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

Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor : ESP_029248_1640 ESP_029960_1640 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.9	56.2	-5.9	7.576	55.5	49.4
Apollinaris Patera : ESP_029125_1705 ESP_030193_1705 (Interval in Earth days: 84)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.21	173.	-8.5	7.734	55.5	48.8
Layered Deposits in West Candor Chasma : ESP_029266_1735 ESP_029899_1735 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.34	283.	-4.1	-29.7	54.7	54.6
Sinuous Channel South of Ascraeus Mons : ESP_028911_1815 ESP_029333_1815 (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
1.599	253.	5.38	-8.72	53.8	55.5
Kasei Valles : ESP_028989_1895 ESP_029833_1895 (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
9.563	282.	6.16	-25.0	54.2	59.5
Graben with Many Slope Streaks : ESP_028978_2060 ESP_029400_2060 (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
25.88	221.	7.23	-5.92	56.9	62.3
Classic Spider Terrain : ESP_028932_0935 ESP_028931_0935 (Interval in Earth days: 0)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-86.3	99.1	-1.9	16.46	91.4	89.7
Proposed Future Landing Site in Ladon Valles Basin : ESP_029304_1600 ESP_038442_1600 (Interval in Earth days: 712)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-19.6	327.	-2.2	27.55	55.4	52.7
Easternmost Portion of Valley Connected to East Side of Jezero Crater : ESP_028970_1990 ESP_029036_1990 (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
18.65	78.7	24.4	4.845	53.7	55.9
Arsia Mons Reticulate Bedform Change Detection : ESP_029215_1740 ESP_029360_1740 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.16	235.	5.36	19.71	54.1	52.6
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