SDO HMI 2011-07-19 10:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.50 | 100.82 | 30.57 | 114.03 | 24.48 | 78.75 | -63.62 | 65.00 | 0.9009 | -85.1 | -184.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.27 | 2.72 | 1.42 | 3.05 | 25.44 | 79.24 | -63.13 | 63.90 | 0.8988 | -269.6 | -173.3 | |
| 11.89 | 64.71 | 12.97 | 70.39 | 24.46 | 79.98 | -62.39 | 64.88 | 0.8926 | -724.8 | -392.0 | |
| 2.72 | -2.00 | 3.00 | -2.00 | 24.74 | 79.66 | -62.71 | 64.62 | 0.8952 | -511.7 | 999999 | |
| 1.18 | 5.26 | 1.33 | 5.93 | 24.59 | 78.91 | -63.47 | 64.89 | 0.9003 | -163.6 | -171.7 | |
| 0.00 | 0.91 | 0.00 | 1.00 | 23.46 | 79.38 | -62.99 | 66.07 | 0.8959 | -179.0 | -124.9 | |
| 0.00 | 1.72 | 0.00 | 1.97 | 24.42 | 78.45 | -63.92 | 65.13 | 0.9033 | 29.0 | 51.1 | |
| 0.00 | 2.72 | 0.00 | 3.10 | 23.80 | 78.49 | -63.88 | 65.81 | 0.9024 | 270.0 | 286.6 | |
| 0.00 | 1.54 | 0.00 | 1.78 | 23.31 | 78.09 | -64.29 | 66.39 | 0.9048 | 537.0 | 464.5 | |
| 4.45 | 5.54 | 5.34 | 6.64 | 23.79 | 77.00 | -65.37 | 65.98 | 0.9124 | 555.0 | 493.9 | |
| 0.00 | 1.00 | 0.00 | 1.23 | 24.17 | 76.38 | -65.99 | 65.62 | 0.9167 | 400.0 | 371.5 | |
| 0.00 | 1.09 | 0.00 | 1.33 | 23.98 | 76.49 | -65.89 | 65.82 | 0.9158 | 432.0 | 368.0 | |
| 0.00 | 1.18 | 0.00 | 1.55 | 25.58 | 74.75 | -67.62 | 64.25 | 0.9276 | 388.0 | 305.7 | |
| 4.99 | 6.53 | 6.51 | 8.52 | 25.09 | 74.87 | -67.50 | 64.77 | 0.9265 | 457.9 | 343.2 | |
| 0.00 | 5.90 | 0.00 | 7.54 | 24.29 | 75.32 | -67.05 | 65.59 | 0.9233 | 433.0 | 336.4 | |
| 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. | |