
INSTRUMENTS
TARGETS
QUICK LINKS
![]() | Accelerometer(ACC) Data are available at Atmospheres Density derived from acceleration data and Winds derived from NAV and ACS data |
![]() | Electra Ultra-high frequency Terminal(EUT) No scientific data available |
![]() | Extreme UltraViolet Monitor(EUV) 5 datasets are available at Planetary Plasma Interactions The EUV monitor is designed to measure the solar irradiance in three broad bands in the soft xray and extreme ultraviolet wavelength range. |
![]() | High Gain Antenna(HGA) No scientific data available |
![]() | Imaging UltraViolet Spectrograph(IUVS) Data are available at Atmospheres IUVS is an Imaging UltraViolet Spectrograph Spanning 110-340 nm with two spectral resolution modes with low resolution (λ/Δλ~400) and high resolution (λ/Δλ=13,800) to measure the D/H ratio. |
![]() | LangMuir Probe and Waves(LPW) 6 datasets are available at Planetary Plasma Interactions The LPW instrument measures the electron density (ne) and temperature (Te) of Mars ionosphere and detects waves that can heat ions in resulting in atmospheric loss. |
![]() | Magnetometer(MAG) 3 datasets are available at Planetary Plasma Interactions The MAVEN magnetic field investigation (MAG) consists of two independent and identical fluxgate magnetometer systems that are interfaced to and controlled by the PFDPU. |
![]() | Neutral Gas and Ion Mass Spectrometer (NGIMS) Data are available at Atmospheres NGIMS is a quadrupole mass spectrometer with open and closed sources. The open ion source mode is used to measure reactive neutral gas species and to sample ambient thermal and suprathermal ions while the closed source samples non-reactive neutrals. The mass range is 2 - 150 Da. |
![]() | Radio Occultation Science Experiment(ROSE) 3 datasets are available at Planetary Plasma Interactions The ROSE data is the signal transmitted from the MAVEN to the ground, so the 'instrument' consists of the MAVEN radio transmitter, and HGA (for which we do have an image), and the antennas of the Deep Space Network (DSN) |
![]() | Remote Sensing Data Processing Unit(RSDPU) No scientific data available |
![]() | Solar Energetic Particle(SEP) 3 datasets are available at Planetary Plasma Interactions SEP consists of 2 sensors, each consisting of a pair of double-ended solid-state telescopes, measuring electrons and ions over the energy ranges ~30-1000 keV and ~30-12,000 keV/nuc respectively. |
SPICE Kernels(SPICE) Data are available at NAIF SPICE | |
![]() | Supra-Thermal And Thermal Ion Composition(STATIC) 3 datasets are available at Planetary Plasma Interactions STATIC is designed to measure the ion composition and distribution function of the cold Martian ionosphere, of the heated suprathermal tail of this plasma in the upper ionosphere, and the pickup ions accelerated by solar wind electric fields. |
![]() | Solar Wind Electron Analyzer(SWEA) 3 datasets are available at Planetary Plasma Interactions SWEA is a symmetric, hemispheric electrostatic analyzer designed to measure the energy and angular distributions of solar wind electrons and ionospheric photoelectrons in the Mars environment. |
![]() | Solar Wind Ion Analyzer(SWIA) 3 datasets are available at Planetary Plasma Interactions SWIA is an electrostatic analyzer designed to measure solar wind and magnetospheric ions in the Martian system over an energy/charge range of ~5-25000 eV/q, and an angular range of 360 x 90 degrees [minus spacecraft obstructions] |
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Web Master: PDS-PPI Operator NASA Official: Becky McCauley-Rench |