urn:nasa:pds:nh_mvic:kem2_raw 1.0 1.19.0.0 Product_Collection Reuter, D. C.; Lunsford, A.; Howett, C.; Protopapa, S.; Singer, K. N.; Stern, S. A. Enke, B.; Gobat, C.; Keeney, B.; Crombie, M. K.; Parker, J. Wm. 2026 10.26007/mx04-jc97 This data set contains raw data taken by the New Horizons Ralph/MVIC instrument during the KEM2 CRUISE mission phase. It contains stellar flux calibrations and high phase angle imaging of Saturn, Uranus, and Neptune. 2024-08-14 1.0 Initial version of PDS4 dataset produced by the New Horizons SOC 2023-08-09T02:35:27.851000Z 2023-09-23T16:05:06.895000Z Science Raw New Horizons Kuiper Belt Extended Mission 2 Mission urn:nasa:pds:context:investigation:mission.new_horizons_kem2 collection_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 NGC 3532 Star Cluster urn:nasa:pds:context:target:star_cluster.ngc_3532 data_to_target Saturn Planet urn:nasa:pds:context:target:planet.saturn data_to_target Uranus Planet urn:nasa:pds:context:target:planet.uranus data_to_target Neptune Planet urn:nasa:pds:context:target:planet.neptune data_to_target urn:nasa:pds:context:resource:resource.nh_mvic_colxn_kem2_raw_online has_resource urn:nasa:pds:context:resource:resource.nh_mvic_online has_resource urn:nasa:pds:nh_mvic:kem2_raw:overview::1.0 collection_to_document MVIC KEM2 Raw Collection Overview urn:nasa:pds:nh_mvic:kem2_cal collection_to_data MVIC KEM2 Cal Data Collection urn:nasa:pds:nh_mvic:calibration_files collection_to_calibration MVIC Calibration Files Collection urn:nasa:pds:nh_documents:mission collection_to_document Document collection for the New Horizons mission. urn:nasa:pds:nh_documents:ralph collection_to_document Document collection for the Ralph instrument package, which houses both LEISA and MVIC. urn:nasa:pds:nh_documents:mission:nhkem2_mission_overview collection_to_document urn:nasa:pds:nh_documents:ralph:ralph_ssr collection_to_document Data collection_kem2_raw.csv 0 PDS DSV 1 181 Line-Feed Comma 2 0 Member Status 1 ASCII_String 1 %1s LIDVID_LID 2 ASCII_LIDVID_LID 255 %-255s inventory_has_member_product