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Full Discussion: Sort references
Top Forums UNIX for Dummies Questions & Answers Sort references Post 302903502 by kristinu on Wednesday 28th of May 2014 05:45:02 AM
Old 05-28-2014
Sort references

I have the following entries and want to perform a sort.
Each entry is separated by a newline, however each line should not be considired seperate. Maybe an awk program or similar, or a small script.

Code:
Anderson, E.R., Duvall, T.L., Jr., and Jefferies, S.M., 1990. Modelling 
     of Solar Oscilation Power Spectra. The Astrophysical Journal, vol. 364, 
     p. 699.

Duvall, T.L., Jr., and Harvey, J.W., 1986. Solar Doppler Shifts: Sources 
     of Continuous Spectra. In Seismology of the Sun and the Distant Stars, 
     (ed. D. Gough), NATO A Ser., Reidel, Dordrecht, p. 105.

Basu, S., Antia, H.M., and Tripathy, S.C. 1999. Ring Diagram Analysis
     of Near-Surface Flow in the Sun. The Astrophysical Journal, vol. 512, 
     pp. 458-470.

Nigam, R., Kosovichev, A.G., Scherrer, P.H., and Schou, J., 1998. 
     Asymmetry in Velocity and Intensity Helioseismic Spectra: A solution 
     to a long-standing puzzle. The Astrophysical Journal, vol. 495, 
     pp. L115-L118.

The sort should yield

Code:
Anderson, E.R., Duvall, T.L., Jr., and Jefferies, S.M., 1990. Modelling 
     of Solar Oscilation Power Spectra. The Astrophysical Journal, vol. 364, 
     p. 699.

Basu, S., Antia, H.M., and Tripathy, S.C. 1999. Ring Diagram Analysis
     of Near-Surface Flow in the Sun. The Astrophysical Journal, vol. 512, 
     pp. 458-470.

Duvall, T.L., Jr., and Harvey, J.W., 1986. Solar Doppler Shifts: Sources 
     of Continuous Spectra. In Seismology of the Sun and the Distant Stars, 
     (ed. D. Gough), NATO A Ser., Reidel, Dordrecht, p. 105.

Nigam, R., Kosovichev, A.G., Scherrer, P.H., and Schou, J., 1998. 
     Asymmetry in Velocity and Intensity Helioseismic Spectra: A solution 
     to a long-standing puzzle. The Astrophysical Journal, vol. 495, 
     pp. L115-L118.

 

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mlib_VolumeRayCast_General(3MLIB)			    mediaLib Library Functions				 mlib_VolumeRayCast_General(3MLIB)

NAME
mlib_VolumeRayCast_General, mlib_VolumeRayCast_General_Parallel_Nearest_U8_Bit, mlib_VolumeRayCast_General_Parallel_Nearest_U8_U8, mlib_VolumeRayCast_General_Parallel_Nearest_S16_S16, mlib_VolumeRayCast_General_Parallel_Trilinear_U8_U8, mlib_VolumeRayCast_General_Paral- lel_Trilinear_S16_S16, mlib_VolumeRayCast_General_Divergent_Nearest_U8_Bit, mlib_VolumeRayCast_General_Divergent_Nearest_U8_U8, mlib_Vol- umeRayCast_General_Divergent_Nearest_S16_S16, mlib_VolumeRayCast_General_Divergent_Trilinear_U8_U8, mlib_VolumeRayCast_General_Diver- gent_Trilinear_S16_S16 - cast a ray (or rays) through a 3D data set SYNOPSIS
cc [ flag... ] file... -lmlib [ library... ] #include <mlib.h> mlib_status mlib_VolumeRayCast_General_Parallel_Nearest_U8_Bit( mlib_rays *rays, const mlib_genvolume *vol, void *buffer); mlib_status mlib_VolumeRayCast_General_Parallel_Nearest_U8_U8( mlib_rays *rays, const mlib_genvolume *vol, void *buffer); mlib_status mlib_VolumeRayCast_General_Parallel_Nearest_S16_S16( mlib_rays *rays, const mlib_genvolume *vol, void *buffer); mlib_status mlib_VolumeRayCast_General_Parallel_Trilinear_U8_U8( mlib_rays *rays, const mlib_genvolume *vol, void *buffer); mlib_status mlib_VolumeRayCast_General_Parallel_Trilinear_S16_S16( mlib_rays *rays, const mlib_genvolume *vol, void *buffer); mlib_status mlib_VolumeRayCast_General_Divergent_Nearest_U8_Bit( mlib_rays *rays, const mlib_genvolume *vol, void *buffer); mlib_status mlib_VolumeRayCast_General_Divergent_Nearest_U8_U8( mlib_rays *rays, const mlib_genvolume *vol, void *buffer); mlib_status mlib_VolumeRayCast_General_Divergent_Nearest_S16_S16( mlib_rays *rays, const mlib_genvolume *vol, void *buffer); mlib_status mlib_VolumeRayCast_General_Divergent_Trilinear_U8_U8( mlib_rays *rays, const mlib_genvolume *vol, void *buffer); mlib_status mlib_VolumeRayCast_General_Divergent_Trilinear_S16_S16( mlib_rays *rays, const mlib_genvolume *vol, void *buffer); DESCRIPTION
Each of these functions casts a ray (or rays) through a three-dimensional(3D) data set, then computes and returns the interpolated samples at each step along the way. In trilinear interpolation, the value at point P is computed from its eight surrounding neighbors based on the equation below. P = (1-a)*(1-b)*(1-c)*P0 + a*(1-b)*(1-c)*Px + (1-a)*b*(1-c)*Py + (1-a)*(1-b)*c*Pz + a*b*(1-c)*Pxy + a*(1-b)*c*Pxz + (1-a)*b*c*Pyz + a*b*c*Pxyz where a, b, and c are the fractional parts of the coordinates of point P. The trilinear interpolation is represented by the following figure: Printed copy or docs.sun.com displays a figure that represents the trilinear interpolation. In nearest neighbor operation, the sample value at point P is replaced by the value of the nearest neighbor voxel. PARAMETERS
Each of the functions takes the following arguments: rays Casting rays. vol Volume data that consists of slices. buffer Working buffer. RETURN VALUES
Each of the functions returns MLIB_SUCCESS if successful. Otherwise it returns MLIB_FAILURE. ATTRIBUTES
See attributes(5) for descriptions of the following attributes: +-----------------------------+-----------------------------+ | ATTRIBUTE TYPE | ATTRIBUTE VALUE | +-----------------------------+-----------------------------+ |Interface Stability |Committed | +-----------------------------+-----------------------------+ |MT-Level |MT-Safe | +-----------------------------+-----------------------------+ SEE ALSO
mlib_VolumeRayCast_Blocked(3MLIB), attributes(5) SunOS 5.11 2 Mar 2007 mlib_VolumeRayCast_General(3MLIB)
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