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

Wrinkle Ridges in Hesperia Planum: ESP_016455_1535 ESP_016811_1535 (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
-26.2	117.	-5.9	7.118	62.1	65.3
Well-Preserved 30-Kilometer Diameter Impact Crater with Bedrock Exposures: ESP_016760_1585 ESP_017538_1585 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-21.4	70.1	-2.0	-13.5	62.0	67.8
Ejecta of Crater Sectioned by Erosion: ESP_016896_1710 ESP_025678_1710 (Interval in Earth days: 684)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.92	315.	6.04	-5.75	54.6	53.8
Small Rampart Crater Near the Central Peak of Lyot Crater: ESP_016326_2305 ESP_060026_2305 (Interval in Earth days: 3405)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
50.39	29.2	-3.9	16.71	47.2	47.4
Potential Rhythmic Layering in East Gale Crater with Hydrated Signature: ESP_016375_1750 ESP_016520_1750 (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
-5.15	138.	1.01	18.09	48.0	48.2
Melas Fossae: ESP_016541_1520 ESP_019877_1520 (Interval in Earth days: 260)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.5	288.	6.46	28.65	63.3	60.7
Cratered Mounds in Galaxias Colles: ESP_016691_2175 ESP_018260_2175 (Interval in Earth days: 122)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
37.23	146.	0	27.19	41.3	40.5
Aram Chaos Mineralogical Variability: ESP_016605_1830 ESP_086812_1830 (Interval in Earth days: 5470)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.889	339.	-8.3	-23.3	46.9	47.0
Ridges and Fill Material Among Knobs on West Flank of Arsia Mons: ESP_016833_1715 ESP_019035_1715 (Interval in Earth days: 171)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.53	235.	-1.7	13.23	54.3	57.3
Deposit Associated with Channels along Floor of Ganges Chasma: ESP_016817_1710 ESP_017239_1710 (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
-8.69	311.	5.05	-13.5	53.8	57.9
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