urn:nasa:pds:nh_mvic 3.0 1.19.0.0 Product_Bundle 2026 This bundle contains collections of raw and processed data from the MVIC instrument onboard the New Horizons spacecraft, as well as a calibration collection of ancillary files used to calibrate the data from raw to processed. 2026-03-06 3.0 (NH SOC) Added KEM2 collections for K7 delivery. 2025-05-01 2.0 (SBN:T. Barnes) Adding Pluto Encounter Raw/Calibrated collections from PDS4 migration by PDS-SBN. Updated the readme.txt file to be more generic. 2023-04-27 1.0 Created during PDS4 migration by PDS-SBN (B. Hirsch). New Horizons Mission urn:nasa:pds:context:investigation:mission.new_horizons bundle_to_investigation New Horizons Kuiper Belt Extended Mission 1 Mission urn:nasa:pds:context:investigation:mission.new_horizons_kem1 bundle_to_investigation New Horizons Kuiper Belt Extended Mission 2 Mission urn:nasa:pds:context:investigation:mission.new_horizons_kem2 bundle_to_investigation New Horizons Spacecraft Host The New Horizons spacecraft observatory includes propulsion, navigation, and communications systems, plus the payload. The spacecraft is roughly 2.5 meters across and its mass is 465 kg including propellant. Design features include 64 Gbits of redundant solid-state data storage, a 290 m/s propulsion budget, and the capability to transmit data from 32 AU at almost 1 kilobit/second. urn:nasa:pds:context:instrument_host:spacecraft.nh is_instrument_host Multispectral Visible Imaging Camera Instrument MVIC is an imager that operates at both visible and near-infrared wavelengths using seven separate Charge-Coupled Device detectors (CCDs). On one of those CCDs, the Pan Frame array, operates as a single-frame array that is exposed to light and then transfers all of its lines to an image with the same dimensions as the CCD. The other six CCDs all use Time Delay and Integration (TDI i.e. multi-line push broom; see TDI section below) to construct images of fixed width and of variable height, which height is dependent on the scan rate and time duration of the observation. Four CCDs have color filters (methane, red, blue and near-infrared) for producing color maps and three CCDs have panchromatic filters for observations where maximum sensitivity to faint light levels is required. In all cases, the light passes from the telescope through a filter and is focused onto the CCDs. MVIC is part of the RALPH instrument package urn:nasa:pds:context:instrument:nh.mvic is_instrument urn:nasa:pds:context:resource:resource.nh_mvic_online has_resource urn:nasa:pds:nh_documents:mission bundle_to_document Document collection for the New Horizons mission. urn:nasa:pds:nh_documents:ralph bundle_to_document Document collection for the Ralph instrument suite. Archive readme.txt 0 UTF-8 Text Line-Feed urn:nasa:pds:nh_mvic:kem1_raw::1.0 Primary bundle_has_data_collection urn:nasa:pds:nh_mvic:kem2_raw::1.0 Primary bundle_has_data_collection urn:nasa:pds:nh_mvic:kem1_cal::1.0 Primary bundle_has_data_collection urn:nasa:pds:nh_mvic:kem2_cal::1.0 Primary bundle_has_data_collection urn:nasa:pds:nh_mvic:calibration_files::1.0 Primary bundle_has_calibration_collection urn:nasa:pds:nh_mvic:pluto_raw::1.0 Primary bundle_has_data_collection urn:nasa:pds:nh_mvic:pluto_cal::1.0 Primary bundle_has_data_collection