SDO HMI 2011-10-04 02:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.01 | 307.86 | 38.26 | 256.53 | 22.94 | 156.38 | -53.00 | 66.26 | 0.8057 | -727.8 | -254.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.67 | 25.84 | 156.01 | -53.36 | 62.79 | 0.8142 | -368.0 | -334.3 | |
| 13.72 | 246.47 | 11.26 | 203.67 | 22.48 | 156.97 | -52.40 | 66.71 | 0.7993 | -985.1 | -291.4 | |
| 21.99 | -2.00 | 18.24 | -2.00 | 22.96 | 156.55 | -52.83 | 66.20 | 0.8041 | -891.4 | 999999 | |
| 1.58 | -2.00 | 1.30 | -2.00 | 22.08 | 156.71 | -52.67 | 67.26 | 0.8012 | -708.7 | 999999 | |
| 0.62 | -2.00 | 0.51 | -2.00 | 22.45 | 156.24 | -53.14 | 66.88 | 0.8063 | -107.9 | 999999 | |
| 4.49 | 53.92 | 3.85 | 46.46 | 24.06 | 155.24 | -54.14 | 65.10 | 0.8181 | -888.2 | -126.9 | |
| 3.61 | -6.00 | 3.10 | -6.00 | 23.85 | 155.03 | -54.35 | 65.39 | 0.8196 | -696.7 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.67 | 20.68 | 155.55 | -53.83 | 69.17 | 0.8103 | 496.0 | 426.6 | |
| 0.00 | 0.88 | 0.00 | 0.77 | 22.98 | 153.96 | -55.41 | 66.61 | 0.8279 | -350.0 | -241.4 | |
| 0.00 | 0.79 | 0.00 | 0.67 | 20.19 | 155.36 | -54.01 | 69.79 | 0.8114 | 621.0 | 521.8 | |
| 0.00 | 1.06 | 0.00 | 0.90 | 21.15 | 154.86 | -54.52 | 68.69 | 0.8174 | -719.0 | -488.2 | |
| 0.00 | 1.76 | 0.00 | 1.51 | 21.30 | 154.72 | -54.66 | 68.53 | 0.8188 | -400.0 | -341.9 | |
| 0.00 | 1.14 | 0.00 | 0.97 | 20.02 | 155.23 | -54.14 | 70.02 | 0.8125 | 431.0 | 383.5 | |
| 0.00 | 0.26 | 0.00 | 0.24 | 23.78 | 152.56 | -56.82 | 65.87 | 0.8413 | 528.0 | 518.3 | |
| 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. | |