Viking Camera Stamp Layer
From JMARS Wiki
The Viking Camera Stamp Layer will display stamps for all the observations made by the visible cameras on the Viking 1 & 2 orbiters. The search interface is similar to the THEMIS Stamp Layer, but there are changes that allow users to search for images by the many parameters associated with Viking camera images.

[edit] Open the Viking Camera Stamp Layer
- Open the Stamp Layer: Chose "Add New Layer" -> "Stamps" -> "Viking Stamps".
- 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
- NOTE: A search can be done with parameters from multiple categories.
- 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:
- 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 by more detailed descriptions of each search parameter.
- 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.

| Filter Type | Acceptable Values |
| Basic Parameters | |
| Image ID(s) | Any Specific Image ID Numbers |
| Spacecraft Name | Viking 1 - Only images from the Viking 1 orbiter Viking 2 - Only images from the Viking 2 orbiter Both Orbiters - Images from the Viking 1 and Viking 2 orbiters |
| Min/Max Longitude | 0 - 360 - East Longitude = Positive, West Longitude = Negative Blank - All Longitudes |
| Min/Max Latitude | 90 - -90 - North Latitude = Positive, South Latitude = Negative Blank - All Latitudes |
| Min/Max Orbit | 1-1485 - Viking 1 1-706 - Viking 2 Blank - All Orbits |
| Advanced Parameters | |
| Mission Phase | Continuation Mission Extended Mission Pre-Orbital Science Primary Mission Survey Mission |
| Instrument | VIS Camera A - Only images from Camera A VIS Camera B - Only images from Camera B Blank - Images from Camera A and Camera B |
| Filters | ALL Blue Minus_Blue Violet Clear Green Red |
| Sample Resolution (km) | 0.0070-30.0000 Blank - All Sample Resolutions |
| Line Resolution (km) | 0.0070-32.5000 Blank - All Line Resolutions |
| Local Solar Time | 00:00-24:00 - Given as HH:MM Blank - All Times |
| Min/Max Solar Longitude | 0 - 360 - 0=Northern Vernal Equinox Blank - All Solar Longitudes |
| Min/Max Phase Angle | 0 - 180 - 0=MOC and Sun In-Line, 90=MOC and Sun at 90deg Angle Blank - All Phase Angles |
| Min/Max Solar Incidence Angle | 0 - 180 - 0=Sun Directly Overhead, 90=Sun on the Horizon Blank - All Incidence Angles |
| Min/Max Emission Angle | 0 - 180 - 0=Viking Directly Overhead, 90=Viking on the Horizon Blank - All Emission Angles |
| Min/Max North Azimuth Angle | 0 - 360 - 0=Image Perpendicular to Longitude Lines, 90=Image Parallel to Longitude Lines Blank - All North Azimuth Angles |
| Min/Max Slant Distance | 0 - 760,000 - Distance from sub-orbiter point to image center (in meters) Blank - All Slant Distances |
| Notes | Any Text Blank - All Notes |
- Search Field Descriptions
- Image ID
- A unique identifier for each image commanded; follows the pattern XXXMYY, where:
- a) XXX is the zero-padded orbit number
- b) M is the spacecraft id (Viking Orbiter 1 = A, Viking Orbiter 2 = B)
- c) YY is the zero padded, two-digit image number from the specified orbit
- A unique identifier for each image commanded; follows the pattern XXXMYY, where:
- Image ID
- Spacecraft Name
- This field identifies which of the two identical Viking orbiters were used to collect the observations.
- Spacecraft Name
- Longitude
- 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. (gives in degrees of East Longitude)
- Longitude
- Latitude
- 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 east positive longitude.
- Latitude
- Orbit
- Spacecraft orbit during which an observation was made.
- Orbit
- Mission Phase
- The Viking orbiter missions were both divided into the following phases:
- Pre-Orbital Science Launch - Mars Orbit Insertion
- Primary Mission Mars Orbit Insertion - November 1976
- Extended Mission November 1976 - May 1978
- Continuation Mission May 1978 - July 1979
- Survey Mision July 1979 - July 1980 (Viking 1 only)
- The Viking orbiter missions were both divided into the following phases:
- Mission Phase
- Instrument
- The VIS subsystem consisted of two identical cameras: A & B.
- Instrument
- Filters
- The VIS cameras took images using the following filters:
- Blue 0.35µm - 0.53µm
- Minus-Blue 0.48µm - 0.70µm
- Violet 0.35µm - 0.47µm
- Clear 0.35µm - 0.70µm
- Green 0.50µm - 0.60µm
- Red 0.55µm - 0.70µm
- The VIS cameras took images using the following filters:
- Filters
- Sample Resolution
- Sample Resolution
- Line Resolution
- Line Resolution
- Local Solar 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 long.
- Local Solar Time'
- Solar Longitude
- 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.)
- a) Northern Spring/Southern Autumn start at 0°
- b) Northern Summer/Southern Winter start at 90°
- c) Northern Autumn/Southern Spring start at 180°
- d) Northern Winter/Southern Summer begin at 270°
- 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.)
- Solar Longitude
- Phase Angle
- This is the angle between the sun, the surface, and the Viking orbiter at the time the picture was obtained.
- Phase Angle
- Solar Incidence Angle
- Derived for the center of the image, this is the angle between the Sun and a "normal" drawn perpendicular to the planet's surface at the time the image was acquired. A higher incidence angle means that a person standing on the ground would see the sun lower toward the horizon.
- Solar Incidence Angle
- Emission Angle
- Measured from the center of the image, this is the angle between the Viking orbiter and a "normal" drawn perpendicular to the planet's surface.
- Emission Angle
- North Azimuth Angle
- The angle between the right edge of the image and north. (Ex: 0=Image Perpendicular to Longitude Lines, 90=Image Parallel to Longitude Lines)
- North Azimuth Angle
- Slant Distance
- 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.
- Slant Distance
- Notes
- A short description or miscellaneous information about the image.
- Notes
[edit] Stamp Layer Functions
- The Viking Camera Stamp Layer's functions are identical to the functions of the Thermal Emission Image System (THEMIS) Stamp Layer and are explained in detail on its wiki page.

