Find research datasets worth reusing

ESO NTT IRSPEC IMAGE DATA FROM SL9 IMPACTS WITH JUPITER V1.0

At the ESO La Silla site is a direct imaging facility (DIFA) at the A Nasmyth focus of the NTT, in front of the image derotator which feeds the IRSPEC infrared spectrograph. Two remotely-controlled 45-degree mirrors can be inserted in the light beam to deviate the telescope beam either to a CCD camera (SUSI) or to an infrared array.

VOYAGER 1 JUPITER MAGNETOMETER RESAMPLED DATA 48.0 SEC

This data set includes Voyager 1 Jupiter encounter magnetometer data that have been resampled at a 48.0 second sample rate. The data set is composed of 6 columns: 1) ctime - this column contains the data acquisition time. The time is always output in the ISO standard spacecraft event time format (yyyy-mm-dd-Thh:mm:ss.sss) but is stored internally in Cline time which is measured in seconds after 00:00:00.000 Jan 01, 1966, 2) br - this column contains the radial component of the magnetic field, 3) bphi - this column contains the phi component of the magnetic field, 4) btheta - this column contains the theta component of the magnetic field, 5) bmag - this column contains the magnitude of the magnetic field, 6) flag - a flag value that indicates either software error or spacecraft hardware interference reduced confidence in this record (flag value of 1 is bad , 0 is good or unchecked). All magnetic field observations are measured in nanoTeslas. The coordinate system for this dataset is Minus System III. All of the magnetic field data are calibrated (see the instrument calibration description for more details). The Jupiter System III coordinate system is defined in Dessler 1983 and the reference documents for this dataset are: Ness et al, 1979 Lepping et al, 1981 Connerney,Acuna,Ness, 1981 Behannon,Burlaga,Ness, 1981

NEW HORIZONS SWAP JUPITER ENCOUNTER V1.0

This data set contains Calibrated data taken by the New Horizons Solar Wind Around Pluto instrument during the Jupiter encounter mission phase.

NEW HORIZONS SWAP JUPITER ENCOUNTER CALIBRATED V4.0

This data set contains Calibrated data taken by the New Horizons Solar Wind Around Pluto instrument during the Jupiter encounter mission phase. This is VERSION 4.0 of this data set. During the Jupiter mission phase, SWAP made near-continuous science observations, taking data between 2 and 12 times per hour. Inbound to Jupiter, real-time science mode data were taken twice per hour, then 12 measurements were recorded per hour in the Jupiter tail. The Jupiter tail observations continue until about 100 days after closest approach, which corresponds to about 2200 RJ downstream. The changes in Version 4.0 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. No new observations were added with Version 4.0.

GALILEO ORBITER AT JUPITER CALIBRATED MAG HIGH RES V1.0

This data set contains high time resolution magnetic field vectors acquired by the Galileo magnetometer (MAG). It includes both satellite flyby and non-flyby data. These data were acquired in order to characterize various portions of the Jovian magnetosphere at high time resolution. The Galileo Magnetospheres Working Group (MWG) collectively acquired high time resolution data for short intervals in order to try and regain some of the magnetospheric science lost due to the low data rates of the phase 2 mission (no high gain antenna) mission. These observations are scattered in Jovian distance, local time, System III longitude, etc. in order to provide some insight into processes that may be active in different regions of the magnetosphere.

NEW HORIZONS SDC JUPITER ENCOUNTER V2.0

This data set contains Calibrated data taken by the New Horizons Student Dust Counter instrument during the Jupiter encounter mission phase.

IUE LWP DATA OF COMET SL9/JUPITER/IMPACT SITES

This data set consists of: (a) Raw Image Data and Label Parameters - each raw image consists of an array of 8-bit picture elements or 'pixels'; (b) Associated with each raw image is a set of 20 header, or label records; (c) Raw images must be corrected for the instrumental effects of the SEC.

P10 JUPITER HVM B-FIELD INSIDE 7 RJ JG COORDS 1 MIN AVG V1.0

Pioneer 10 Vector Helium Magnetometer (HVM) data from the Jupiter encounter period between 1973-12-03T21:50 and 1973-12-04T07:54.

