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author | Thomas Vander Stichele <thomas@apestaart.org> | 2005-12-06 19:55:58 +0000 |
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committer | Thomas Vander Stichele <thomas@apestaart.org> | 2005-12-06 19:55:58 +0000 |
commit | bdb814f6ef56edca67e1241eb16df22fdd8ab17c (patch) | |
tree | 7b43c9dfbf67b852503d263a322064f0101bf591 /sys/qcam | |
parent | 04ad447fcfa1502907339a6a68e975bb6d35536a (diff) | |
download | gst-plugins-bad-bdb814f6ef56edca67e1241eb16df22fdd8ab17c.tar.gz gst-plugins-bad-bdb814f6ef56edca67e1241eb16df22fdd8ab17c.tar.bz2 gst-plugins-bad-bdb814f6ef56edca67e1241eb16df22fdd8ab17c.zip |
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Original commit message from CVS:
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Diffstat (limited to 'sys/qcam')
-rw-r--r-- | sys/qcam/dark.c | 58 | ||||
-rw-r--r-- | sys/qcam/gstqcamsrc.c | 26 |
2 files changed, 42 insertions, 42 deletions
diff --git a/sys/qcam/dark.c b/sys/qcam/dark.c index ac462b36..cdfa2ab8 100644 --- a/sys/qcam/dark.c +++ b/sys/qcam/dark.c @@ -25,17 +25,17 @@ OTHER DEALINGS IN THE SOFTWARE. ******************************************************************/ /* Fixdark - Routine to repair dark current artifacts in qcam output. - Basic idea: the Qcam CCD suffers from "dark current"; - that is, some of the CCD pixels will leak current under - long exposures, even if they're in the dark, and this - shows up as ugly speckling on images taken in low light. + Routine to repair dark current artifacts in qcam output. + Basic idea: the Qcam CCD suffers from "dark current"; + that is, some of the CCD pixels will leak current under + long exposures, even if they're in the dark, and this + shows up as ugly speckling on images taken in low light. - Fortunately, the leaky pixels are the same from shot to - shot. So, we can figure out which pixels are leaky by - taking some establishing shots in the dark, and try to - fix those pixels on subsequent shots. The dark - establishing shots need only be done once per camera. + Fortunately, the leaky pixels are the same from shot to + shot. So, we can figure out which pixels are leaky by + taking some establishing shots in the dark, and try to + fix those pixels on subsequent shots. The dark + establishing shots need only be done once per camera. */ #ifdef HAVE_CONFIG_H @@ -77,7 +77,7 @@ read_darkmask() } if (fread(master_darkmask1, sizeof(unsigned char), MAX_WIDTH*MAX_HEIGHT, fp) != - MAX_WIDTH*MAX_HEIGHT) { + MAX_WIDTH*MAX_HEIGHT) { #ifdef DEBUG fprintf(stderr, "Error reading darkfile\n"); #endif @@ -88,14 +88,14 @@ read_darkmask() for (x = 0; x < MAX_WIDTH; x += 2) { min_bright = master_darkmask1[y][x]; if (y < MAX_HEIGHT-1 && master_darkmask1[y+1][x] < min_bright) - min_bright = master_darkmask1[y+1][x]; + min_bright = master_darkmask1[y+1][x]; if (x < MAX_WIDTH-1 && master_darkmask1[y][x+1] < min_bright) - min_bright = master_darkmask1[y][x+1]; + min_bright = master_darkmask1[y][x+1]; if (y < MAX_HEIGHT-1 && x < MAX_WIDTH-1 && master_darkmask1[y+1][x+1] < min_bright) - min_bright = master_darkmask1[y+1][x+1]; + min_bright = master_darkmask1[y+1][x+1]; master_darkmask2[y/2][x/2] = min_bright; - assert(y/2 < MAX_HEIGHT/2+1); - assert(x/2 < MAX_WIDTH/2+1); + assert(y/2 < MAX_HEIGHT/2+1); + assert(x/2 < MAX_WIDTH/2+1); } } @@ -103,14 +103,14 @@ read_darkmask() for (x = 0; x < MAX_WIDTH/2; x += 2) { min_bright = master_darkmask2[y][x]; if (y < MAX_HEIGHT/2-1 && master_darkmask2[y+1][x] < min_bright) - min_bright = master_darkmask2[y+1][x]; + min_bright = master_darkmask2[y+1][x]; if (x < MAX_WIDTH/2-1 && master_darkmask2[y][x+1] < min_bright) - min_bright = master_darkmask2[y][x+1]; + min_bright = master_darkmask2[y][x+1]; if (y < MAX_HEIGHT/2-1 && x < MAX_WIDTH-1 && master_darkmask2[y+1][x+1] < min_bright) - min_bright = master_darkmask2[y+1][x+1]; + min_bright = master_darkmask2[y+1][x+1]; master_darkmask4[y/2][x/2] = min_bright; - assert(y/2 < MAX_HEIGHT/4+1); - assert(x/2 < MAX_WIDTH/4+1); + assert(y/2 < MAX_HEIGHT/4+1); + assert(x/2 < MAX_WIDTH/4+1); } } @@ -121,15 +121,15 @@ read_darkmask() /* fixdark - We first record a list of bad leaky pixels, by making a - number of exposures in the dark. master_darkmask holds - this information. It's a map of the CCD. - master_darkmask[y][x] == val means that the pixel is - unreliable for brightnesses of "val" and above. + We first record a list of bad leaky pixels, by making a + number of exposures in the dark. master_darkmask holds + this information. It's a map of the CCD. + master_darkmask[y][x] == val means that the pixel is + unreliable for brightnesses of "val" and above. - We go over the image. If a pixel is bad, look at the - adjacent four pixels, average the ones that have good - values, and use that instead. + We go over the image. If a pixel is bad, look at the + adjacent four pixels, average the ones that have good + values, and use that instead. */ int diff --git a/sys/qcam/gstqcamsrc.c b/sys/qcam/gstqcamsrc.c index 901beca5..2bae6d85 100644 --- a/sys/qcam/gstqcamsrc.c +++ b/sys/qcam/gstqcamsrc.c @@ -40,19 +40,19 @@ GST_ELEMENT_DETAILS ("QCam Source", "Read from a QuickCam device", "Wim Taymans <wim.taymans@chello.be>"); -#define AE_NONE 3 - -#define DEF_WIDTH 320 -#define DEF_HEIGHT 224 -#define DEF_BRIGHTNESS 226 -#define DEF_WHITEBAL 128 -#define DEF_CONTRAST 72 -#define DEF_TOP 1 -#define DEF_LEFT 14 -#define DEF_TRANSFER_SCALE 2 -#define DEF_DEPTH 6 -#define DEF_PORT 0x378 -#define DEF_AUTOEXP AE_NONE +#define AE_NONE 3 + +#define DEF_WIDTH 320 +#define DEF_HEIGHT 224 +#define DEF_BRIGHTNESS 226 +#define DEF_WHITEBAL 128 +#define DEF_CONTRAST 72 +#define DEF_TOP 1 +#define DEF_LEFT 14 +#define DEF_TRANSFER_SCALE 2 +#define DEF_DEPTH 6 +#define DEF_PORT 0x378 +#define DEF_AUTOEXP AE_NONE static GstStaticPadTemplate gst_qcamsrc_src_factory = GST_STATIC_PAD_TEMPLATE ("src", |