From Edward Arnold GRAFTON
@. . . . . . The attached images are for the 5/29 image for the red,
blue and luminance channels. I changed the technique for this image a little
from before by gathering 3 images for the red filtered image (which were
averaged together) instead of only one from before. This may help in providing
more accurate color data. I hope that Yukio Morita has some good luck with his
new technique.
(30 May 2001 email)
@･････This image was taken
06/03/01 at 7:28 UT from Houston, Texas.
http://www.egrafton.com/06-03-01.jpg
The attached images are from the
6/03 image (below) for the red, blue and luminance channels.
http://www.egrafton.com/06-03-01.jpg
(
@･････I see now that
the 5/29 image is linked to the CMO gallery. I had overlooked it before because
it did not have a thumbnail image but just "click". Perhaps if I were
not so tired from working all day and staying up many nights to get images of
Mars I would not have made this mistake. Thanks for clearing this up for me.
I looked at MORITA's
images on 25 May and they are excellent. Many thanks to OKANO
for his innovation in image processing with the LRGB method. A couple of
years ago my friends and I came up with the CMY method of producing images.
Perhaps you saw our article in the Dec. 1998 issue of S&T.
Today I received the issues of
CMO and was very excited to get them. They will provide me many hours of
pleasant reading but more importantly an education. Unlike yourself and your
peers, I am not an expert on Mars but have learned a lot in the last few weeks.
The CMO will issues will be of much value to me to become a trained Mars
observer. Yours truly
（4 June 2001 email）
Ed GRAFTON (