SDO HMI 2011-11-03 02:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.61 | 119.64 | 77.79 | 396.78 | 6.45 | 255.27 | 81.60 | 275.92 | 0.9860 | 76.1 | -35.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.13 | 74.74 | 35.16 | 326.08 | 6.12 | 257.47 | 83.80 | 275.69 | 0.9939 | 550.9 | -32.2 | |
| 2.68 | -1.00 | 10.79 | -1.00 | 5.83 | 256.92 | 83.24 | 275.36 | 0.9928 | -390.7 | 999999 | |
| 0.00 | 2.68 | 0.00 | 4.49 | 7.69 | 246.85 | 73.18 | 276.76 | 0.9566 | 67.0 | 53.5 | |
| 3.11 | 27.68 | 5.15 | 44.89 | 8.07 | 246.61 | 72.93 | 277.15 | 0.9552 | 278.1 | -304.9 | |
| 15.48 | -4.00 | 25.04 | -4.00 | 8.19 | 246.25 | 72.58 | 277.26 | 0.9534 | -513.1 | 999999 | |
| 0.00 | 5.71 | 0.00 | 8.74 | 7.66 | 245.13 | 71.46 | 276.67 | 0.9474 | -13.0 | -140.3 | |
| 0.00 | 2.25 | 0.00 | 3.28 | 8.03 | 244.16 | 70.48 | 277.03 | 0.9419 | 537.0 | 377.7 | |
| 0.00 | 1.30 | 0.00 | 1.89 | 8.45 | 244.15 | 70.48 | 277.47 | 0.9417 | 269.0 | 183.3 | |
| 0.00 | 0.78 | 0.00 | 1.15 | 11.12 | 244.46 | 70.78 | 280.32 | 0.9433 | 270.0 | 181.2 | |
| 0.00 | 0.87 | 0.00 | 1.18 | 8.28 | 242.75 | 69.08 | 277.25 | 0.9334 | 433.0 | 343.4 | |
| 0.00 | 1.12 | 0.00 | 1.63 | 11.33 | 244.11 | 70.44 | 280.53 | 0.9413 | 232.0 | 212.2 | |
| 1.21 | 1.73 | 1.65 | 2.35 | 8.46 | 242.66 | 68.98 | 277.45 | 0.9328 | 349.8 | 385.8 | |
| 0.00 | 0.78 | 0.00 | 1.10 | 11.30 | 243.55 | 69.88 | 280.50 | 0.9380 | 417.0 | 353.1 | |
| 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. | |