Instituto Nacional de Técnica Aeroespacial INTA, 28850 Torrejon de Ardoz, Spain.
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
Sensors (Basel). 2022 Apr 10;22(8):2907. doi: 10.3390/s22082907.
The Radiation and Dust Sensor is one of six sensors of the Mars Environmental Dynamics Analyzer onboard the Perseverance rover from the Mars 2020 NASA mission. Its primary goal is to characterize the airbone dust in the Mars atmosphere, inferring its concentration, shape and optical properties. Thanks to its geometry, the sensor will be capable of studying dust-lifting processes with a high temporal resolution and high spatial coverage. Thanks to its multiwavelength design, it will characterize the solar spectrum from Mars' surface. The present work describes the sensor design from the scientific and technical requirements, the qualification processes to demonstrate its endurance on Mars' surface, the calibration activities to demonstrate its performance, and its validation campaign in a representative Mars analog. As a result of this process, we obtained a very compact sensor, fully digital, with a mass below 1 kg and exceptional power consumption and data budget features.
辐射和尘埃传感器是美国宇航局“毅力号”火星 2020 任务漫游车上的火星环境动力学分析仪的六个传感器之一。它的主要目标是描述火星大气中的气载尘埃,推断其浓度、形状和光学特性。由于其几何形状,传感器将能够以高时间分辨率和高空间覆盖率研究扬尘过程。由于其多波长设计,它将从火星表面描述太阳光谱。本工作从科学和技术要求、在火星表面展示其耐久性的资格认证过程、展示其性能的校准活动以及在有代表性的火星模拟中进行的验证活动来描述传感器设计。通过这个过程,我们得到了一个非常紧凑的传感器,完全数字化,重量低于 1 公斤,具有出色的功耗和数据预算特性。