SDO HMI 2011-11-15 15:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.57 | 134.95 | 70.19 | 364.49 | 19.52 | 88.04 | 79.70 | 289.38 | 0.9823 | 24.3 | -133.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.44 | 49.40 | 12.30 | 184.10 | 18.98 | 91.01 | 82.67 | 288.78 | 0.9913 | -402.8 | -77.5 | |
| 4.38 | -1.00 | 16.48 | -1.00 | 19.25 | 91.26 | 82.92 | 289.06 | 0.9918 | 525.6 | 999999 | |
| 1.46 | 3.78 | 3.80 | 9.85 | 18.39 | 87.64 | 79.30 | 288.19 | 0.9824 | 210.4 | 97.6 | |
| 0.00 | 2.23 | 0.00 | 5.15 | 18.21 | 86.20 | 77.87 | 288.03 | 0.9776 | 0.0 | 50.2 | |
| 2.23 | 24.57 | 5.07 | 53.84 | 18.68 | 86.05 | 77.71 | 288.52 | 0.9771 | -379.4 | -270.6 | |
| 2.06 | -5.00 | 4.59 | -5.00 | 19.08 | 85.63 | 77.29 | 288.93 | 0.9757 | -474.2 | 999999 | |
| 0.00 | 1.72 | 0.00 | 4.64 | 20.47 | 88.17 | 79.83 | 290.31 | 0.9840 | -291.0 | -312.7 | |
| 0.86 | 1.37 | 1.95 | 3.11 | 20.20 | 85.84 | 77.50 | 290.08 | 0.9765 | -255.5 | -232.7 | |
| 0.00 | 0.26 | 0.00 | 0.50 | 19.34 | 83.45 | 75.11 | 289.27 | 0.9672 | 342.0 | 302.7 | |
| 0.00 | 1.37 | 0.00 | 2.71 | 19.85 | 83.91 | 75.57 | 289.78 | 0.9692 | -197.0 | -120.6 | |
| 1.80 | 48.88 | 3.77 | 98.01 | 20.79 | 84.80 | 76.46 | 290.71 | 0.9728 | -435.4 | -211.4 | |
| 0.00 | 1.37 | 0.00 | 2.58 | 19.61 | 83.07 | 74.73 | 289.56 | 0.9656 | 439.0 | 383.4 | |
| 3.01 | -11.00 | 6.34 | -11.00 | 21.23 | 84.82 | 76.49 | 291.17 | 0.9730 | -542.7 | 999999 | |
| 8.33 | -11.00 | 15.89 | -11.00 | 20.48 | 83.28 | 74.94 | 290.46 | 0.9667 | 422.4 | 999999 | |
| 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. | |