scholarly journals Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE)

2007 ◽  
Vol 112 (E5) ◽  
Author(s):  
Alfred S. McEwen ◽  
Eric M. Eliason ◽  
James W. Bergstrom ◽  
Nathan T. Bridges ◽  
Candice J. Hansen ◽  
...  
Keyword(s):  
High Resolution ◽  
High Resolution Imaging ◽  
Imaging Science ◽  
Resolution Imaging

The High Resolution Imaging Science Experiment (HiRISE) during MRO’s Primary Science Phase (PSP)

Icarus ◽  
2010 ◽  
Vol 205 (1) ◽  
pp. 2-37 ◽  
Author(s):  
Alfred S. McEwen ◽  
Maria E. Banks ◽  
Nicole Baugh ◽  
Kris Becker ◽  
Aaron Boyd ◽  
...  
Keyword(s):  
High Resolution ◽  
Primary Science ◽  
High Resolution Imaging ◽  
Imaging Science ◽  
Resolution Imaging

Introduction to the High Resolution Imaging Science Experiment (HiRISE) Special Issue of Icarus

Icarus ◽  
2010 ◽  
Vol 205 (1) ◽  
pp. 1
Author(s):  
Kenneth E. Herkenhoff ◽  
Laszlo P. Keszthelyi ◽  
Alfred S. McEwen
Keyword(s):  
High Resolution ◽  
High Resolution Imaging ◽  
Special Issue ◽  
Imaging Science ◽  
Resolution Imaging

scholarly journals DETECTING THE SOURCES OF ICE BLOCK FALLS AT THE MARTIAN NORTH POLAR SCARPS BY ANALYSIS OF MULTI-TEMPORAL HIRISE IMAGERY

2021 ◽  
Vol XLIII-B3-2021 ◽  
pp. 673-678
Author(s):  
S. Su ◽  
L. Fanara ◽  
X. Zhang ◽  
K. Gwinner ◽  
E. Hauber ◽  
...  
Keyword(s):  
High Resolution ◽  
Change Detection ◽  
Detection Method ◽  
High Resolution Imaging ◽  
Mass Wasting ◽  
Multi Temporal ◽  
Imaging Science ◽  
Resolution Imaging ◽  
North Polar ◽  
Integrated Software

Abstract. We have developed a method for automatically detecting the sources of ice block falls at the Martian north polar scarps. Multitemporal red-filter High Resolution Imaging Science Experiment (HiRISE) images were processed by using the open source NASA Ames Stereo Pipeline in combination with the USGS Integrated Software for Imagers and Spectrometers to produce 0.25 m resolution images as well as a 1 m resolution DTM. The multi-temporal HiRISE images were firstly ortho-rectified by the DTM, and then co-registered by using the Enhanced Correlation Coefficient Maximization (ECC) algorithm. We applied the change detection method on the well-aligned sub-meter scale HiRISE images, which were taken in Mars Year 29 and Mars Year 30, to investigate mass wasting at the scarp area centred at 85.0°N, 151.5°E. The idea of the change detection method is to identify changing shadow patterns based on the grayscale difference between the images. The final results show that erosion events occurred at the full length of this study’s scarp within one Mars Year. However, only the upper and lower part of the scarp show erosion activity, whereas the intermediate parts seem inactive, and this correlates with the slope.

scholarly journals The Temporal Variation of Optical Depth in the Candidate Landing Area of China’s Mars Mission (Tianwen-1)

2021 ◽  
Vol 13 (5) ◽  
pp. 1029
Author(s):  
Zhencheng Tang ◽  
Jianjun Liu ◽  
Xing Wang ◽  
Xin Ren ◽  
Wei Yan ◽  
...  
Keyword(s):  
High Resolution ◽  
Temporal Variation ◽  
Optical Depth ◽  
Seasonal Pattern ◽  
High Resolution Imaging ◽  
Atmospheric Dust ◽  
Mars Mission ◽  
Imaging Camera ◽  
Imaging Science ◽  
Resolution Imaging

The atmospheric dust is an important factor in the evolution of the Martian climate and has a major impact on the scientific exploration of the Martian lander or rover and its payload. This paper used remote sensing images to calculate atmospheric optical depth that characterizes the spatial distribution of the atmospheric dust of Mars. The optical depth calculated by the images of the High Resolution Imaging Science Experiment (HiRISE) in the inspection area of the Spirit rover had a similar temporal variation to the optical depth directly measured by the Spirit rover from the sunlight decay. We also used the HiRISE images to acquire the seasonal variation of optical depths in the candidate landing area of China’s Mars Mission (Tianwen-1). The results have shown that the seasonal pattern of the optical depth in the candidate landing area is consistent with the dust storm sequences in this area. After Tianwen-1 enters the orbit around Mars, the images collected by the Moderate Resolution Imaging Camera (MoRIC), and the High Resolution Imaging Camera (HiRIC) can be used to study the atmospheric optical depth in the candidate landing area, providing reference for the safe landing and operation of the lander and rover.

Color imaging of Mars by the High Resolution Imaging Science Experiment (HiRISE)

Icarus ◽  
2010 ◽  
Vol 205 (1) ◽  
pp. 38-52 ◽  
Author(s):  
W. Alan Delamere ◽  
Livio L. Tornabene ◽  
Alfred S. McEwen ◽  
Kris Becker ◽  
James W. Bergstrom ◽  
...  
Keyword(s):  
High Resolution ◽  
High Resolution Imaging ◽  
Color Imaging ◽  
Imaging Science ◽  
Resolution Imaging
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