Position tomography and seismic inversion

28 mins 46 secs,  106.69 MB,  iPod Video  480x270,  29.97 fps,  44100 Hz,  506.39 kbits/sec
Share this media item:
Embed this media item:


About this item
Image inherited from collection
Description: Symes, W (Rice University)
Friday 16 December 2011, 16:30-17:00
 
Created: 2011-12-19 13:11
Collection: Inverse Problems
Publisher: Isaac Newton Institute
Copyright: Symes, W
Language: eng (English)
 
Abstract: Active source seismic data may depend on more parameters than the spatial dimension of the earth model, and thus must satisfy some internal consistency conditions. Membership in the kernel of an annihilation operator provides one useful way to express these conditions. For linearized data simulation with smooth reference model, annihilators may belong to well-studied classes of oscillatory integral operators, which have rich geometric structure. I will describe generally how annihilators arise and lead to inversion algorithms, and specifically how space-shift annihilators and associated position tomography problems may be used to determine the reference model in the linearized description of reflected waveform inversion.
Available Formats
Format Quality Bitrate Size
MPEG-4 Video 640x360    1.84 Mbits/sec 399.09 MB View Download
WebM 640x360    1.59 Mbits/sec 342.44 MB View Download
Flash Video 484x272    568.88 kbits/sec 119.86 MB View Download
iPod Video * 480x270    506.39 kbits/sec 106.69 MB View Download
MP3 44100 Hz 125.05 kbits/sec 26.15 MB Listen Download
Auto (Allows browser to choose a format it supports)