SDO HMI 2011-11-02 17:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 160.45 | 1186.03 | 270.87 | 2092.29 | 18.98 | 105.55 | -73.08 | 71.38 | 0.9532 | -152.3 | 93.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.69 | 9.85 | 1.02 | 14.60 | 22.51 | 108.02 | -70.61 | 67.61 | 0.9440 | 197.1 | -269.4 | |
| 0.52 | -1.00 | 0.76 | -1.00 | 22.17 | 108.32 | -70.32 | 67.95 | 0.9423 | 110.2 | 999999 | |
| 4.15 | -1.00 | 6.13 | -1.00 | 22.29 | 108.09 | -70.55 | 67.84 | 0.9435 | -449.5 | 999999 | |
| 18.85 | 900.69 | 24.69 | 1420.10 | 18.42 | 110.65 | -67.98 | 71.83 | 0.9274 | -943.6 | 84.0 | |
| 46.42 | -4.00 | 64.02 | -4.00 | 18.93 | 109.42 | -69.21 | 71.34 | 0.9350 | -581.3 | 999999 | |
| 6.83 | -4.00 | 9.71 | -4.00 | 18.98 | 108.74 | -69.90 | 71.32 | 0.9389 | 138.8 | 999999 | |
| 2.51 | 93.62 | 4.11 | 168.29 | 21.50 | 105.85 | -72.78 | 68.78 | 0.9547 | -278.9 | 386.3 | |
| 2.16 | -7.00 | 3.54 | -7.00 | 21.24 | 105.85 | -72.78 | 69.05 | 0.9547 | -317.1 | 999999 | |
| 3.28 | -7.00 | 5.56 | -7.00 | 21.26 | 105.26 | -73.37 | 69.05 | 0.9575 | 451.5 | 999999 | |
| 9.16 | -4.00 | 13.41 | -4.00 | 18.40 | 108.07 | -70.57 | 71.97 | 0.9426 | -407.5 | 999999 | |
| 0.95 | -7.00 | 1.60 | -7.00 | 20.91 | 105.27 | -73.37 | 69.41 | 0.9574 | -254.5 | 999999 | |
| 1.04 | -7.00 | 1.80 | -7.00 | 20.73 | 104.83 | -73.81 | 69.63 | 0.9594 | -109.8 | 999999 | |
| 5.96 | -4.00 | 9.05 | -4.00 | 18.47 | 107.31 | -71.32 | 71.91 | 0.9467 | 240.2 | 999999 | |
| 6.05 | -4.00 | 9.04 | -4.00 | 18.09 | 107.59 | -71.04 | 72.31 | 0.9451 | -255.3 | 999999 | |
| 0.00 | 14.09 | 0.00 | 19.77 | 16.41 | 108.97 | -69.66 | 74.05 | 0.9370 | -158.0 | -141.5 | |
| 0.52 | -4.00 | 0.78 | -4.00 | 18.01 | 107.37 | -71.26 | 72.40 | 0.9463 | 139.7 | 999999 | |
| 4.41 | -4.00 | 7.78 | -4.00 | 19.63 | 104.50 | -74.13 | 70.78 | 0.9608 | 266.6 | 999999 | |
| 1.73 | -4.00 | 3.65 | -4.00 | 21.23 | 101.62 | -77.02 | 69.17 | 0.9729 | 446.7 | 999999 | |
| 0.00 | 1.47 | 0.00 | 3.55 | 22.21 | 99.59 | -79.05 | 68.18 | 0.9800 | 198.0 | 124.5 | |
| 2.68 | -4.00 | 4.69 | -4.00 | 18.94 | 104.54 | -74.09 | 71.50 | 0.9605 | 745.5 | 999999 | |
| 5.10 | -4.00 | 8.57 | -4.00 | 17.83 | 105.25 | -73.38 | 72.64 | 0.9570 | 380.0 | 999999 | |
| 7.61 | -4.00 | 12.60 | -4.00 | 17.57 | 105.54 | -73.10 | 72.91 | 0.9557 | -364.0 | 999999 | |
| 0.00 | 0.61 | 0.00 | 1.43 | 21.40 | 99.91 | -78.72 | 69.01 | 0.9789 | 444.0 | 484.7 | |
| 1.04 | -4.00 | 1.82 | -4.00 | 18.09 | 104.51 | -74.13 | 72.38 | 0.9606 | 862.0 | 999999 | |
| 0.00 | 3.11 | 0.00 | 9.08 | 22.03 | 97.52 | -81.11 | 68.36 | 0.9861 | 470.0 | 379.6 | |
| 4.58 | -4.00 | 9.24 | -4.00 | 19.34 | 102.24 | -76.40 | 71.11 | 0.9704 | 527.4 | 999999 | |
| 0.00 | 2.59 | 0.00 | 4.90 | 17.25 | 103.20 | -75.43 | 73.27 | 0.9664 | 631.0 | 500.9 | |
| 0.00 | 2.42 | 0.00 | 6.22 | 19.93 | 98.88 | -79.75 | 70.51 | 0.9823 | 378.0 | 350.1 | |
| 12.02 | 126.64 | 30.68 | 370.32 | 19.27 | 98.94 | -79.70 | 71.18 | 0.9821 | 438.6 | -27.3 | |
| 0.00 | 0.86 | 0.00 | 2.16 | 18.53 | 99.26 | -79.37 | 71.93 | 0.9811 | 353.0 | 322.9 | |
| 6.14 | -29.00 | 17.93 | -29.00 | 19.29 | 97.52 | -81.11 | 71.13 | 0.9862 | 150.4 | 999999 | |
| 0.00 | 0.95 | 0.00 | 2.05 | 17.08 | 101.26 | -77.38 | 73.44 | 0.9742 | 378.0 | 309.5 | |
| 0.00 | 5.27 | 0.00 | 13.04 | 18.14 | 99.45 | -79.19 | 72.34 | 0.9805 | 260.0 | 222.8 | |
| 6.05 | -29.00 | 18.69 | -29.00 | 19.13 | 97.04 | -81.60 | 71.29 | 0.9875 | -373.4 | 999999 | |
| 0.00 | 23.86 | 0.00 | 56.78 | 17.46 | 99.93 | -78.70 | 73.04 | 0.9789 | 263.0 | 127.3 | |
| 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. | |