Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

POWER SPECTRUM CALCULATION FOR THE CORNELL WIGGLER A SASE EXPERIMENT AT BNL

Conference ·
OSTI ID:758973
 [1]
  1. BROOKHAVEN NATIONAL LABORATORY

Recently the authors showed [I] that the widely used simulation code TDA3D, even though a single frequency code, can be used to determine the power spectrum in the SASE process with excellent approximation in the exponential growth regime. In this paper, they apply this method to the BNL Cornell Wiggler A SASE experiment as an example. When the gain is not very high, there are many modes in the radiation, which seems to make the analytical calculation very difficult. However, they show that the increment of the radiation due to SASE over the spontaneous radiation can be expanded in terms of guided modes with rapid convergence. Thus when the spontaneous radiation is subtracted from the SASE power during the calculation, there is a good agreement between the analytical theory and the numerical simulation.

Research Organization:
Brookhaven National Lab., Upton, NY (US)
Sponsoring Organization:
USDOE Office of Energy Research (ER) (US)
DOE Contract Number:
AC02-98CH10886
OSTI ID:
758973
Report Number(s):
BNL--65854; KC0204011; KC0204011
Country of Publication:
United States
Language:
English

Similar Records

Power spectrum calculation for the Cornell Wiggler A SASE experiment at BNL
Technical Report · Sat Aug 01 00:00:00 EDT 1998 · OSTI ID:674828

Calculation of the output power in self-amplified spontaneous radiation using scaling of power with number of simulation particles
Journal Article · Thu Oct 01 00:00:00 EDT 1998 · Physical Review. E, Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics · OSTI ID:662229

The APS SASE FEL : modeling and code comparison.
Conference · Tue Apr 20 00:00:00 EDT 1999 · OSTI ID:11130