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

Pit and Channel on Southwestern Pavonis Mons: PSP_009923_1785 PSP_010213_1785 (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
-1.67	246.	-21.	14.06	58.1	55.7
Distributaries From Athabasca Valles: PSP_009768_1880 PSP_010045_1880 (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
7.721	154.	7.98	-19.7	51.6	54.3
Unnamed Pristine Crater Near Tempe Terra: PSP_009526_2045 PSP_010370_2045 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.31	279.	0.18	-20.5	46.1	52.4
Clay-Bearing Unit in the Western Arabia Region: PSP_009735_1985 PSP_009880_1985 (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
18.19	335.	-7.7	7.217	49.1	48.4
Possible Flute Casts in Ares Vallis: PSP_009722_1960 PSP_009867_1960 (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
15.92	329.	2.51	17.22	48.9	48.1
Small Shield Covering the Noctis Fossae: PSP_010305_1780 PSP_010661_1780 (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
-1.91	256.	-7.0	-0.74	57.3	56.9
High-Latitude Exposure of North Polar Layered Deposits: PSP_010100_2675 PSP_010457_2675 (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
87.29	32.0	-5.8	-15.5	68.3	73.1
Unconformities in North Polar Layered Deposits: PSP_010124_2650 PSP_010242_2650 (Interval in Earth days: 9)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
84.81	128.	-7.7	7.364	67.0	67.7
Tooting Crater Southern Ejecta Layer: PSP_009766_2030 PSP_009832_2030 (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
22.53	207.	2.91	-16.9	47.2	49.2
Fresh 8-Kilometer Diameter Impact Crater: PSP_009625_1900 ESP_016060_1900 (Interval in Earth days: 501)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
9.793	98.5	4.97	-22.4	50.7	41.9
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