SDO HMI 2011-10-22 15:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.80 | 394.93 | 109.19 | 775.46 | 7.73 | 249.16 | -75.64 | 83.40 | 0.9637 | -196.4 | -62.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.22 | 0.00 | 1.65 | 10.95 | 255.65 | -69.15 | 80.29 | 0.9324 | -158.0 | -181.7 | |
| 23.66 | 256.39 | 33.47 | 374.39 | 6.20 | 254.88 | -69.92 | 85.34 | 0.9383 | -727.2 | -132.4 | |
| 14.35 | -2.00 | 21.22 | -2.00 | 6.10 | 254.00 | -70.79 | 85.40 | 0.9435 | -312.3 | 999999 | |
| 1.04 | -2.00 | 1.54 | -2.00 | 5.67 | 253.94 | -70.85 | 85.85 | 0.9440 | -272.8 | 999999 | |
| 2.96 | -2.00 | 4.53 | -2.00 | 5.94 | 253.29 | -71.50 | 85.51 | 0.9476 | 208.8 | 999999 | |
| 0.00 | 1.30 | 0.00 | 2.14 | 4.66 | 251.98 | -72.81 | 86.77 | 0.9550 | 364.0 | 378.7 | |
| 0.00 | 0.61 | 0.00 | 1.15 | 6.13 | 249.61 | -75.19 | 85.07 | 0.9660 | -238.0 | -149.0 | |
| 0.00 | 3.39 | 0.00 | 7.16 | 6.58 | 247.88 | -76.92 | 84.49 | 0.9732 | 340.0 | 294.2 | |
| 4.44 | 126.28 | 11.97 | 374.52 | 10.23 | 244.70 | -80.10 | 80.55 | 0.9836 | 367.1 | -17.4 | |
| 2.52 | -9.00 | 6.80 | -9.00 | 9.77 | 244.63 | -80.16 | 81.02 | 0.9839 | 332.6 | 999999 | |
| 5.22 | -9.00 | 14.60 | -9.00 | 9.43 | 244.24 | -80.56 | 81.34 | 0.9852 | 402.5 | 999999 | |
| 0.00 | 4.35 | 0.00 | 10.93 | 6.48 | 245.71 | -79.08 | 84.44 | 0.9811 | 297.0 | 229.5 | |
| 0.00 | 1.39 | 0.00 | 3.52 | 6.68 | 245.59 | -79.21 | 84.23 | 0.9815 | 271.0 | 138.9 | |
| 4.61 | -9.00 | 15.06 | -9.00 | 8.55 | 242.91 | -81.88 | 82.14 | 0.9890 | -371.2 | 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. | |