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The Solar Energetic Particle (SEP) instrument is part of the Particles and Fields (P & F) Package and determines the impact of SEPs on the upper atmosphere.
Solar Energetic Particle Instrument for MAVEN Spacecraft
The Suprathermal and Thermal Ion Composition (STATIC) instrument is part of the Particles and Fields (P & F) Package and measures thermal ions to moderate energy escaping ions.
Suprathermal And Thermal Ion Composition Instrument for MAVEN Spacecraft
The Langmuir Probe and Waves (LPW) instrument is part of the Particles and Fields (P & F) Package and determines ionospheric properties and wave heating of escaping ions and solar EUV input to the atmosphere.
Langmuir Probe And Waves Instrument for MAVEN Spacecraft
A towering dust devil, casts a serpentine shadow over the Martian surface in this image acquired by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.
The Serpent Dust Devil of Mars
The MAVEN spacecraft core structure is successfully lowered and mated to the hydrazine propulsion tank and boat tail assembly at Lockheed Martin, Denver.
MAVEN Stucture Tank Integration
The Thermal Emission Imaging System (THEMIS) camera on NASA's Mars Odyssey spacecraft has completed an unprecedented full decade of observing Mars from orbit.
Tenth Anniversary Image from Camera on NASA Mars Orbiter
The MAVEN spacecraft structure is placed into a reaction chamber, where it completed a static loads test to ensure that it will withstand the extreme forces of launch.
MAVEN Spacecraft in Reaction Structure
A NASA Mars Science Laboratory test rover called the Vehicle System Test Bed, or VSTB, serves as the closest double for Curiosity in evaluations of the mission's hardware and software.
Testing Precision of Movement of Curiosity's Robotic Arm
This self-portait from NASA's Mars Exploration Rover Opportunity shows dust accumulation on the rover's solar panels as the mission approached its fifth Martian winter.
Dusty Mars Rover's Self Portrait
This image, taken Jan. 26, 2012, shows NASA's no-longer-active Phoenix Mars Lander spacecraft after its second Martian arctic winter.
Phoenix Lander After Second Martian Winter
The Mars Hand Lens Imager (MAHLI) camera at the end of the robotic arm of NASA's Curiosity rover will use a calibration target attached to a shoulder joint of the arm.
Calibration Target on Curiosity for Camera on Rover's Arm
This image, taken Jan. 26, 2012, shows the back shell of NASA's Phoenix Mars Lander spacecraft after its second Martian arctic winter.
Phoenix Back Shell After Second Martian Winter
Near the lower left corner of this view is the three-petal lander platform that NASA's Mars Exploration Rover Spirit drove off in January 2004.
Spirit Lander and Bonneville Crater in Color
During pre-flight testing in March 2011, the Mars Hand Lens Imager (MAHLI) camera on NASA's Mars rover Curiosity took this image of the MAHLI calibration target under illumination from MAHLI's two ultraviolet LEDs (light emitting diodes).
MAHLI Calibration Target in Ultraviolet Light
During pre-flight testing, the Mars Hand Lens Imager (MAHLI) camera on NASA's Mars rover Curiosity took this image of the MAHLI calibration target from a distance of 3.94 inches (10 centimeters) away from the target.
Calibration Target as Seen by Mars Hand Lens Imager
This image provides a way to have a full-size printout of the calibration target for the Mars Hand Lens Imager (MAHLI) camera on NASA's Mars rover Curiosity.
Full-Scale Image of MAHLI Calibration Target
The Lincoln penny in this photograph is part of a camera calibration target attached to NASA's Mars rover Curiosity, which is on track for a landing on Mars the night of Aug. 5 to Aug. 6, 2012.
Lincoln Cent on Mars Rover
Two instruments at the end of the robotic arm on NASA's Mars rover Curiosity will use calibration targets attached to a shoulder joint of the arm.
Contact Instrument Calibration Targets on Mars Rover Curiosity
This enhanced-color image shows sand dunes trapped in an impact crater in Noachis Terra, Mars.
Dunes in Noachis Terra Region of Mars
Echus Chasma forms the boundary between the Tharsis volcanoes to the west and Lunae Planum to the east. This region is one of both tectonically fractured rocks (top of image) and volcanic flows (middle and bottom of image). Echus Chasma empties into Kasei Valles.
Echus Chasma
Two spacecraft engineers join a grouping of vehicles providing a comparison of three generations of Mars rovers developed at NASA's Jet Propulsion Laboratory, Pasadena, Calif. The setting is JPL's Mars Yard testing area.
Three Generations of Rovers with Crouching Engineers
Two spacecraft engineers stand with a group of vehicles providing a comparison of three generations of Mars rovers developed at NASA's Jet Propulsion Laboratory, Pasadena, Calif. The setting is JPL's Mars Yard testing area.
Three Generations of Rovers with Standing Engineers
This grouping of two test rovers and a flight spare provides a graphic comparison of three generations of Mars rovers developed at NASA's Jet Propulsion Laboratory, Pasadena, Calif. The setting is JPL's Mars Yard testing area.
Three Generations of Rovers in Mars Yard
This grouping of two test rovers and a flight spare provides a graphic comparison of three generations of Mars rovers developed at NASA's Jet Propulsion Laboratory, Pasadena, Calif. The setting is JPL's Mars Yard testing area.
Three Generations in Mars Yard, High Viewpoint
Western flank of Elysium Mons.
Elysium Mons
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