Mars radar clutter and surface roughness characteristics from MARSIS data

被引:13
|
作者
Campbell, Bruce A. [1 ]
Schroeder, Dustin M. [2 ]
Whitten, Jennifer L. [1 ]
机构
[1] Smithsonian Inst, Ctr Earth & Planetary Studies, MRC 315,POB 37012, Washington, DC 20560 USA
[2] Stanford Univ, Dept Geophys, 397 Panama Mall, Stanford, CA, Panama
关键词
Radar observations; Mars; surface; Jupiter; satellites; SUBSURFACE; IONOSPHERE; ECHOES; MOON;
D O I
10.1016/j.icarus.2017.07.011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Radar sounder studies of icy, sedimentary, and volcanic settings can be affected by reflections from surface topography surrounding the sensor nadir location. These off-nadir "clutter" returns appear at similar time delays to subsurface echoes and complicate geologic interpretation. Additionally, broadening of the radar echo in delay by surface returns sets a limit on the detectability of subsurface interfaces. We use MARSIS 4MHz data to study variations in the nadir and off-nadir clutter echoes, from about 300 km to 1000 km altitude, R, for a wide range of surface roughness. This analysis uses a new method of characterizing ionospheric attenuation to merge observations over a range of solar zenith angle and date. Mirror-like reflections should scale as R-2, but the observed 4MHz nadir echoes often decline by a somewhat smaller power-law factor because MARSIS on-board processing increases the number of summed pulses with altitude. Prior predictions of the contributions from clutter suggest a steeper decline with R than the nadir echoes, but in very rough areas the ratio of off-nadir returns to nadir echoes shows instead an increase of about R-1/2 with altitude. This is likely due in part to an increase in backscatter from the surface as the radar incidence angle at some round-trip time delay declines with increasing R. It is possible that nadir and clutter echo properties in other planetary sounding observations, including RIME and REASON flyby data for Europa, will vary in the same way with altitude, but there may be differences in the nature and scale of target roughness (e.g., icy versus rocky surfaces). We present global maps of the ionosphere- and altitude-corrected nadir echo strength, and of a "clutter" parameter based on the ratio of off-nadir to nadir echoes. The clutter map offers a view of surface roughness at similar to 75m length scale, bridging the spatial-scale gap between SHARAD roughness estimates and MOLA-derived parameters. Published by Elsevier Inc.
引用
收藏
页码:22 / 30
页数:9
相关论文
共 50 条
  • [21] NeMars: An empirical model of the martian dayside ionosphere based on Mars Express MARSIS data
    Sanchez-Cano, B.
    Radicella, S. M.
    Herraiz, M.
    Witasse, O.
    Rodriguez-Caderot, G.
    ICARUS, 2013, 225 (01) : 236 - 247
  • [22] The Analysis of the Topside Additional Layer of Martian Ionosphere Using MARSIS/Mars Express Data
    Kim, Eojin
    Seo, Haingja
    Kim, Joo Hyeon
    Lee, Joo Hee
    Kim, Yong Ha
    Choi, Gi-Hyuk
    Sim, Eun-Sup
    JOURNAL OF ASTRONOMY AND SPACE SCIENCE, 2012, 29 (04) : 337 - 342
  • [23] Radar Observations of Liquid Water in the South Polar Region of Mars: Indications from Astrobiology Perspectives
    Zhou, Junyi
    Ding, Chunyu
    Xiong, Siting
    Su, Yan
    Li, Jiawei
    Chen, Mengna
    Dai, Shun
    UNIVERSE, 2024, 10 (01)
  • [24] Calibration of Mars Reconnaissance Orbiter Shallow Radar (SHARAD) data for subsurface probing and surface reflectivity studies
    Campbell, Bruce A.
    Morgan, Gareth A.
    Bernardini, Fabrizio
    Putzig, Nathaniel E.
    Nunes, Daniel C.
    Plaut, Jeffrey J.
    ICARUS, 2021, 360
  • [25] Simulation of Martian Near-Surface Structure and Imaging of Future GPR Data From Mars
    Zhang, Ling
    Xu, Yi
    Zeng, Zhaofa
    Li, Jing
    Zhang, Dong
    IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, 2022, 60
  • [26] Total electron content in the Martian atmosphere: A critical assessment of the Mars Express MARSIS data sets
    Sanchez-Cano, B.
    Morgan, D. D.
    Witasse, O.
    Radicella, S. M.
    Herraiz, M.
    Orosei, R.
    Cartacci, M.
    Cicchetti, A.
    Noschese, R.
    Kofman, W.
    Grima, C.
    Mouginot, J.
    Gurnett, D. A.
    Lester, M.
    Blelly, P. -L.
    Opgenoorth, H.
    Quinsac, G.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2015, 120 (03) : 2166 - 2182
  • [27] Surface Clutter Discrimination Analysis for Radar Sounding Interferometry
    Haynes, Mark S.
    Chapin, Elaine
    Moussessian, Alina
    Madsen, Soren N.
    IEEE TRANSACTIONS ON AEROSPACE AND ELECTRONIC SYSTEMS, 2019, 55 (02) : 989 - 1003
  • [28] Characteristics of First Order Sea Clutter for High Frequency Hybrid Sky Surface Wave Radar
    Zhou, Qing
    Zheng, Hong
    Li, Miao
    Zhang, Lan
    PROCEEDINGS OF THE 2020 IEEE INTERNATIONAL CONFERENCE ON COMPUTATIONAL ELECTROMAGNETICS (ICCEM 2020), 2020, : 121 - 123
  • [29] ANALYSIS OF SURFACE CLUTTER FOR SUBSURFACE RADAR SOUNDING ON VENUS
    Thakur, Sanchari
    Paolaz, Elisa Nicolussi
    Sbalchiero, Elisa
    Bruzzone, Lorenzo
    2022 IEEE INTERNATIONAL GEOSCIENCE AND REMOTE SENSING SYMPOSIUM (IGARSS 2022), 2022, : 1340 - 1343
  • [30] Simulation of radar echoes from Mars' surface/subsurface and inversion of surface media parameters
    Liu, Chuan
    Ye, Hongxia
    Jin, Ya-Qiu
    RADIO SCIENCE, 2014, 49 (07) : 473 - 484