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.SH NOTES |
| 93 |
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This tool overlaps with |
| 94 |
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.I dctimestep, |
| 95 |
< |
but provides some important capabilities. |
| 96 |
< |
First, |
| 95 |
> |
but provides some missing capabilities. |
| 96 |
> |
Foremost, |
| 97 |
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.I pvsum |
| 98 |
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reads and can produce spectral pictures and matrices, whereas |
| 99 |
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.I dctimestep |
| 100 |
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expects and requires 3-component pictures and matrices throughout. |
| 101 |
< |
Changing the data structures in |
| 102 |
< |
.I dctimestep |
| 103 |
< |
proved too difficult and likely to |
| 104 |
< |
lead to a less efficient implementation, especially on systems with |
| 105 |
< |
limited memory. |
| 106 |
< |
In contrast, |
| 101 |
> |
In addition, |
| 102 |
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.I pvsum |
| 103 |
|
accelerates picture sums on Unix systems with more |
| 104 |
< |
memory and processint ability. |
| 105 |
< |
Second, operation was simplified by focusing on the Daylight Coefficient |
| 104 |
> |
memory and CPU cores. |
| 105 |
> |
Operations were simplified by focusing on the Daylight Coefficient |
| 106 |
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command form, where the DC matrix is represented as a collection of |
| 107 |
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pictures. |
| 108 |
< |
By excluding the other operation modes of |
| 109 |
< |
.I dctimestep, |
| 110 |
< |
new functionality could be explored and optimized, |
| 111 |
< |
such as floating-point support and |
| 117 |
< |
sending output to commands as well as files. |
| 108 |
> |
Finally, |
| 109 |
> |
.I pvsum |
| 110 |
> |
offers more flexible floating-point support and |
| 111 |
> |
can output to commands as well as files. |
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.SH AUTHOR |
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Greg Ward |
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.SH "SEE ALSO" |