High Resolution Imaging Science Experiment (HiRISE) Stamp Layer
From JMARS Wiki
The HiRISE Stamp Layer will display stamps for all of the images taken by the High Resolution Imaging Science Experiment (HiRISE) aboard the Mars Reconnaissance Orbiter. While the query interface is similar to the THEMIS Stamp Layer, there are some differences which allow users to search for images by the many parameters associated with HiRISE images. For more information on using the HiRISE Stamp Layer, click on the title above.

[edit] Open the HiRISE Stamp Layer
- Open the Stamp Layer: Chose "Add New Layer" -> "Stamps" -> "HiRISE 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 Image ID Numbers |
| 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 | Any Orbit Range Blank - All Orbits |
| Advanced Parameters | |
| Mission Phase | POST-MOI - Post Mars Orbit Insertion PSP - Primary Science Phase Transition - Aerobraking Phase Blank - All Mission Phases |
| Min/Max Map Scale | Any Resolution Blank - All Orbits |
| Min/Max Lines | xxx Blank - Any Lines |
| Min/Max Line Samples | xxx Blank - Any Line Samples |
| Min/Max Solar Longitude | 0 - 360 - 0=Northern Vernal Equinox Blank - All Solar Longitudes |
| Min/Max Local Time (24hr) | 00:00-24:00 - Given as HH:MM Blank - All Times |
| 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=HiRISE Directly Overhead, 90=HiRISE on the Horizon Blank - All Emission Angles |
| Phase Angle | 0 - 180 - 0=HiRISE and Sun In-Line, 90=HiRISE and Sun at 90deg Angle Blank - All Phase Angles |
| Slant Distance | 0 - 5000 - Distance from sub-MGS point to image center (in meters) Blank - All Slant Distances |
| Stereo Flag | Yes - Image is part of a Stereo Pair No - Image is not part of a Stereo Pair Blank - All Flags |
| Rationale Description | Any Text Blank - Any Rationale Descriptions |
- Search Field Descriptions
- Image ID
- A unique identifier for each image commanded; follows the pattern XXX_oooooo_####, where:
- a) XXX is a 3-digit mission phase identifier
- b) oooooo is the zero padded 6 digit orbit number
- c) #### is a zero-padded four digit target code (which is latitude dependent)
- A unique identifier for each image commanded; follows the pattern XXX_oooooo_####, where:
- Image ID
- 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 this image was observed. By definition, orbits begin at the ascending equator crossing of Global Surveyor's polar orbit.
- Orbit
- Mission Phase
- The MRO/HiRISE mission has been divided into the following phases:
- Post-MOI Post Mars Orbit Insertion
- PSP Primary Science Phase
- Transition Aero-Breaking Period Prior to Final Orbit
- The MRO/HiRISE mission has been divided into the following phases:
- Mission Phase
- Map Scale
- Spatial resolution (in pixels per meter) at the center of the image.
- Map Scale
- Lines
- Lines
- Line Samples
- Line Samples
- 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
- Local 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 Time'
- 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.
- Incidence Angle
- Emission Angle
- Measured from the center of the image, this is the angle between the HiRISE and a "normal" drawn perpendicular to the planet's surface. In most cases, the HiRISE is looking "straight down" and the emission angle is thus close to 0°.
- Emission Angle
- Phase Angle
- This is the angle between the sun, the surface, and the HiRISE at the time the picture was obtained.
- Phase 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
- Stereo Flag
- Designates which images are part of a stereo pair.
- Stereo Flag
- Rationale Description
- A short description of why the image was targeted.
- Rationale Description
[edit] Stamp Layer Functions
- The HiRISE 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.

