PDS: The Planetary Atmospheres Node
| | Dust | UV Spectra | Abundances | ||
LADEE | Detects individual dust grains with m ≥ 1.7x10-16kg (radius ≥ 0.3 μm) LDEX | Detects K, Na, Al, Si, Ca, Li, OH, H2O UVS | 1-92 AMU detects H2, He, Ne, CH4, OH, H2O, CO, Ar-36, Ar-40, and CO2 NMS | ||
CLPS | PITMS | ||||
ARTEMIS | Artemis is a pair of spacecraft based on repurposed components of the THEMIS mission that utilized spacecraft placed in Earth-Moon L1 and L2 orbits. They carry a suite of instruments to measure the magnetic and electric fields, thermal electrons and ions and energetic particle distribution functions | ||||
Currently the ARTEMIS data is available at the THEMIS web site at Berkeley http://themis.ssl.berkeley.edu/data_products. It will be archived at the PDS Planetary Plasma Interactions Node (PPI) | |||||
APOLLO | Apollo 15 Orbital Mass Spectrometer Apollo 16 Orbital Mass Spectrometer at the PDS Geosciences Node | ||||
Ladee spice files are available at the NAIF Node
