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.

Candidate Landing Site for 2020 Mission in Northeast Syrtis Major Region:   ESP_038029_1980   ESP_046271_1980   (Interval in Earth days: 642)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.53

76.6

4.59

-17.0

59.2

51.4

Infrared-Distinct Crater:   ESP_038309_1460   ESP_046775_1460   (Interval in Earth days: 660)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.8

1.28

-1.5

8.972

58.2

57.4

Hardened Dunes in Arcadia Planitia:   ESP_038143_2205   ESP_055536_2205   (Interval in Earth days: 1355)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.98

202.

-3.1

-20.7

69.0

64.2

A Light Toned Deposit in Arsinoes Chaos:   ESP_037545_1730   ESP_089278_1730   (Interval in Earth days: 4030)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.03

332.

2.25

-14.9

57.3

60.8

Possible Future Mars Landing Site in Oxia Planum:   ESP_037070_1985   ESP_037136_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.12

336.

7.98

-13.7

51.6

53.9

InSight Mission Candidate Landing Site:   ESP_037961_1845   ESP_038449_1845   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.572

135.

-11.

0.843

58.1

58.0

Daedalia Planum Lava Flows:   ESP_037720_1565   ESP_046028_1565   (Interval in Earth days: 647)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.0

237.

-0.1

-27.2

61.0

61.7

Candidate Landing Site for 2020 Mission Near Nili Fossae:   ESP_037673_2015   ESP_037739_2015   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.14

74.1

4.25

-14.2

56.9

59.0

Extensive Raised Ridges in Eridania Region:   ESP_037788_1495   ESP_046109_1495   (Interval in Earth days: 649)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.3

181.

4.59

28.59

62.4

60.9

Hebes Chasma:   ESP_037705_1790   ESP_046659_1790   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.05

283.

-2.8

8.6

56.8

50.8


  


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