MESSENGER MDIS Narrow-angle Map-Projected Regional Targeted Mosaic (RTMNAC)

RTMNAC – Narrow-angle Map-projected Regional Targeted Mosaic

Instrument: MESSENGER Mercury Dual Imaging System

PDS4 Bundle: urn:nasa:pds:messenger_mdis_8001DOI: 10.17189/a666-n296

For more information about MDIS RTM products, see the CDR/RDR Product SIS.

The Mercury Dual Imaging System (MDIS) Narrow-angle Map-projected Regional Targeted Mosaic (RTMNAC) data products include regional mosaics of target observations directed at regions of interest. RTMNAC observations are NAC image strips acquired either for high-resolution imaging of morphology or as context for Mercury Atmospheric and Surface Composition Spectrometer (MASCS) or Mercury Laser Altimeter (MLA) observations. Each mosaic is map-projected in an orthographic projection. NAC mosaics contain 4 backplanes: observation ID, solar incidence angle, emission angle, and phase angle.

The observations that make up the RTMNAC data set are scattered throughout the Calibrated Data Record (CDRNAC) data set linked by a Site ID in their PDS label. In this data set, the images for each Site ID are collected, coregistered if they are multispectral, map-projected, and photometrically corrected to a standard geometry of incidence angle, i=30°, emission angle, e=0°, and phase angle, g=30°. All map-projections are orthographic and near the native resolution of the images to preserve spatial resolution.

The sequence of processing for creation of an RTMNAC from CDRNACs and Derived Data Records (DDRNACs) is the following:

  1. Experiment Data Records (EDRNACs) are assembled from raw data.

  2. Radiance images are created from the EDRNACs and calibration files.

  3. Radiance is converted to I/F CDRNACs by dividing by [pi*(solar flux at 1 AU)/(heliocentric distance in AU)2].

  4. I/F is photometrically corrected to i=30°, e=0°, and g=30°.

  5. Gimbal positions are extracted from the spacecraft housekeeping.

  6. DDRNACs are created. The surface intercept on a model of Mercury’s surface is calculated for each spatial pixel. The angles of this pixel relative to the equatorial plane and reference longitude constitute the latitude and longitude of the pixel. For that latitude and longitude, solar incidence, emission, and phase angles are determined.

  7. I/F corrected to i=30° and e=0° is map-projected into RTMs using the latitude and longitude information in the DDRNACs. The same procedure is used on DDRNACs to assemble the backplanes with derived information. They are appended to the image band in the following order:

    1. Observation ID

    2. Solar Incidence Angle

    3. Emission Angle

    4. Phase Angle

MDIS observing scenarios pertaining to the RTMs are the following:

  • Pixel Binning: Some RTM images are unbinned and 1024 x 1024 pixels. Some images are 2x2 pixel binned in the focal plane hardware (also known as “on-chip” binning), resulting in 512 x 512 images, only where needed to increase image cadence and along-track overlap.

  • 12-8 bit compression: Images are read off the detector in 12-bit format. 12-bit images may be converted to 8-bit images using one of eight lookup tables (LUTs). Typically, NAC image strips have been converted to 8 bits.

  • FAST/DPCM compression: All the images are compressed losslessly using FAST/DPCM compression as they are read out of the DPU, to conserve recorder space. Once the data are written to the recorder, they can be uncompressed and recompressed more aggressively in the spacecraft MP.

  • Wavelet compression: Images may be integer wavelet transform-compressed in the MP, typically at 4:1 for monochrome data, but any value from 1 to 32 can be used. Lossless compression was used when downlink allowed.

  • Exposure Control: The exposure time of MDIS images can be set manually by command, or automatically by the software. In manual mode, exposure times from 1-989, 1001-1989, …, to 9001-9989 ms are available. In autoexposure mode the exposure time of the next image is computed by DPU software, and cannot exceed 989 ms in duration. If the time of the next image occurs before the calculation can be completed, and pixel binning or filter position change, then the algorithm compensates for predicted changes in scene brightness and filter transmission using an onboard data structure. Most images in RTMs were acquired using automatic exposure, with an upper limit on exposure time to limit image smear.

  • Pointing: The MDIS imagers are mounted on a pivot platform, which is itself mounted to the MESSENGER spacecraft deck. The pivot platform is controlled by a stepper motor, which is controlled by the DPU. The pivot platform can move in either direction. The total range of motion is 240 degrees, limited by mechanical “hard” stops, and is further constrained by “soft” stops applied by the software. The nominal pointing position for MDIS is defined as 0 degrees, aligned with the spacecraft +Z axis and the boresight for several other instruments. The range of the soft stops is set to 40 degrees in the spacecraft –Y direction (toward the MESSENGER sunshade) and +50 degrees in the +Y direction (away from the sunshade). The pivot position can be commanded in intervals of 0.01 degrees within this range. During acquisition of targeted observations, the pointing of the pivot varied depending on the type of target and whether the observation was coordinated with MASCS or MLA. NAC image strips are mostly pointed at low to moderate emission angles, and solar incidence angles near 68 degrees. However, NAC images taken to provide context for MASCS or MLA observations are pointed close to the +Z axis coaligned with the appropriate other instrument.

MDIS RTMNAC products have the following file names:

MDIS_RTM_N01_ssssss_nnnnnnn_v.IMG (with detached PDS label)

where:

MDIS = instrument = Mercury Dual Imaging System

RTM = product type = Regional Targeted Mosaic

N = camera = NAC

01 = bands = 01 for the NAC because it is a single-band imager

sssssss = 6-digit integer giving the unique Site ID of the region covered by the product

nnnnnnn = image observation ID of the first image (lowest ID)

v = version number

In ODE, RTMNAC products have the following product IDs:

MDIS_RTM_N01_SSSSSS_NNNNNNN_V