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

East Endeavour Crater Dune Field: ESP_042674_1775 ESP_042740_1775 (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
-2.32	354.	7.30	-16.8	44.2	46.5
Echus Chasma Layered Deposits: ESP_042624_1790 ESP_069316_1790 (Interval in Earth days: 2080)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.04	280.	-4.9	-22.9	44.0	55.8
Candidate Landing Site for 2020 Mission: ESP_042430_1510 ESP_042364_1510 (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
-28.6	181.	-9.5	13.55	57.4	55.1
Fan on Crater Floor: ESP_042661_1505 ESP_046327_1505 (Interval in Earth days: 286)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-29.1	353.	3.01	-13.7	60.0	61.5
Convoluted Folds in Light-Toned Sulfates along Ius Chasma Floor: ESP_042255_1725 ESP_042466_1725 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.45	275.	6.80	-6.78	42.4	45.5
Inverted Channels on Fan in Saheki Crater: ESP_042368_1580 ESP_042869_1580 (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
-21.9	72.7	-2.1	12.98	51.9	57.0
Daedalia Planum Lava Flows: ESP_042072_1570 ESP_042573_1570 (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
-22.8	234.	2.53	16.55	48.1	53.9
Oxia Palus Region: ESP_042134_1985 ESP_053962_1985 (Interval in Earth days: 922)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.04	335.	7.47	-28.4	37.8	47.7
Fluvial Streambed in Mangala Valles: ESP_042653_1650 ESP_042719_1650 (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
-14.9	209.	3.83	-19.9	50.7	53.0
Sand Filled Crater in Medusae Fossae Region: ESP_042640_1815 ESP_042785_1815 (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
1.585	203.	-7.5	6.324	43.4	43.4
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