[cig-commits] r12030 - seismo/3D/automeasure/latex

[alessia at geodynamics.org]

Author: alessia
Date: 2008-05-26 23:16:17 -0700 (Mon, 26 May 2008)
New Revision: 12030

Modified:
   seismo/3D/automeasure/latex/acknowledgements.tex
   seismo/3D/automeasure/latex/discussion.tex
   seismo/3D/automeasure/latex/flexwin_paper.pdf
   seismo/3D/automeasure/latex/method.tex
Log:
Added reference to CIG

Modified: seismo/3D/automeasure/latex/acknowledgements.tex
===================================================================
--- seismo/3D/automeasure/latex/acknowledgements.tex	2008-05-25 12:19:13 UTC (rev 12029)
+++ seismo/3D/automeasure/latex/acknowledgements.tex	2008-05-27 06:16:17 UTC (rev 12030)
@@ -5,9 +5,6 @@
 National Science Foundation under grant EAR-0711177.
 The numerical simulations for this research were performed
 on the GPS Dell cluster.
-The facilities of the IRIS Data Management System, and specifi- 
-cally the IRIS Data Management Center, were used for access to 
+The facilities of the IRIS Data Management System, and specifically the IRIS Data Management Center, were used for access to 
 waveform and metadata required in global scale examples of this study. The IRIS DMS is funded through the National Science Foundation and specifically 
-the GEO Directorate through the Instrumentation and Facilities Pro- 
-gram of the National Science Foundation under Cooperative Agree- 
-ment EAR-0004370.  Additional global scale data was provided by the GEOSCOPE network.
+the GEO Directorate through the Instrumentation and Facilities Program of the National Science Foundation under Cooperative Agreement EAR-0004370.  Additional global scale data was provided by the GEOSCOPE network.

Modified: seismo/3D/automeasure/latex/discussion.tex
===================================================================
--- seismo/3D/automeasure/latex/discussion.tex	2008-05-25 12:19:13 UTC (rev 12029)
+++ seismo/3D/automeasure/latex/discussion.tex	2008-05-27 06:16:17 UTC (rev 12030)
@@ -25,4 +25,5 @@
 %Finally, we envision that successive iterations of a particular tomographic model may require minor adjustments to the tuning parameters, as the fits improve between the synthetic and observed seismograms, permitting higher frequency information to be used.
 
 The desire to study regions of detailed structure and to examine the effects of finite source processes requires seismologists to deal with increasingly complex seismic records.  Furthermore, with increasing coverage and sampling rate, the available data becomes voluminous and challenging to manage. In using the FLEXWIN package, the onus would still be on the seismologist to tune the algorithm parameters so as to pick time windows appropriate for each specific study target. For a given data-set and a given set of tuning parameters, the time-window picking is entirely reproducible.  The automated and signal processing nature of the procedure should eliminate some of the human bias involved in picking measurement windows, while expediting the process of analyzing tens to hundreds of thousands of records.
-
+FLEXWIN is available as an open-source package through CIG (Computational
+Infrastructure for Geodynamics, {\tt http://www.geodynamics.org}).

Modified: seismo/3D/automeasure/latex/flexwin_paper.pdf
===================================================================
(Binary files differ)

Modified: seismo/3D/automeasure/latex/method.tex
===================================================================
--- seismo/3D/automeasure/latex/method.tex	2008-05-25 12:19:13 UTC (rev 12029)
+++ seismo/3D/automeasure/latex/method.tex	2008-05-27 06:16:17 UTC (rev 12030)
@@ -1,6 +1,6 @@
 \section{The selection algorithm\label{sec:algorithm}} 
 
-Our algorithm, called FLEXWIN to reflect its FLEXibility in picking time WINdows for measurement,  operates on pairs of
+Our open-source algorithm, called FLEXWIN to reflect its FLEXibility in picking time WINdows for measurement,  operates on pairs of
 observed and synthetic single component seismograms.  There is no restriction
 on the type of simulation used to generate the synthetics, though realistic
 Earth models and more complete propagation theories yield waveforms that are more similar to the observed