HiRISE | Stereo Pairs

Stereo Pairs

An explanation of stereo pairs and their use (PDF)

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Stereo Pair List (csv) Pairendipity Stereo Pairendipity CTX Stereo SPORCs

Recent Crater: ESP_025867_2200 ESP_025788_2200 (Interval in Earth days: 7)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
39.57	185.	24.1	-3.39	38.0	40.5
Pits and Channels in Amazonis Planitia: ESP_025827_2025 ESP_025893_2025 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
22.21	202.	5.00	-14.3	40.3	42.1
A Youthful Crater and Its Ejecta: ESP_026099_2320 ESP_027866_2320 (Interval in Earth days: 137)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
51.63	333.	-1.5	12.84	43.0	49.9
Possible Future Mars Landing Site of 2018 Joint Rover in Trouvelot Crater: ESP_025835_1965 ESP_026125_1965 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.12	347.	-15.	12.93	43.7	42.5
Possibly Fresh 4-Kilometer Diameter Crater: ESP_025901_2460 ESP_026455_2460 (Interval in Earth days: 43)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
65.76	334.	0.65	-20.0	49.7	50.1
Fresh Rayed Crater: ESP_025894_1560 ESP_026316_1560 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.5	179.	6.40	-8.72	64.5	67.8
Rampart Crater Terrain Sample: ESP_026199_2515 ESP_026001_2515 (Interval in Earth days: 15)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
71.43	122.	-18.	0	53.2	52.5
Flow with Wide Leveed Channel: ESP_025998_1760 ESP_027264_1760 (Interval in Earth days: 98)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-3.90	217.	3.13	-22.8	52.5	57.3
Eastern Portion of Well-Preserved 10-Kilometer Impact Crater: ESP_026028_1810 ESP_033597_1810 (Interval in Earth days: 590)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
0.748	116.	20.4	-5.22	48.7	41.3
Flow Boundary in Elysium Planitia: ESP_026105_2085 ESP_026593_2085 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
27.99	172.	3.05	-24.4	40.2	43.8
	Page 574 of 878 (8,772 images)