The Visualization Center at Scripps Institution of Oceanography: Education and Outreach

Since opening in March 2002, the Visualization Center at Scripps has had more than 2,500 visitors, of which ∼500 were education- and outreach-related. Based upon follow-up requests and referrals, we expect these numbers to grow. The center's state-of-the-art visualization technology projects high-resolution, multidimensional images onto a 120° curved Panoram® floor-to-ceiling screen (8′6″ by 28′4″) that immerses viewers in a virtual environment (Figure 1). The center is ideal for presenting and manipulating very large data sets to groups of up to 50 people, and the system is equipped with transmitters and LCD shutter glasses that allow stereographic 3D viewing of high-resolution data sets through a set of specialized eyeglasses (Figure 2). The lenses in the glasses flicker synchronously with the computer images at 48 flames per second, per eye, thus producing a stereo or 3D effect. Figure 1. ▴ A group of visitors in the Visualization Center at Scripps view the topography of Mars. Multiple video streams can be simultaneously displayed, including the SGI® megadesktop, S-VHS video, DVD video, and video from a laptop computer; the user can quickly toggle between these various platforms (Kent et al., 2002). Similarly, the five-channel surround-sound audio system can be integrated through several inputs, allowing for numerous video and audio combinations. For instance, one third of the screen can display S-VHS video of damaging earthquakes, while the remaining portion of the screen can show an interactive underground 3D flight through seismicity in the regions presented in the video. Alternatively, the audio surround-sound system can be set to produce sounds of various synthetically generated earthquakes (http://quake.wr.usgs.gov/info/listen/allsounds.htmt), while the corresponding seismicity, topography, and seismic station locations and telemetry paths are juxtaposed on the screen with the associated seismic waves. Figure 2. ▴ Visitors to the Visualization Center at Scripps use specially designed 3D glasses to view high-resolution stereo images of the …

[1]  D. Agnew,et al.  The complete (3‐D) surface displacement field in the epicentral area of the 1999 MW7.1 Hector Mine Earthquake, California, from space geodetic observations , 2001 .

[2]  David T. Sandwell,et al.  Fault creep along the southern San Andreas from interferometric synthetic aperture radar, permanent scatterers, and stacking , 2003 .

[3]  Ruth A. Harris,et al.  Introduction to Special Section: Stress Triggers, Stress Shadows, and Implications for Seismic Hazard , 1998 .

[4]  Bernard Minster,et al.  Deformation on Nearby Faults Induced by the 1999 Hector Mine Earthquake , 2002, Science.

[5]  D. Sandwell,et al.  Driving Forces for Limited Tectonics on Venus , 1997 .

[6]  S. Moran,et al.  Seismic Response of the Katmai Volcanoes to the 6 December 1999 Magnitude 7.0 Karluk Lake Earthquake, Alaska , 2001 .

[7]  A. Rubin,et al.  Implications of diverse fault orientations imaged in relocated aftershocks of the Mount Lewis, ML 5.7, California, earthquake , 2002 .

[8]  Peter M. Shearer,et al.  A New Method for Determining First-Motion Focal Mechanisms , 2002 .

[9]  S. Wiemer,et al.  Change in the probability for earthquakes in Southern California due to the Landers magnitude 7.3 earthquake. , 2000, Science.

[10]  Gregory C. Beroza,et al.  Foreshock sequence of the 1992 Landers, California, earthquake and its implications for earthquake nucleation , 1995 .

[11]  Jian Lin,et al.  Delayed triggering of the 1999 Hector Mine earthquake by viscoelastic stress transfer , 2001, Nature.

[12]  D. Kilb A strong correlation between induced peak dynamic Coulomb stress change from the 1992 M7.3 Landers, California, earthquake and the hypocenter of the 1999 M7.1 Hector Mine, California, earthquake , 2003 .

[13]  G. Kent,et al.  An examination of along-axis variation of magma chamber width , 1998 .

[14]  Steven P. Miller,et al.  SIOExplorer: Digital Library Project , 2001, MTS/IEEE Oceans 2001. An Ocean Odyssey. Conference Proceedings (IEEE Cat. No.01CH37295).

[15]  J. Gomberg,et al.  The initial subevent of the 1994 Northridge, California, earthquake: Is earthquake size predictable? , 1999 .

[16]  F. Vernon,et al.  Small-scale stress heterogeneity in the Anza seismic gap, southern California , 1994 .

[17]  Yehuda Bock,et al.  Near real‐time radar interferometry of the Mw 7.1 Hector Mine Earthquake , 2000 .

[18]  P. Bodin,et al.  Triggering of earthquake aftershocks by dynamic stresses , 2000, Nature.

[19]  P. Barton,et al.  Evidence from three-dimensional seismic reflectivity images for enhanced melt supply beneath mid-ocean -ridge discontinuities , 2000, Nature.

[20]  David T. Sandwell,et al.  Small‐scale deformations associated with the 1992 Landers, California, earthquake mapped by synthetic aperture radar interferometry phase gradients , 1998 .

[21]  J. Bowen,et al.  Education and Outreach Based on Data from the Anza Seismic Network in Southern California , 2003 .

[22]  W. Ellsworth,et al.  Seismicity Remotely Triggered by the Magnitude 7.3 Landers, California, Earthquake , 1993, Science.

[23]  J. Haase,et al.  Constraints on temporal variations in velocity near Anza, California, from analysis of similar event pairs , 1995, Bulletin of the Seismological Society of America.

[24]  P. Shearer Parallel fault strands at 9‐km depth resolved on the Imperial Fault, Southern California , 2001 .