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DAWN FC2 CALIBRATION IMAGES V1.0

Abstract ======== Framing Camera 2 is one of two identical units flying on Dawn spacecraft. This dataset includes the image files to be used in the calibration of the raw data throughout the mission. These files represent the behaviour of each individual pixel with respect to dark current generation and pixel-to-pixel non-uniformity as a function of the filter. As these are elaborated image products, not obtained from a specific image acquisition, they do not have any ancillary data.

HUYGENS ACP CALIBRATED ENGINEERING & SCIENCE DATA

This data set is composed of data produced during the descent to Titan on January 14 2005 from the ACP instrument (Engineering data) and also from the GCMS instrument (Science data) which analyses the gaseous products from ACP.

DAWN FC2 CALIBRATED MARS FLYBY IMAGES V1.0

Framing Camera 2 is one of two identical units flying on Dawn spacecraft. This dataset includes the Reduced Data Record (RDR) version of all available images acquired during the Mars Flyby phase. As in the original Raw data sets, in addition to the imagery, anciliary information is stored within the image headers, as well as a detailed account of all the reference files used for the calibartion. Calibration files needed for further processing are archived as a separate data set.

PVO VENUS ONMS CALIBRATED NEUTRAL DENSITY HIGH RES. V1.0

This data set has at least preliminary composition for every data point measured but not necessarily final composition values. The instrument was designed to determine the composition of the neutral thermosphere/exosphere of Venus. The term composition includes both the type of neutral gases present and their quantitative amount. The measurements begin at the orbit's periapsis altitude and extend to a limiting altitude at which the ambient signal becomes comparable to the gas background and/or detector measurement threshold. The neutral composition includes helium, atomic nitrogen, atomic oxygen, molecular nitrogen, carbon monoxide and carbon dioxide. The data reduction has been described in [NIEMANNETAL1980A] and [KASPRZAKETAL1980].

NEW HORIZONS SWAP PLUTO ENCOUNTER CALIBRATED V3.0

This data set contains Calibrated data taken by the New Horizons Solar Wind Around Pluto instrument during the Pluto encounter mission phase. This is VERSION 3.0 of this data set. This data set contains SWAP observations taken during the the Approach (Jan-Jul, 2015), Encounter, Departure, and Transition mission sub-phases, including flyby observations taken on 14 July, 2015, and departure and calibration data through late October, 2016. This data set completes the Pluto mission phase deliveries for SWAP. This is version 3.0 of this dataset. Changes since version 2.0 include the addition of data downlinked between the end of January, 2016 and the end of October, 2016, completing the delivery of all data covering the Pluto Encounter and subsequent Calibration Campaign. Also, updates were made to the calibration files, documentation, and catalog files. Finally, downlink data several days beyond the end of the nominal end of mission phase were included in this data set in an attempt to fill out the products at the nominal end of mission phase; refer to the CONFIDENCE_LEVEL_NOTE in this data set catalog for more details.

NEW HORIZONS SDC PLUTO CRUISE CALIBRATED V2.0

This data set contains Calibrated data taken by the New Horizons Student Dust Counter instrument during the pluto cruise mission phase. This is VERSION 2.0 of this data set. SDC collected science data intermittently during the hibernation years following the Jupiter encounter, designated as the PLUTOCRUISE phase. There were also Annual Checkouts (ACOs), STIM calibrations, Noise calibrations, and an anomaly in November, 2007. SDC's main science data collection periods were during hibernation. During ACOs, science data are taken intermittently but the user must be careful in analyzing these data since there is usually more activity on the spacecraft during hibernation. STIM and Noise refer to scheduled calibrations and are done with a regular cadence of one per year after the Jupiter encounter; they occurred sporadically in the early years of the mission. Note that some SDC data files have the same stop and start time and a zero exposure time. The reason for this is that the start and stop time for SDC data files are the event times for the first and last events in the files, so for files that contain a single event, these two values are the same. The changes in Version 2.0 were re-running of the ancillary data in the data product, updated geometry from newer SPICE kernels, minor editing of the documentation, catalogs, etc., and resolution of liens from the December, 2014 review, plus those from the May, 2016 review of the Pluto Encounter data sets. New observations added with this version (V2.0) include ongoing cruise observations from August, 2014 through January, 2015.

NEW HORIZONS MVIC PLUTO ENCOUNTER CALIBRATED V1.0

This data set contains Calibrated data taken by the New Horizons Multispectral Visible Imaging Camera instrument during the Pluto encounter mission phase. This is VERSION 1.0 of this data set.

NEW HORIZONS LORRI PLUTO ENCOUNTER CALIBRATED V1.0

This data set contains Calibrated data taken by the New Horizons Long Range Reconnaissance Imager instrument during the Pluto encounter mission phase. This is VERSION 1.0 of this data set.

MRO CRISM CALIBRATION DATA RECORD V1.0

This dataset contains CRISM VNIR and IR Calibration Data Records (CDRs), which are used to convert data from raw DNs to units of radiance or I/F for the CRISM instrument on MRO.

