SGHA Research

This information/article is copyright, 2006 by Cody Polston, Bob Carter and SGHA. All rights reserved.
Location: Shaffer Hotel, Mountainair, NM
Date taken: October 29, 2007
Photographer: C. Polston
M/E/EM fields: 7 nt
Camera Model : Sony MVC-CD 350, IR enhanced

 SGHA Research ~ Photograph analysis ~ Shaffer Hotel Photoss

A digital image can be treated as a data set to extract information. This is the information that we extracted from a digital photograph taken during a investigation at the Jerome Mining Museum.

Clicking on this image will open the photo in a new window. EXIF data is intact.

EXIF Data

Photo DSC03636
Date and Time 10/29/2007 8:27 PM
Exp. Time 1/40
F/Stop 3.8
Exp. Program Normal
Exp. Bias +2.0
Metering Mode Pattern
Light Source Unknown
Flash Flash fired
Focal Length compulsory flash mode
Focal Length (35 mm) return light not detected
ISO Speed 6.4;-;200
Orientation Normal
Dimensions 2048 x 1536
File Size 1372 KB

Clicking on this image will open the photo in a new window. EXIF data is intact.

EXIF Data

Photo DSC03637
Date and Time 10/29/2007 8:27 PM
Exp. Time 1/40
F/Stop 4.0
Exp. Program Normal
Exp. Bias +2.0
Metering Mode Pattern
Light Source Unknown
Flash Flash fired
Focal Length compulsory flash mode
Focal Length (35 mm) return light not detected
ISO Speed 6.4;-;200
Orientation Normal
Dimensions 2048 x 1536
File Size 1372 KB

A digital image can be treated as a data set to extract information. Each pixel's intensity value is a measure of how much energy was used to generate it within the band of spectrum used to produce the image. The sum of the pixel intensities is a measure of the total energy used to create the whole image.The highest output of energy from the object in the photograph is the lighter "glow" of the eclipse. The Sesmimetric value of the "glow" is estimated at 78.Another oddity is that the "warm" area of the object is pushing away a cooler section of air.

In 3336, light refraction is reveiled showing that the object in the image is 3-dimensional.

Spectrum

Refraction is the change in direction of a wave due to a change in its speed. This is most commonly seen when a wave passes from one medium to another. Refraction of light is the most commonly seen example, but any type of wave can refract when it interacts with a medium. The question is, what is bending the UV light while the visible is unaffected?

More interesting componets are found in the spectrum and IR bandpass filters applied to 3637.

The bandpass analysis suggests that the object is in the near infrared portion of the spectrum.

These photographs are are quite different than the other images that we have gotten with the X-spectrum camera. Currently we are attempting to find possible natural explainations for the phenomena recorded in these images.

Spectrum

Bandpass

Programs used for analysis: Image J , Scanalyze, Analyze 7.0

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