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

Possible Chloride Salt Deposits Observed in THEMIS: PSP_010597_1470 PSP_007380_1470 (Interval in Earth days: 251)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-32.7	205.	18.1	-6.34	69.5	63.4
High-Latitude Exposure of North Polar Layered Deposits: PSP_010808_2720 ESP_028150_2680 (Interval in Earth days: 1351)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
87.93	95.5	-6.3	-11.4	79.4	74.3
Complex Morphology in Acidalia Region: ESP_011384_2185 ESP_011661_2185 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
38.01	310.	7.35	-13.2	63.5	68.9
Very Fresh Small Crater at 48 North Latitude: PSP_010638_2280 ESP_051951_2280 (Interval in Earth days: 3219)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
47.60	157.	2.16	-18.8	56.3	43.7
Section of Wall Rock on the South Rim of Coprates Chasma: PSP_010501_1645 ESP_016026_1645 (Interval in Earth days: 431)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.4	305.	5.32	23.12	62.0	48.0
Mesas with Circumferential Depressions Near Kasei Valles: ESP_011319_2100 ESP_011464_2100 (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
29.64	289.	-20.	-7.41	62.3	62.9
Diverse Hydrated Silicates Near Atlantis Chaos: PSP_010822_1445 ESP_063291_1445 (Interval in Earth days: 4089)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.2	184.	2.16	23.10	70.0	71.3
Light-Toned Layering South of Ius Chasma with Unusual Morphology: PSP_010423_1720 ESP_016726_1720 (Interval in Earth days: 491)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.01	275.	-10.	7.863	60.0	52.5
Possible MSL Landing Site in Holden Crater: ESP_011397_1535 ESP_011898_1535 (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
-26.3	324.	3.35	27.36	61.3	54.6
Central Region of an Impact Crater: PSP_010812_1665 ESP_027730_1665 (Interval in Earth days: 1319)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.2	94.9	0.22	14.92	60.5	59.2
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