Basic IMAGE version of Foils prepared 4 April 1996

Foil 7 Expected Signal versus Noise in Gravitational Wave Detectors

From Collection of GIF Images for General NPAC Projects April96- General NPAC ScreenDumps -- April 1996 on . by Geoffrey C. Fox
Comparison between rms noise h/rms in LIGO's first and advanced detector systems and the characteristic amplitude h/c of gravitational wave bursts from several hypothesized sources
  • NS is a Neutron Star
  • BH is a Black Hole
Science 256,281-412, 17 April 92
1 1
2 2
3 3
4 4
5 5
6 6
7 7
8 8
9 9
10 10
to:

© Northeast Parallel Architectures Center, Syracuse University, npac@npac.syr.edu

If you have any comments about this server, send e-mail to webmaster@npac.syr.edu.

Page produced by wwwfoil on Sat Feb 7 1998