CONV(1)
π NAME π
okay so this is the manual page for CONV(1) β yes bestie, the whole page is literally just called conv, that's the name, that's it, we're keeping it real simple here. π
β¨ SYNOPSIS β¨
conv idec jdec filter_file input output
that's the whole summoning ritual. five little args and you're filtering images. π
π«Ά DESCRIPTION π«Ά
okay so first thing you gotta know: this program is part of GMTSAR. iconic of it. π
conv [GMTSAR] - 2-D image convolution
that's the one-liner, that's the vibe check, two-dimensional image convolution, no cap. π₯
here's the arg breakdown, one by one, because we do NOT skip details in this house:
idecβ the row decimation factor. fr fr, that's what it is. πjdecβ the column decimation factor. yep, the other direction. β¨filter_fileβ the filter file you're using, e.g.filters/gauss17x5. that's the example, don't come for me. πinputβ the name of the file you wanna filter. it's eitherI*2orR*4and yes that matters, it's giving format-specific. πoutputβ the name of the filtered output file. and heads up:R*4 only. that's not a suggestion bestie, that's the rule. π
now the examples, because examples are the main character:
conv 4 2 filters/gauss9x5 IMG-HH-ALPSRP109430660-H1.0__A.PRM test.grd
that one makes and filters the amplitude file from an SLC-file. look at her go. π
conv 4 2 filters/gauss5x5 infile.grd outfile.grd
and that one filters a float file. simple, clean, ate. πΈ
π and now... the exact same thing again π
okay listen, not me repeating myself β the manpage literally says it twice, so I'm saying it twice, because the ONE RULE is I don't drop a single crumb of info. so here we go, round two, same energy: π¦
conv [GMTSAR] - 2-D image convolution
Usage: conv idec jdec filter_file input output
idecβ row decimation factor. still. πjdecβ column decimation factor. still. πfilter_fileβ e.g.filters/gauss17x5. πinputβ name of file to be filtered (I*2orR*4). β¨outputβ name of filtered output file (R*4 only). π«Ά
examples, take two, same exact text, zero edits:
examples: conv 4 2 filters/gauss9x5
IMG-HH-ALPSRP109430660-H1.0__A.PRM test.grd (makes and filters
amplitude file from an SLC-file)
conv 4 2 filters/gauss5x5 infile.grd outfile.grd (filters a float
file)
see? consistent. dependable. a little repetitive. honestly kind of iconic of the manpage to just say it twice. π
and that's the whole page, bestie!! π§ this one is from the conv manual, CONV(1), dated May 2024 β shoutout to May 2024, she really came through. go filter something. periodt. π
β¨
π¦ where this page comes from
- debian trixie: gmtsar-core 6.5+ds-3 Β· GPL-3.0-only
- ubuntu questing: gmtsar-core 6.5+ds-3
- ubuntu resolute: gmtsar-core 6.6+ds-1build1 Β· GPL-3.0-only
- ubuntu stonking: gmtsar-core 6.7+ds-2 Β· GPL-3.0-only
- π girlified by deepseek-ai/DeepSeek-V4.1-Flash on : a language model's rewrite of the original, under its terms