diff --git a/Instrument/AMDA/Voyager1/CRS.xml b/Instrument/AMDA/Voyager1/CRS.xml
index be86ece..339768c 100644
--- a/Instrument/AMDA/Voyager1/CRS.xml
+++ b/Instrument/AMDA/Voyager1/CRS.xml
@@ -5,7 +5,7 @@
spase://CDPP/Instrument/AMDA/Voyager1/CRS
CRS
-
+ Cosmic Ray System
2009-05-20T21:10:13Z
A
diff --git a/Instrument/AMDA/Voyager1/LECP.xml b/Instrument/AMDA/Voyager1/LECP.xml
index a4345b3..a3149f5 100644
--- a/Instrument/AMDA/Voyager1/LECP.xml
+++ b/Instrument/AMDA/Voyager1/LECP.xml
@@ -5,7 +5,7 @@
spase://CDPP/Instrument/AMDA/Voyager1/LECP
LECP
-
+ Low-Energy Charged Particles
2009-05-20T21:10:13Z
A
diff --git a/Instrument/AMDA/Voyager1/MAG.xml b/Instrument/AMDA/Voyager1/MAG.xml
index 5def65d..8ee7f3c 100644
--- a/Instrument/AMDA/Voyager1/MAG.xml
+++ b/Instrument/AMDA/Voyager1/MAG.xml
@@ -4,8 +4,8 @@
spase://CDPP/Instrument/AMDA/Voyager1/MAG
- Triaxial Fluxgate Magnetometer (MAG)
- MAG
+ MAG
+ Triaxial Fluxgate Magnetometer
2009-05-20T21:10:03Z
This experiment was designed to investigate the magnetic fields of Jupiter and Saturn, the solar-wind interaction with the magnetospheres of these planets, and the interplanetary magnetic field out to the solar wind boundary with the interstellar magnetic field and beyond, if crossed. The investigation was carried out using two high-field and two low-field triaxial fluxgate magnetometers. Data accuracy of the interplanetary fields was plus or minus 0.1 nT, and the range of measurements was from 0.01 nT to 2.E-3 T.
diff --git a/Instrument/AMDA/Voyager1/PLS.xml b/Instrument/AMDA/Voyager1/PLS.xml
index 5c2391e..e1962e1 100644
--- a/Instrument/AMDA/Voyager1/PLS.xml
+++ b/Instrument/AMDA/Voyager1/PLS.xml
@@ -4,8 +4,8 @@
spase://CDPP/Instrument/AMDA/Voyager1/PLS
- Plasma Spectrometer (PLS)
- PLS
+ PLS
+ Plasma Spectrometer
2009-05-20T21:10:02Z
The plasma investigation made use of two Faraday-cup detectors, one pointed along the earth-spacecraft line and one at right angles to this line. The earth-pointing detector determined the macroscopic properties of the plasma ions, obtaining accurate values of their velocity, density, and pressure. Three sequential energy scans were employed with (delta E)/E equal to 20, 7.2, and 1.8%, allowing a coverage from subsonic to highly supersonic flow. The side-looking Faraday cup measured electrons in the energy range from 5 eV to 1 keV.
diff --git a/Instrument/AMDA/Voyager2/CRS.xml b/Instrument/AMDA/Voyager2/CRS.xml
index e59e221..c35ee15 100644
--- a/Instrument/AMDA/Voyager2/CRS.xml
+++ b/Instrument/AMDA/Voyager2/CRS.xml
@@ -4,8 +4,8 @@
spase://CDPP/Instrument/AMDA/Voyager2/CRS
- Cosmic Ray System (CRS)
- CRS
+ CRS
+ Cosmic Ray System
2009-05-20T21:10:14Z
This investigation studied the origin and acceleration process, life history, and dynamic contribution of interstellar cosmic rays, the nucleosynthesis of elements in cosmic-ray sources, the behavior of cosmic rays in the interplanetary medium, and the trapped planetary energetic particle environment. The instrumentation included a High-Energy Telescope System (HETS) and a Low-Energy Telescope System (LETS). The HETS covered an energy range between 6 and 500 MeV/nucleon for nuclei ranging in atomic numbers from 1 through 30. In addition, electrons in the energy range between 3 and 100 MeV were measured by this telescope and an electron telescope. The LETS measured the energy and determined the identity of nuclei for energies between .15 and 30 MeV/nucleon and atomic numbers from 1 to 30. The instruments also measured the anisotropies of electrons and nuclei. In addition, electrons in the energy range between 3 and 100 MeV were measured by the electron telescope.
