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

Channels or Flow Features with Inverted Topography on Arsia Mons: PSP_005915_1720 ESP_011690_1720 (Interval in Earth days: 450)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.81	242.	-5.1	8.736	33.9	56.6
Light-Toned Outcrops in Noctis Labyrinthus: PSP_006692_1740 ESP_024427_1740 (Interval in Earth days: 1382)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.99	267.	1.10	14.97	39.0	37.4
Gullies in Palikir Crater: PSP_005943_1380 ESP_011428_1380 (Interval in Earth days: 427)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-41.5	202.	3.28	-12.4	45.9	67.3
Fresh 6-Kilometer Diameter Crater Near Galaxias Mensae: PSP_005971_2160 ESP_011456_2160 (Interval in Earth days: 428)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
35.88	147.	1.17	-12.5	52.6	65.4
Possible Pingo at the Border Between Fretted Crater Ejecta: PSP_006632_2240 PSP_010337_2240 (Interval in Earth days: 288)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
43.79	98.7	1.07	-21.5	50.4	53.6
Exposure of High-Latitude Polar Layered Deposits Not Well Observed: PSP_005735_0890 PSP_005721_0910 (Interval in Earth days: 1)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-88.7	218.	18.7	19.02	79.2	78.6
Hale Crater Rim Complex with Gullies of Both Sides: PSP_006545_1435 PSP_007112_1435 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.9	324.	0	-12.5	52.2	62.1
Large Crater on Edge of South Polar Layered Deposits: PSP_005575_0995 PSP_005839_0995 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-80.5	189.	-6.9	-21.1	70.3	75.6
Eridania Scopulus: PSP_006565_1270 ESP_011338_1270 (Interval in Earth days: 372)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-52.7	141.	0	-12.7	64.5	73.4
Impact Flow Features: PSP_005616_1440 ESP_011536_1440 (Interval in Earth days: 461)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.7	129.	-4.5	21.05	38.9	61.4
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