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

Valleys in Alba Patera: ESP_026102_2260 ESP_026181_2260 (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
45.62	251.	1.83	25.09	41.0	38.8
Crater with Viscous Flows and a Channel: ESP_025970_2235 ESP_025904_2235 (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
42.90	257.	-8.9	7.02	41.4	40.1
Light-Toned Material along Coprates Chasma Wallrock and Plateau: ESP_025929_1645 ESP_026430_1645 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.5	303.	-6.5	17.74	60.0	61.1
Dark Slope Streak Extending to Channel Floor: ESP_026064_2045 ESP_026697_2045 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.17	212.	0	-15.4	41.0	44.0
Small Fresh Crater on Northern Plains: ESP_026076_2320 ESP_026419_2320 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
51.66	236.	24.6	-3.11	40.7	42.9
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
Newton Crater Valleys and Alluvial Fans: ESP_026012_1410 ESP_026078_1410 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.7	199.	4.09	-15.0	76.7	78.1
Eastern Rim of Well-Preserved 15-Kilometer Crater Near Alba Mons: ESP_026142_2195 ESP_025852_2195 (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
39.10	238.	17.9	-3.88	38.6	40.4
Interior Deposits of Pangboche Crater: ESP_026024_1975 ESP_026169_1975 (Interval in Earth days: 11)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.25	226.	-13.	1.589	43.7	43.1
Well-Preserved Impact Crater on Floor of Coprates Chasma: ESP_025982_1675 ESP_025626_1675 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.3	294.	14.8	0	56.9	55.1
	Page 595 of 896 (8,955 images)