diff --git a/Instrument/AMDA/Voyager2/LECP.xml b/Instrument/AMDA/Voyager2/LECP.xml
index 58ea254..18fb180 100644
--- a/Instrument/AMDA/Voyager2/LECP.xml
+++ b/Instrument/AMDA/Voyager2/LECP.xml
@@ -4,8 +4,8 @@
spase://CDPP/Instrument/AMDA/Voyager2/LECP
- Low-Energy Charged Particles (LECP)
- LECP
+ LECP
+ Low-Energy Charged Particles
2009-05-20T21:10:14Z
This experiment was designed to study energetic particles in both planetary and interplanetary environments. In the planetary mode, particle sensing occurred with six different solid-state, totally depleted, surface-barrier type detectors. Both coincidence and singles count data were available from two of the detectors. By looking out at a shallow angle from behind the sun shield, measurements were made in regions where particle fluxes were so high as to saturate low-energy detectors. A current mode option was also available for high flux environments. In the interplanetary mode the experiment was equipped with a particle telescope which had solid-state detectors ranging from 2 - 2450 micrometers in thickness. The telescope consisted of two multi-dE/dx x E systems placed back to back in order to use a common all solid-state active anticoincidence shield. The telescope allowed the identification of protons, alpha particles, and heavier nuclei (Z from 3 to 26) in the range from 0.05 to 30 MeV. The combined dynamic range of all the instruments extended from approximately 1.E-5 to greater than 1.E12 particles/(sq cm-s-sr). The energy range covered extended from approximately 10 keV to greater than 11 MeV for electrons and from approximately 15 keV to greater than or equal to 150 MeV for protons and heavier ions. A stepping motor rotated the array of detectors through eight discrete sectors in 45-deg increments, thus allowing a 360-deg scan. For a description of the experiment see Space Science Reviews, 1977, v. 21, pp. 329-354.
diff --git a/Instrument/AMDA/Voyager2/MAG.xml b/Instrument/AMDA/Voyager2/MAG.xml
index 1c06b1d..9398734 100644
--- a/Instrument/AMDA/Voyager2/MAG.xml
+++ b/Instrument/AMDA/Voyager2/MAG.xml
@@ -4,8 +4,8 @@
spase://CDPP/Instrument/AMDA/Voyager2/MAG
- Triaxial Fluxgate Magnetometer (MAG)
- MAG
+ MAG
+ Triaxial Fluxgate Magnetometer
2009-05-20T21:10:14Z
This experiment was designed to investigate (1) the magnetic fields of Jupiter, Saturn, Uranus, and Neptune and (2) the solar-wind interaction of the magnetospheres of these planets with the interplanetary magnetic field out to the solar-wind boundary with the interstellar magnetic field, and beyond, if crossed. The investigation was carried out using two high-field and two low-field triaxial fluxgate magnetometers. Data accuracy of the interplanetary fields was plus or minus 0.1 nT, and the range of measurements was from 0.01 nT to 2.E-3 T.
diff --git a/Instrument/AMDA/Voyager2/PLS.xml b/Instrument/AMDA/Voyager2/PLS.xml
index 2bf6939..01ee4b5 100644
--- a/Instrument/AMDA/Voyager2/PLS.xml
+++ b/Instrument/AMDA/Voyager2/PLS.xml
@@ -4,8 +4,8 @@
spase://CDPP/Instrument/AMDA/Voyager2/PLS
- Plasma Spectrometer (PLS)
- PLS
+ PLS
+ Plasma Spectrometer
2009-05-20T21:10:14Z
The plasma investigation made use of two Faraday-cup detectors, one pointed along the earth-spacecraft line and one at right angles to this line. The earth-pointing detector determined the macroscopic properties of the plasma ions, obtaining accurate values of their velocity, density, and pressure. Three sequential energy scans were employed with (delta E)/E equal to 29, 7.2, and 1.8%, allowing a coverage from subsonic to highly supersonic flow. The side-looking Faraday cup measured electrons in the energy range from 5 eV to 1 keV.
diff --git a/Instrument/AMDA/Voyager2/PWS.xml b/Instrument/AMDA/Voyager2/PWS.xml
index 406dc60..6b539f0 100644
--- a/Instrument/AMDA/Voyager2/PWS.xml
+++ b/Instrument/AMDA/Voyager2/PWS.xml
@@ -4,8 +4,8 @@
spase://CDPP/Instrument/AMDA/Voyager2/PWS
- Plasma Wave System (PWS)
- PWS
+ PWS
+ Plasma Wave System
2009-05-20T21:10:14Z
This investigation provided continuous, sheath-independent measurements of the electron density profiles at Jupiter and Saturn and will provide similar measurements for Uranus and Neptune. It also gave basic information on local wave-particle interactions required to carry out comparative studies of the physics of the magnetospheres of these planets. The instrumentation consisted of a 16-channel step frequency receiver and a low-frequency waveform receiver with associated electronics. The frequency range for this instrument was from 10 Hz to 56 kHz. This instrument shared the 10-m antennas developed for the planetary radio astronomy investigation.
diff --git a/NumericalData/AMDA/Galileo/ephemeris/gll-orb-ca.xml b/NumericalData/AMDA/Galileo/ephemeris/gll-orb-ca.xml
index e54ca09..4c7cb93 100644
--- a/NumericalData/AMDA/Galileo/ephemeris/gll-orb-ca.xml
+++ b/NumericalData/AMDA/Galileo/ephemeris/gll-orb-ca.xml
@@ -4,7 +4,7 @@
spase://CDPP/NumericalData/AMDA/Galileo/ephemeris/gll-orb-ca
- Callisto Flybys
+ flybys callisto
2015-10-07T14:35:00.000Z
Trajectory of Galileo during Callisto flybys. Obtained from NASA/PDS MAG dataset.
Available coordinate systems:
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