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1) AIM/CDE dust grain impact data maxmize
Resource ID:spase://VSPO/NumericalData/AIM/CDE/PT1D
Start:2007-06-01 00:00:00 Observatory:AIM Cadence:
Stop:2016-09-14 08:00:04 Instrument:AIM Cosmic Dust Experiment Resource:NumericalData
AIM/CDE (Cosmic Dust Experiment) data are available as Levels 1 and 2 daily netCDF files. L1 data contains, for each dust grain impact, a time tag, pulse height data, a number of electrons released by the impact, and engineering and housekeeping data. L2 data adds the mass of the impacting particle and spacecraft location at time of impact. Future L3 and L4 products will add total mass impacting per orbit and impact rates (L3) and mass correlation with CIPS total particle mass and Polar Mesospheric Cloud brightness.(

2) Ulysses Dust Detection System Data maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/DUST/PT1M
Start:1990-10-27 18:53:00 Observatory:Ulysses Cadence:1 minute
Stop:1992-12-31 23:18:00 Instrument:Cosmic Dust (GRU/DUST) Resource:NumericalData
This data set contains information collected by the Ulysses Cosmic Dust instrument on the dust environment in interplanetary space within the inner solar system, between Jupiter and the Sun, and at high polar latitudes of the Sun. Both interplanetary and interstellar dust particles have been detected. This information is collected with a dust impact experiment, from which may be inferred direction of motion, mass, velocity and charge (see ULYDINST.CAT). The data presented in this dataset include instrumental readouts, inferred metadata, calibration information and a calendar of events.

3) Ulysses GAS UV Full-Sky Data maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/GAS/Full-Sky/PT24H
Start:1990-10-27 00:00:00 Observatory:Ulysses Cadence:24 hours
Stop:2007-08-18 23:59:59 Instrument:Ulysses Interstellar Neutral Gas (GAS) Experiment Resource:NumericalData
This Ulysses GAS experiment data set consists of pixel map data and image files for sky maps generated from GAS measurements in a mode primarily sensitive to ultraviolet photons. The accumulated counts and Ecliptic (spacecraft-centered) angle coordinates for each sky map pixel are given in the ascii files *.TXT. The positions of the Sun and the planets vary with time and with the position of the spacecraft along its trajectory, while the positions of stars remain fixed. The full images are provided in GIF (*.GIF files) and postscript (*.PS files) format, the GIF files being easily viewed on-line (see below) with an Internet web browser. The actual positions of Sun, Earth, and Jupiter are indicated by yellow, green, and white dots, respectively. The area around the Sun is excluded from observation to avoid damaging intensities from direct sunlight. The files USER_GUIDE.TXT, FORMAT.TXT, and REFERENCE.TXT, respectively, give an overall description of the various datatypes, the record format for the DATA datatype, and a list of GAS-related publications. The users guide defines the nomenclature of the file names.

4) Ulysses GAS Interstellar Helium Maps maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/GAS/Interstellar-Helium/PT24H
Start:1990-10-27 00:00:00 Observatory:Ulysses Cadence:24 hours
Stop:2007-11-25 23:59:59 Instrument:Ulysses Interstellar Neutral Gas (GAS) Experiment Resource:NumericalData
This Ulysses GAS experiment data set consists of pixel map data and image files for sky maps generated from GAS measurements in the mode primarily sensitive to neutral helium atoms from inflow of interstellar gas into the heliosphere. The accumulated counts and Ecliptic (spacecraft-centered) angle coordinates for each sky map pixel are given in the ascii files *.TXT. The positions of the Sun and the planets vary with time and with the position of the spacecraft along its trajectory, while the positions of stars remain fixed. The full images are provided in GIF (*.GIF files) and postscript (*.PS files) format, the GIF files being easily viewed on-line (see below) with an Internet web browser. The actual positions of Sun, Earth, and Jupiter are indicated by yellow, green and white dots, respectively. The area around the Sun is excluded from observation to avoid damaging intensities from direct sunlight. The files USER_GUIDE.TXT, FORMAT.TXT, and REFERENCE.TXT, respectively, give an overall description of the various datatypes, the record format for the DATA datatype, and a list of GAS-related publications. The users guide defines the nomenclature of the file names. Further details about the data and the experiment may be found in Witte et al., Astron. Astrophys. Suppl. Ser., 92, No. 2, 333-348, 1992 (NSSDC TRF # B40459-000A). Data analysis methods for interstellar helium are described in Banaszkiewicz et al., Astron. Astrophys. Suppl. Ser., 120, 587-602, 1996 (B45706-000A).

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