HiRISE | Stereo Pairs

Stereo Pairs

An explanation of stereo pairs and their use (PDF)

In addition to planned stereo pairs, the Pairendipity software can identify all overlapping images suitable for stereo processing. Global lists of such image pairs for the HiRISE and CTX datasets are provided here ordered by latitude. Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column). Stereo images planned within the same 14-day operations cycle are known as SPORCs.

Pairendipity Stereo Pairendipity CTX Stereo SPORCs

Candidate Future Landing Site North of Hellas Basin: ESP_024224_1540 ESP_031872_1540 (Interval in Earth days: 595)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-25.8	54.7	-24.	9.444	47.0	32.1
Remnant of Unconformable Deposit in Electris: ESP_023929_1425 ESP_024074_1425 (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
-37.0	189.	-20.	-5.72	49.1	50.5
MSL Landing Site in Gale Crater: ESP_023957_1755 ESP_024023_1755 (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
-4.55	137.	15.1	-6.86	32.6	34.9
Massif in Reull Vallis: ESP_024051_1365 ESP_024407_1365 (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
-43.2	97.0	7.01	22.35	53.8	59.0
Possible Mud Volcanoes Located in Acidalia Planitia: ESP_024227_2240 ESP_024359_2240 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
43.66	318.	23.1	-2.47	48.5	48.7
Dunes: ESP_024060_1205 ESP_023928_1205 (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
-59.1	218.	-18.	5.39	67.4	63.9
Possible MSL Rover Landing Site in Gale Crater: ESP_024102_1755 ESP_025368_1755 (Interval in Earth days: 99)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.53	137.	29.8	-7.89	32.3	48.7
Pits and Gullies: ESP_024205_1435 ESP_031919_1435 (Interval in Earth days: 601)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.9	214.	-18.	-5.67	52.7	37.0
Prominent Channel Form on Tyrrhena Patera: ESP_024222_1590 ESP_024723_1590 (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
-20.9	107.	-7.9	15.92	43.1	48.9
Valleys on Western Hecates Tholus: ESP_024207_2130 ESP_024352_2130 (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
32.52	149.	-0.4	16.28	43.3	41.0
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