10.03.2016 Curiosity Self-Portrait at 'Murray Buttes'
10.03.2016 Butte 'M9a' in 'Murray Buttes' on Mars
09.19.2016 Ribbon Cutting
09.09.2016 Farewell to Murray Buttes (Image 5)
09.09.2016 Farewell to Murray Buttes (Image 4)
09.09.2016 Farewell to Murray Buttes (Image 3)
09.09.2016 Farewell to Murray Buttes (Image 2)
09.09.2016 Farewell to Murray Buttes (Image 1)
08.26.2016 Out-of-this-World Records
03.30.2016 Erisa Hines
03.30.2016 Buzz Aldrin
02.12.2016 Women in Science
02.09.2016 Adam Steltzner, a JPL engineer
01.27.2016 Night Close-up of Martian Sand Grains
01.27.2016 Curiosity Self-Portrait at Martian Sand Dune
12.17.2015 Alteration Effects at Gale and Gusev Craters
12.17.2015 Full-Circle View Near 'Marias Pass' on Mars
12.11.2015 Surface Close-up of a Martian Sand Dune
12.11.2015 Martian Sand Disturbed by Rover Wheel
11.24.2015 Carbon Exchange and Loss Processes on Mars
11.17.2015 Chemical Laptop 1
11.11.2015 Thick, Dark Veins at 'Garden City,' Mars
11.11.2015 Dark, Thin Fracture-Filling Material
10.08.2015 Secrets of 'Hidden Valley' on Mars
10.08.2015 Strata at Base of Mount Sharp
10.02.2015 Mount Sharp Comes In Sharply
Radiation Measurements on MarsThe Radiation Assessment Detector (RAD) instrument on NASA's Curiosity Mars rover monitors the natural radiation environment at the surface of Mars. It can see the radiation from two sources, galactic cosmic rays and solar energetic particles. This graph plots measurements made during the rover's first 10 months on Mars. The vertical axis is in micrograys per day. Micrograys are unit of measurement for absorbed radiation dose. The horizontal axis is time, labelled on the bottom as months from August 2012 to June 2013 and on the top as the number of sols (Martian days) since landing.
The observations have been almost entirely due to galactic cosmic rays, which contribute a slowly varying dose rate of about 210 micrograys per day. Variations are due to day-to-night differences in the shielding provided by the atmosphere. Sudden drops in the radiation, so-called Forbush decreases, such as seen on sols 50, 97, 208 and 259, result from extra shielding provided by interplanetary coronal mass ejections driven by the sun. The longer-term increase and decrease peaking close to Sol 200 is driven by Martian seasonal effects.
Only one solar particle event has been observed by RAD on the surface of Mars, and it was rather weak. Researchers had expected to see more solar particle events, but for unknown reasons, the sun is currently much less active than during recent peaks in the solar-activity cycle. After the RAD measurements during Curiosity's flight to Mars and on the surface of Mars, solar particle events are the big unknowns in predicting the radiation exposure for a human mission to Mars. If the instrument had been taking measurements on Mars during the comparable period of the solar-activity cycle about 11 years ago, it would probably have seen eight events in 300 sols, contributing an unknown but certainly significantly higher amount to the overall dose.
Image Credit: NASA/JPL-Caltech/SwRI