a monochromator. Inset drawing at upper right shows the project's placement on SPEAR. (SLAC - Zawojski)
SSRP Sears garden shed
An early SSRP Experimental Station used a Sears "Garden Shed" mounted on the concrete roof of SPEAR. Ian Munro (third from right, wearing a tie), a visitor for one year from Daresbury, was the key scientist in the development of this station. He provided haggis and drinks to celebrate the first light. On Munro's right are Ben Salzburg, Axel Golde, Sebastian Doniach (first Director of SSRP) and George Brown.  (SLAC)
Doniach, Bienenstock, Winick 1977
Seb Doniach (left), SSRP's Director, Associate Director Art Bienenstock, and Deputy Director Herman Winick in discussion outside Building 120, SSRP, January 1977. (SLAC - Faust)
SSRP staff meeting 1977
SSRP Weekly staff meeting including Herman Winick, Arthur Bienenstock, Ron Gould, and Seb Doniach; January 1977.  (SLAC - Faust)
Spicer and Lindau, 1977
William Spicer and Ingolf Lindau outside Building 120, January 1977.  (SLAC - Faust)
Pianetta, Hunter, Brown, Businger, Jako
Piero Pianetta, Sally Hunter, George Brown, Ursalla Businger, and Chris Jako outside SSRP, 20 April 1977.  (SLAC)
USNWC-China Lake group
Jim Stanford, Vern Jones, and Victor Rehn (left to right) of the US Naval Weapons Center-China Lake with mirror for the eight degree experimental station on the first SSRP beam line. At the time, this mirror was the smoothest piece of copper in the world.  (SLAC)
Sally Hunter
Sally Hunter, a Stanford graduate student working with Professor Artie Bienenstock, loads a sample for EXAFS measurements on Beam Line 1-5. The blue box was the original "hutch" at SSRL and was constructed so as to be radiation safe when the beam was on, but simple and quick to access when the beam was off. As the complexity of the experiments has grown over time, so has the size of the hutches.  (SLAC)
Working on beamline 1-4
Working on SSRL beam line 1-4 (left to right), postdoctoral fellow Marguerite Yevitz, Professor Keith Hodgson, postdoctoral fellow Alex Wlodawer and graduate student James Phillips did a series of experiments that demonstrated the significant value of synchrotron radiation for protein crystallography measurements. The group, including postdoctoral fellow Julia Goodfellow, and Drs. Paul Phizackerley and Ethan Merrit, also exploited the variable wavelength nature of synchrotron radiation.   (SLAC)

The First Beamlines

  Experimental Station Early Users / Investigators Design/Construction Operational
1-1 4° Beam Line - UV
and soft X-radiation <2keV
F. Brown, R. Bachrach, S. Hagstrom (Xerox);
I. Lindau, W. Spicer (Stanford University);
D. Shirley (LBL)
F. Brown et al. (Xerox Research Center).
Soft X-ray Grazing Incidence Monochromator
[Grasshopper] design by N. Lien
(University of Wisconsin),
funded by Xerox Research Center.
Grazing-incidence Mirror by U.S. Navy Michelson Lab
May-June 1974
1-2 8° Rising Beam Line
- UV [VUV] radiation <.3keV
V. Rehn et al. (U.S. Navy Michelson Lab, China Lake);
I. Lindau, W. Spicer (Stanford)
V. Rehn et al. (U.S. Navy Michelson Lab).
McPherson Normal Incidence Monochromator
and Grazing-incidence Mirror contracted by
U.S. Navy Michelson Lab
June 1974
1-3 X-ray Photoemission Spectroscopy (XPS) I. Lindau, S.Doniach, W.Spicer,
P.Pianetta* (Stanford); P. Citrin (Bell Lab)
I. Lindau (Stanford), Double crystal Monochromator
design by P. Pianetta*
High vacuum sample chamber and energy analyzer
by I. Lindau
May 1974
(Also used during
1973-74
Pilot Project)
1-4 X-ray diffraction (Biology Beam Line)
- Low angle diffraction camera
N.Webb et al. (California Institute of Technology);
I. Matsubara (University of Tokyo);
K. Hodgson (Stanford)
N.Webb et al. (California Institute of Technology)
funded and built Grazing-incidence monochromator
(curved crystal, double-focusing)
with low angle diffraction camera
June 1974
1-5 Extended X-ray
Absorption-edge
Fine Structure
(EXAFS)
P. Eisenberger (Bell Lab);
S. Doniach, B. Kincaid,* M. Weissbluth,
A. Bienenstock, S. Hunter* (Stanford); F. Lytle (Boeing),
D. Sayers, E. Stern (University of Washington)
P. Eisenberger (Bell Lab),
D. Sayers (University of Washington)
Rapidly Tunable Hard X-ray Monochromator
(channel-cut silicon crystal)
funded by Bell Lab and Seattle Group
(Boeing and University of Washington)
May 1974

*Graduate students

Sources (in chronological order)

Contemporary

Later histories and personal narratives

The Archives also holds: a video of Herman Winick giving an illustrated talk about the history of SSRP/SSRL, including time-lapse footage of the set up of Cullie Sparks' experiment; snapshots of folks at work; and further information about the X-ray science conducted here.

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