Image Sets  03 September, 2009 07:34

New Images From 03 September 2009 Added

09-246_07.05.11_VMC_Img_No_1.pngNew images have been posted to the image database. These images are from the VMC observation on 03 September 2009. To access the images click the link below. Also you can access the Celestia file to see where the images were captured and access the raw data in the zip file (for more details see Help us with the VMC)



03/09/2009 07:05-07:34 Gallery

Celestia Script

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Image Sets  02 September, 2009 17:43

New Images From 02 September 2009 Added

09-245_17.17.45_VMC_Img_No_1.pngNew images have been posted to the image database. These images are from the VMC observation on 02 September 2009. To access the images click the link below. Also you can access the Celestia file to see where the images were captured and access the raw data in the zip file (for more details see Help us with the VMC)



02/09/2009 17:17-17:47 Gallery

Celestia Script

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Image Sets  01 September, 2009 07:18

New Images From 01 September 2009 Added

09-244_06.49.10_VMC_Img_No_1.pngNew images have been posted to the image database. These images are from the VMC observation on 01 September 2009. To access the images click the link below. Also you can access the Celestia file to see where the images were captured and access the raw data in the zip file (for more details see Help us with the VMC)



01/09/2009 06:49-07:18 Gallery

Celestia Script

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   Slideshow
VMC submission by Mike Malaska - 24 Hour Image Processing. To make the image, raw images No 8 and No 16 were processed through the rgb2png utility, then image No 8 was aligned and placed under image No 16. Contrast for No.8 was adjusted to match as well as a blending mask added. Then an overall curves layer was added, followed by a Channel mix layer, then Hue/Saturation was increased +50 and a second curves layer added. Known residual artifacts were clone stamped out. Then a copy was converted to grayscale using a B&W conversion layer, and this image HIPassed by 5 pixels and overlaid onto the Gaussian blurred color layer. Image Credit: Mike Malaska/ESA 5 VMC observations obtained early February 2010 show that clouds that form in the morning disappear in the afternoon. The attached image composite shows the five individual observations at different Martian day times. Roman Makhin: I took 7 images from the Dec 23rd 2009 (2009-12-23_01.13-01.42) observation: 09-357_01.20.42_VMC_Img_No_11.raw, 09-357_01.23.38_VMC_Img_No_15.raw, 09-357_01.26.34_VMC_Img_No_19.raw, 09-357_01.29.30_VMC_Img_No_23.raw, 09-357_01.32.26_VMC_Img_No_27.raw, 09-357_01.35.22_VMC_Img_No_31.raw and 09-357_01.38.18_VMC_Img_No_35.raw. I extracted the colour information from them using version 3 of the vmc2rgb utility, then processed the images through colour mixer in GIMP and, finally, applied auto white balance. I was using Auto Pano Giga 2.0.6 software (spherical projection, exposure correction) to create the mosaic. Image Credits: ESA/Roman Makhin Image submitted by Ted Stryk, Powell, TN, USA. Ted writes: Credit: ESA/Peter Wellmann