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Viking Camera Stamp Layer
The Viking Camera Stamp Layer will display stamps for all images acquired by the Visible Imaging Subsystem (VIS) onboard the Viking 1 & 2 orbiters. While the search interface is similar to the THEMIS Stamp Layer, there are some differences that allow users to search for images based on the unique parameters associated with Viking VIS images.
Open the Viking Camera Stamp Layer
- Open the Stamp Layer: Chose "Add New Layer" -> "Imagery" -> "Viking" OR Chose "Add New Layer" -> "Instrument" -> "Viking" .
- Search Parameter Categories: The search parameters are divided into categories since there are so many of them. Clicking on the down arrow on the right side of the category name will reveal all the search parameters in that category. The categories are:
- Basic Parameters
- Advanced Parameters
- Enter Search Parameters: It is not necessary to enter values for each parameter, but the more specific your search the faster it will be. The allowable values for each field are given in the quick reference table below followed.
- Perform Image Search: Clicking OK will make the Stamp Layer perform the search and display the results. Depending on how specific the search parameters are, it may take the Stamp Layer a few minutes to find and create stamps for all of the images. Once the stamps are displayed in the Viewing Window, users can right-click on an outline to either render the image (display the image data in JMARS) or view the image in a web browser.
Viking Search Parameter Glossary
Filter Type |
Acceptable Values |
Description |
Image ID(s) |
Any Specific Image ID Number(s) |
A unique identifier for each image commanded; follows the pattern XXXMYY, where:
|
Spacecraft Name |
Viking 1 - Only images from the Viking 1 orbiter |
This field identifies which of the two identical Viking orbiters were used to acquire the observations. |
Min/Max Longitude |
0 to 360(East Longitude = Positive) |
This is the approximate longitude on the planet Mars of the image center. All values are based on the IAU 2000 aerocentric model of Mars with east positive longitude. |
Min/Max Latitude |
90 to -90(North Latitude = Positive) |
This is the approximate latitude on the planet Mars of the image center. All values are based on the IAU 2000 aerocentric model of Mars with north positive latitude. |
Min/Max Orbit |
1 - 1485(Viking 1) |
Viking spacecraft orbit during which an observation was acquired. |
Mission Phase |
Continuation Mission |
The Viking orbiter missions were both divided into the following phases:
|
Instrument |
VIS Camera A(Only images from Camera A) |
The VIS subsystem consisted of two identical cameras: A & B.
|
Filter |
Blue |
The VIS cameras took images using the following filters:
|
Min/Max Sample Resolution |
0.0070 km - 30.0000 km |
The "horizontal" resolution of the image pixels, in km/pixel. |
Min/MaxLine Resolution |
0.0070 km - 32.5000 km |
The "vertical" resolution of the image pixels, in km/pixel. |
Min/MaxLocal Solar Time |
00:00 - 24:00(Given as HH:MM in Mars time) |
This is the local time on Mars at the center of the image relative to a division of the Martian day into 24 equal parts. A martian day is slightly longer than 24 hours and 37 minutes, so these times are in "Mars hours, Mars minutes and Mars seconds". |
Min/Max Solar Longitude |
0 - 360(Northern Vernal Equinox = 0) |
This is the position of Mars relative to the Sun measured in degrees from the vernal equinox (start of northern Spring). This number is used as a measure of Martian seasons. (Also known as heliocentric longitude and abbreviated Ls.)
|
Min/Max Phase Angle |
0 - 180 (Viking VIS camera and Sun In-Line = 0) |
This is the angle between the sun, the surface, and the Viking orbiter at the time the picture was obtained. |
Min/Max Incidence Angle |
0 - 180(Sun Directly Overhead = 0) |
Derived for the center of the image, this is the angle between the Sun and a "normal" line drawn perpendicular to the planet's surface at the time the image was acquired. A higher incidence angle means that the sun closer to the horizon. |
Min/Max Emission Angle |
0 - 180(Viking Directly Overhead = 0) |
Measured from the center of the image, this is the angle between the Viking orbiter and a "normal" line drawn perpendicular to the planet's surface. |
Min/Max North Azimuth Angle |
0 - 360(Image Centerline Along Polar Axis = 0) |
The angle between the right edge of the image and north. (ex: Image Perpendicular to Longitude Lines = 0) |
Min/Max Slant Distance |
0 - 760,000(Distance (m) from sub-orbiter point to image center) |
This number is similar to the spacecraft altitude, but also takes into account the emission angle. If the emission angle is 0 then this number is the same as the spacecraft altitude. If the emission angle is much greater than 0, then the "slant distance" to the surface at the center of the image is also greater than the spacecraft altitude. |
Notes |
Any Text |
A short description or miscellaneous information about the image. |
Stamp Layer Functions
The Viking Camera Stamp Layer's functions are identical to the functions of the Stamp Layer and are explained in detail on the Stamp Layer page.