MSSSO CASPIR STAR CALS BEFORE SL9 IMPACTS WITH JUPITER V1.0

This archive contains star images used as calibrations in preparation for the collision of Comet Shoemaker-Levy 9 with Jupiter obtained with CASPIR on the Australian National University 2.3 m telescope at Siding Spring Observatory, Australia, by Peter J. McGregor and Mark G. Allen. Each subdirectory contains data for one night. A more specific description of the state of the data is given below.

NEW HORIZONS LEISA JUPITER ENCOUNTER V1.1

This data set contains Calibrated data taken by the New Horizons Linear Etalon Imaging Spectral Array instrument during the Jupiter encounter mission phase.

VOYAGER 1 JUPITER PLASMA DERIVED ION MOMENTS 96 SEC

THIS DATA SET CONTAINS THE BEST ESTIMATES OF THE TOTAL ION DENSITY AT JUPITER DURING THE VOYAGER 1 ENCOUNTER IN THE PLS VOLTAGE RANGE (10-5950 EV/Q). IT IS CALCULATED USING THE METHOD OF MCNUTT ET AL. (1981) WHICH TO FIRST ORDER CONSISTS OF TAKING THE TOTAL MEASURED CURRENT AND DIVIDING BY THE COLLECTOR AREA AND PLASMA BULK VELOCITY. THIS METHOD IS ONLY ACCURATE FOR HIGH MACH NUMBER FLOWS DIRECTLY INTO THE DETECTOR, AND MAY RESULT IN UNDERESTIMATES OF THE TOTAL DENSITY OF A FACTOR OF 2 IN THE OUTER MAGNETOSPHERE. THUS ABSOLUTE DENSITIES SHOULD BE TREATED WITH CAUTION, BUT DENSITY VARIATIONS IN THE DATA SET CAN BE TRUSTED. THE LOW RESOLUTION MODE DENSITY IS USED BEFORE 1979 63 1300, AFTER THIS THE LARGER OF THE HIGH AND LOW RESOLUTION MODE DENSITIES IN A 96 SEC PERIOD IS USED SINCE THE L-MODE SPECTRA OFTEN ARE SATURATED. COROTATION IS ASSUMED INSIDE L=17.5, AND A CONSTANT VELOCITY COMPONENT OF 200 KM/S INTO THE D CUP IS USED OUTSIDE OF THIS. THESE ARE THE DENSITIES GIVEN IN THE MCNUTT ET AL. (1981) PAPER CORRECTED BY A FACTOR OF 1.209 (.9617) FOR DENSITIES OBTAINED FROM THE SIDE (MAIN) SENSOR. THIS CORRECTION IS DUE TO A BETTER CALCULATION OF THE EFFECTIVE AREA OF THE SENSORS. DATA FORMAT: COLUMNS 1-6 ARE TIME (YEAR, DAY, HOUR, MIN, SEC, MSEC) COLUMN 7 IS THE MOMENT DENSITY IN CM-3. EACH ROW HAS FORMAT (6I4, E12.3). VALUES OF 1.E32 INDICATE THAT THE PARAMETER COULD NOT BE OBTAINED FROM THE DATA USING THE STANDARD ANALYSIS TECHNIQUE. ADDITIONAL INFORMATION ABOUT THIS DATASET AND THE INSTRUMENT WHICH PRODUCED IT CAN BE FOUND ELSEWHERE IN THIS CATALOG. AN OVERVIEW OF THE DATA IN THIS DATA SET CAN BE FOUND IN MCNUTT ET AL. (1981) AND A COMPLETE INSTRUMENT DESCRIPTION CAN BE FOUND IN BRIDGE (1977).

Voyager 1 Jupiter Ephemeris Heliographic Coordinates Bundle

This bundle consists of Voyager 1 Jupiter encounter ephemeris data in Heliographic coordinates. Two versions, both covering the same time period, but containing slightly different data, are provided. One version was generated by the Voyager MAG team from Voyager 1 SEDR, the other by the PDS/PPI node using the VG1_JUP.BSP and PCK00003.TPC SPICE kernels.

