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.

Mawrth Vallis Region:   ESP_039879_2025   ESP_040301_2025   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.02

342.

-5.3

-24.1

60.9

56.9

Small Volcano in Ceraunius Fossae Region:   ESP_039645_2060   ESP_040001_2060   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.50

250.

-10.

3.512

65.8

61.5

Seasonal Monitoring Candidate:   ESP_039874_0930   ESP_039901_0930   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.0

170.

8.00

1.074

64.9

65.9

Barchan Dune Changes:   ESP_039666_1380   ESP_039732_1380   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.4

44.6

1.20

-14.9

41.0

41.6

Ridges in Zephyria Planum:   ESP_039675_1760   ESP_040097_1760   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.03

153.

5.34

-6.18

46.5

42.2

Floor Deposits in East Candor Chasma:   ESP_039604_1720   ESP_039749_1720   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.04

293.

-6.5

15.65

46.4

43.1

Alluvial Fan in Equatorial Crater:   ESP_039889_1565   ESP_040522_1565   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.1

74.0

9.04

-14.3

37.4

35.0

Gullies and Viscous Flow Feature in Nereidum Montes:   ESP_039643_1400   ESP_039709_1400   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.4

311.

4.84

-12.0

40.6

41.2

Fresh Gullied Crater with Diverse Lithologies:   ESP_039616_1420   ESP_039682_1420   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.5

329.

-3.3

-20.1

41.2

41.8

Alluvial Fans in Southeastern Mojave Crater:   ESP_039695_1875   ESP_040618_1875   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.214

327.

-7.2

11.40

53.2

41.0


  


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