EPOXI EARTH OBS - MRI CALIBRATED IMAGES V2.0

This dataset contains calibrated, 750-nm filter images of Earth acquired by the Deep Impact Medium Resolution Visible CCD (MRI) during the EPOCh and Cruise 2 phases of the EPOXI mission. The MRI instrument was only used during the first Earth observing period on 18-19 March 2008 and the last two on 27-28 March and 04-05 October 2009. Each observing period lasted approximately 24 hours, and one MRI image was taken simultaneously with the first north/south scan of the HRI IR spectrometer at half-hour intervals to serve as context spectra. On 27-28 September 2009 during the first attempt at Earth south polar observations, a full set of MRI context images was acquired although the HRII and HRIV instruments were turned off by fault protection shortly after the sequence started. Version 2.0 includes the application of a horizontal destriping process, new absolute calibration constants for filters, and revised electronic crosstalk calibration files.

NEW HORIZONS SWAP PLUTO ENCOUNTER CALIBRATED V1.0

This data set contains Calibrated data taken by the New Horizons Solar Wind Around Pluto instrument during the Pluto encounter mission phase. This is VERSION 1.0 of this data set.

NEW HORIZONS PEPSSI PLUTO CRUISE CALIBRATED V1.0

This data set contains Calibrated data taken by the New Horizons Pluto Energetic Particle Spectrometer Science Investigation instrument during the pluto cruise mission phase. This is VERSION 1.0 of this data set.

DAWN FC1 CALIBRATED CRUISE CHECKOUT/CALIB IMAGES V1.0

Abstract ======== Framing Camera 1 is one of two identical units flying on Dawn spacecraft. This dataset includes the Reduced Data Record (RDR) version of all available images acquired during the initial checkout and pre-Vesta cruise phases (Checkout, Earth to Mars, and Mars to Vesta). As in the original Raw data sets, in addition to the imagery, ancillary information is stored within the image headers, as well as a detailed account of all the reference files used for the calibration. Calibration files needed for further processing are archived as a separate data set.

ROSETTA-ORBITER EARTH RPCMAG 3 EAR2 CALIBRATED V3.0

This dataset contains CALIBRATED DATA of the second Earth Flyby(EAR2). The closest approach (CA) took place on November 13, 2007 at 20:57

MR6/MR7 MARS INFRARED SPECTROMETER CALIBRATED DATA V1.0

This data set is a partial collection of spectra in digital form from the Mariner 6 and 7 Infrared Spectrometer experiments. All Mars and near-Mars sky spectra are included here, as well as some relevant laboratory spectra of blackbody sources. Lacking are the inflight spectra of reference targets including the wavelength calibration spectra. The IRS data are arranged as a single set of 512 spectra calibration spectra, followed by 122 Mariner 6 spectra, followed by 354 Mariner 7 spectra. The latter set is larger because the long-wavelength channel detector system failed on Mariner 6. These spectra are presented here in raw form, as originally supplied to the NSSDC on microfiche. Note that the geometry information in the spectrum headers was revised by the producer in 1984 to account for the revision in the location of the Mars pole following Mariner 9 observations.

NEW HORIZONS LORRI JUPITER ENCOUNTER CALIBRATED V2.0

This data set contains Calibrated data taken by the New Horizons Long Range Reconnaissance Imager instrument during the Jupiter encounter mission phase. This is VERSION 2.0 of this data set.

LRO MOON MINI-RF 5 MAP-PROJECTED CALIBRATED DATA REC V1.0

This data set contains archival map-projected calibrated data acquired from the Mini-RF instrument during the LRO mission and associated ancillary data.

CASSINI SS/S RPWS CALIBRATED LP POTENTIAL CURRENT V1.0

The Cassini Radio and Plasma Wave Science (RPWS) Langmuir Probe Sweep voltage-current data set comprises calibrated Voltage-Current (U-I) characteristics acquired almost continuously from most mission phases during the entire Cassini mission. The full data set of Voltage-Current characteristics is intended to become the most comprehensive and complete data set from which thermal plasma parameters can be derived in the Cassini RPWS archive. Data are presented in text tables and are organised so as to have fixed-length records for ease in data handling. These can be used to derive higher level data products like thermal plasma parameters, e.g., electron density and temperature.

EPOXI MARS OBS - HRIV CALIBRATED IMAGES V2.0

This data set contains calibrated narrow band filter images (350-950 nm) images of Mars acquired by the Deep Impact High Resolution Visible CCD (HRIV) for the EPOCh project during the second cruise phase of the EPOXI mission. One set of observations was acquired on 20-21 November 2009 to characterize Mars as an analog for extrasolar planets. The observing period lasted approximately 24 hours. HRIV images were acquired once per hour with the filters centered on 350, 750 and 950 nm, whereas the 450-, 550-, 650-, and 850-nm data were taken every 15 minutes. Version 2.0 includes the application of a horizontal destriping process and revised electronic crosstalk calibration files.

DAWN GRAND CALIBRATED MARS FLYBY COUNTS V1.0

The GRaND RDR are a time-ordered collection of corrected gamma ray and neutron counting data and calibrated pulse height spectra acquired by GRaND during all phases of the Dawn mission. This data set is specific to Mars Gravity Assist (MGA), and includes data acquired during Mars approach and flyby. The RDR is a calibrated data set derived from the Experiment Data Records (EDR), consisting of time-series counting rates from which elemental abundances can be determined. Ancillary ephemeris and pointing data needed for analysis and mapping of the time series data are included in the data set.