VOYAGER 2 JUPITER POSITION RESAMPLED DATA 48.0 SECONDS

This data set includes Voyager 2 Jupiter encounter position data that have been generated at a 48.0 second sample rate using the NAIF SPICE kernals. The data set is composed of 4 columns: 1) ctime - this column contains the data acquisition time. The time is always output in the ISO standard spacecraft event time format (yyyy-mm-dd-Thh:mm:ss.sss) but is stored internally in Cline time which is measured in seconds after 00:00:00.000 Jan 01, 1966, 2) r - this column contains the radial distance from Jupiter in Rj = 71398 km, 3) longitude - this column contains the east longitude of the spacecraft in degrees, 4) latitude - this column contains the latitude of the spacecraft in degrees. Position data is given in Minus System III coordinates.

NEW HORIZONS REX JUPITER ENCOUNTER RAW V2.0

This data set contains Raw data taken by the New Horizons Radio Science Experiment instrument during the Jupiter encounter mission phase. This is VERSION 2.0 of this data set. The REX datasets over the mission include calibrations using known radio sources, Jupiter, and cold sky measurements; operational readiness tests (ORTs); internal test pattern calibration; and prime science radiometry and occultation observations during the Pluto Encounter.

VG1 LECP 0.4S HIGH RESOLUTION JUPITER FAR ENCOUNTER DATA

This far encounter data set consists of electron and ion counting rate data from the Low Energy Charged Particle (LECP) experiment on Voyager 1 while the spacecraft was within the vicinity of Jupiter. This instrument measures the intensities of in-situ charged particles ( >15 keV electrons and >30 keV ions) with various levels of discrimination based on energy range and mass species. A subset of almost 100 LECP channels are included in this data set. The LECP data are globally calibrated to the extent possible. Particles include electrons, protons, alpha particles, and light, medium, and heavy nuclei particles.

P11 JUPITER CRT ELECTRON/PROTON/ION FLUX 15 MIN AVGS V1.0

Pioneer 11 Cosmic-Ray Telescope (CRT) data from the Jupiter encounter period from 1974-11-26 and 1974-12-09. The data set provides 15.0 minute flux averages from 18 electron, proton, and heavy ion channels.

ULYSSES JUPITER EPAC OMNI-DIRECTIONAL PROTON FLUX 1 HR AVG

This data set contains Ulysses Energetic Particle Composition Experiment (EPAC) 1 hour averaged omni-directional proton flux data from the Ulysses Jupiter encounter 1992-Jan-25 to 1992-Feb-28. These data were recorded by Omni-directional Protons Spin Averages Telescopes (OPTL) 1-4.

restrictednotspecifiedApr 2025View details →

Voyager 1 Plasma Spectrometer (PLS) VIPER-Fit Plasma Ion Composition near Jupiter, 96 s Data

These Data are from a Re-Analysis of the Voyager Plasma Spectrometer, PLS, Data at Jupiter by the PLS Group at the Laboratory for Atmospheric and Space Physics, LASP, at the University of Colorado. Density, Temperature, and Flow Velocity Fits for total and individual Ions were done using the Voyager Ion PLS Experiment Response, VIPER, Code and Error Analysis as described at http://lasp.colorado.edu/home.mop/missions/voyager/viper/. Fits are determined from processing of the Ion Currents from the A, B, C, and D Cups of the Instrument. As per the Fit Case Variable, one of five different Constraints were used in the VIPER Fits for each 96 s Time Interval: (1) Free Variation of all Parameters (mainly for the cold Ion Torus), (2) Constraint of the Ion Abundances for the five major Species (O+, O++, S+, S++, S+++) to standard Composition as determined from Delamere et al., (2005), (3) fixed Ion Composition and Flow Speed, (4) Cold Blobs in the Plasmasheet where resolved Peaks can be Fit with allowance for some Variance in Composition, (5) Interpolation between Composition of Cold Torus and standard Abundances at 6 RJ from Delamere et al., (2005). Reference: Delamere, P.A., Bagenal, F., and Steffl, A. (2005), Radial Variations in the Io Plasma Torus During the Cassini Era, J. of Geophys. Res., Space Phys., 110(A12), A12223, doi:10.1029/2005JA011251.

ULYSSES JUPITER EPAC PROTON SPECTRAL TELSCP1 DATA 1 HR V1.0

This data set contains Ulysses Energetic Particle Composition Experiment (EPAC) 1 hour averaged sectored proton flux data from the Ulysses Jupiter encounter 1992-Jan-25 to 1992-Feb-28. These data were recorded by Proton Spectral Telescope 1 (PSTL1).

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.