SDO HMI 2011-11-02 13:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 145.36 | 989.02 | 277.80 | 2003.91 | 19.04 | 105.44 | -75.40 | 71.36 | 0.9637 | -104.3 | 96.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.30 | 9.34 | 2.13 | 15.42 | 22.40 | 108.05 | -72.79 | 67.84 | 0.9549 | -420.6 | -264.0 | |
| 0.35 | -1.00 | 0.56 | -1.00 | 22.18 | 108.22 | -72.62 | 68.06 | 0.9541 | 43.8 | 999999 | |
| 21.19 | 714.11 | 30.41 | 1241.48 | 18.50 | 110.71 | -70.12 | 71.85 | 0.9401 | -827.1 | 64.9 | |
| 37.01 | -3.00 | 56.23 | -3.00 | 18.98 | 109.56 | -71.27 | 71.38 | 0.9465 | -439.2 | 999999 | |
| 1.04 | 99.96 | 1.94 | 214.40 | 21.79 | 105.73 | -75.11 | 68.56 | 0.9653 | 142.1 | 435.6 | |
| 0.00 | 1.99 | 0.00 | 3.77 | 21.99 | 105.42 | -75.42 | 68.36 | 0.9666 | 414.0 | 264.0 | |
| 1.21 | -5.00 | 2.25 | -5.00 | 21.47 | 105.82 | -75.02 | 68.88 | 0.9649 | -228.2 | 999999 | |
| 7.26 | -3.00 | 11.34 | -3.00 | 18.94 | 109.00 | -71.84 | 71.44 | 0.9495 | 142.0 | 999999 | |
| 2.25 | -5.00 | 4.20 | -5.00 | 21.17 | 105.64 | -75.20 | 69.20 | 0.9656 | -264.5 | 999999 | |
| 2.85 | -5.00 | 5.58 | -5.00 | 21.19 | 104.96 | -75.88 | 69.19 | 0.9684 | 515.0 | 999999 | |
| 3.03 | -5.00 | 6.67 | -5.00 | 21.92 | 103.13 | -77.71 | 68.47 | 0.9755 | 426.1 | 999999 | |
| 13.92 | -3.00 | 22.84 | -3.00 | 18.30 | 107.90 | -72.94 | 72.14 | 0.9550 | -281.1 | 999999 | |
| 0.00 | 0.86 | 0.00 | 2.09 | 22.03 | 101.94 | -78.90 | 68.36 | 0.9795 | -279.0 | -238.6 | |
| 6.57 | -3.00 | 11.13 | -3.00 | 18.36 | 107.39 | -73.45 | 72.09 | 0.9574 | 217.7 | 999999 | |
| 0.00 | 0.35 | 0.00 | 0.54 | 16.81 | 108.88 | -71.96 | 73.68 | 0.9498 | -294.0 | -369.8 | |
| 3.98 | 12.11 | 6.17 | 18.88 | 16.33 | 109.02 | -71.81 | 74.19 | 0.9490 | -117.5 | -100.2 | |
| 5.27 | -3.00 | 10.60 | -3.00 | 19.61 | 104.55 | -76.29 | 70.83 | 0.9700 | 316.8 | 999999 | |
| 0.43 | -5.00 | 1.06 | -5.00 | 21.25 | 101.69 | -79.15 | 69.17 | 0.9803 | 450.8 | 999999 | |
| 0.00 | 1.38 | 0.00 | 4.95 | 22.09 | 97.79 | -83.05 | 68.27 | 0.9908 | 329.0 | 318.6 | |
| 4.76 | -3.00 | 9.12 | -3.00 | 17.84 | 105.27 | -75.57 | 72.66 | 0.9669 | 368.4 | 999999 | |
| 1.99 | -3.00 | 3.93 | -3.00 | 18.12 | 104.78 | -76.06 | 72.37 | 0.9690 | 963.9 | 999999 | |
| 5.53 | -3.00 | 10.41 | -3.00 | 17.57 | 105.48 | -75.36 | 72.93 | 0.9661 | -254.2 | 999999 | |
| 0.00 | 3.29 | 0.00 | 10.16 | 21.02 | 99.04 | -81.80 | 69.37 | 0.9879 | 467.0 | 406.2 | |
| 3.20 | -3.00 | 7.48 | -3.00 | 19.33 | 102.34 | -78.49 | 71.13 | 0.9782 | 366.7 | 999999 | |
| 0.00 | 1.47 | 0.00 | 3.39 | 18.67 | 102.50 | -78.34 | 71.80 | 0.9777 | 524.0 | 468.6 | |
| 0.00 | 5.19 | 0.00 | 10.65 | 17.04 | 104.18 | -76.66 | 73.48 | 0.9714 | 419.0 | 441.0 | |
| 0.00 | 0.78 | 0.00 | 2.37 | 19.80 | 99.30 | -81.54 | 70.61 | 0.9873 | 457.0 | 456.3 | |
| 1.64 | 34.68 | 4.01 | 94.96 | 18.25 | 101.75 | -79.09 | 72.23 | 0.9802 | 430.2 | 235.8 | |
| 0.00 | 0.35 | 0.00 | 0.76 | 17.25 | 103.17 | -77.67 | 73.26 | 0.9753 | 413.0 | 420.5 | |
| 8.99 | 99.27 | 27.98 | 368.00 | 19.22 | 99.16 | -81.68 | 71.19 | 0.9877 | 384.7 | -57.1 | |
| 1.56 | -30.00 | 5.55 | -30.00 | 19.51 | 97.90 | -82.94 | 70.87 | 0.9907 | 54.6 | 999999 | |
| 0.35 | -30.00 | 1.25 | -30.00 | 19.27 | 97.55 | -83.29 | 71.11 | 0.9915 | 46.2 | 999999 | |
| 7.52 | -30.00 | 29.09 | -30.00 | 19.15 | 97.33 | -83.51 | 71.21 | 0.9920 | -309.4 | 999999 | |
| 0.00 | 2.51 | 0.00 | 7.48 | 18.15 | 99.48 | -81.36 | 72.29 | 0.9870 | 315.0 | 298.9 | |
| 2.16 | -28.00 | 5.87 | -28.00 | 17.38 | 100.63 | -80.21 | 73.09 | 0.9838 | 300.0 | 999999 | |
| 0.00 | 1.38 | 0.00 | 4.61 | 18.03 | 98.36 | -82.47 | 72.38 | 0.9898 | -97.0 | -108.0 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |