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

Sedimentary Fan in Crater in Terra Cimmeria: ESP_076652_1445 ESP_077140_1445 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-34.9	161.	-3.9	15.93	46.4	53.0
Inverted Channel and Possible Lake Deposits: ESP_076462_1725 ESP_084242_1725 (Interval in Earth days: 606)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.56	303.	-5.5	29.60	35.8	38.1
Small Candidate Lake Deposit Downstream of Alluvial Fan: ESP_076629_1675 ESP_076972_1675 (Interval in Earth days: 26)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.5	66.0	-6.2	-19.7	37.3	41.7
Dipping Layers in Ejecta: ESP_076391_2160 ESP_075824_2160 (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
35.65	75.9	-6.4	-18.4	55.5	63.9
Layering in Western Arabia Terra: ESP_076447_1900 ESP_075959_1900 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
9.843	351.	-19.	-5.22	40.8	43.7
Youthful Crater in THEMIS V22898007 and at Edge of MOC E11-03928: ESP_076415_1345 ESP_084037_1345 (Interval in Earth days: 594)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-45.2	150.	5.97	-6.29	48.5	41.2
Aeolian Erosion of Medusa Fossae Formation: ESP_076386_1760 ESP_076241_1760 (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
-3.93	214.	25.0	0.959	33.5	35.6
Streamlined Hills in Osuga Valles: ESP_076435_1640 ESP_076369_1640 (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
-16.0	320.	5.27	22.25	35.6	33.7
Small Delta or Fan: ESP_076539_2150 ESP_077027_2150 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
34.76	356.	-6.0	7.624	53.1	47.2
Stepped Fan on West Crater Wall of Gale Crater: ESP_076534_1750 ESP_077154_1750 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.00	136.	8.87	-1.44	35.0	40.0
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