SDO HMI 2011-07-19 11:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.31 | 112.27 | 33.38 | 125.10 | 24.50 | 78.73 | -63.09 | 64.92 | 0.8972 | -38.1 | -155.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.91 | 2.72 | 2.10 | 2.99 | 25.48 | 79.26 | -62.56 | 63.78 | 0.8949 | -269.5 | -272.4 | |
| 10.53 | 69.43 | 11.27 | 74.38 | 24.47 | 80.01 | -61.81 | 64.80 | 0.8885 | -776.5 | -365.4 | |
| 1.63 | -2.00 | 1.77 | -2.00 | 24.74 | 79.70 | -62.12 | 64.54 | 0.8910 | -519.8 | 999999 | |
| 0.45 | -2.00 | 0.50 | -2.00 | 24.85 | 79.31 | -62.51 | 64.47 | 0.8939 | -421.0 | 999999 | |
| 2.63 | 8.62 | 2.91 | 9.61 | 24.60 | 79.03 | -62.80 | 64.79 | 0.8957 | -242.0 | -31.7 | |
| 0.00 | 1.63 | 0.00 | 1.85 | 24.27 | 78.19 | -63.63 | 65.25 | 0.9011 | 348.0 | 220.6 | |
| 0.00 | 1.18 | 0.00 | 1.31 | 23.56 | 78.76 | -63.06 | 65.98 | 0.8965 | 399.0 | 357.7 | |
| 0.00 | 2.45 | 0.00 | 2.74 | 23.71 | 78.55 | -63.27 | 65.84 | 0.8981 | 576.0 | 401.5 | |
| 1.00 | 1.91 | 1.13 | 2.16 | 23.38 | 78.09 | -63.73 | 66.26 | 0.9010 | 482.6 | 444.3 | |
| 0.00 | 1.18 | 0.00 | 1.36 | 23.71 | 77.72 | -64.11 | 65.93 | 0.9039 | 550.0 | 506.5 | |
| 0.00 | 0.64 | 0.00 | 0.77 | 24.53 | 76.29 | -65.53 | 65.18 | 0.9140 | 414.0 | 352.1 | |
| 4.36 | 5.26 | 5.13 | 6.20 | 23.76 | 76.97 | -64.85 | 65.96 | 0.9089 | 572.3 | 495.7 | |
| 1.18 | 1.63 | 1.42 | 1.97 | 24.14 | 76.36 | -65.46 | 65.60 | 0.9132 | 385.5 | 486.6 | |
| 0.00 | 0.73 | 0.00 | 0.87 | 23.98 | 76.43 | -65.39 | 65.77 | 0.9126 | 433.0 | 364.9 | |
| 0.45 | 2.27 | 0.58 | 2.92 | 25.52 | 74.72 | -67.10 | 64.27 | 0.9244 | 431.8 | 339.2 | |
| 3.99 | 6.63 | 5.10 | 8.45 | 25.13 | 74.90 | -66.92 | 64.67 | 0.9231 | 450.6 | 409.3 | |
| 1.18 | 5.99 | 1.47 | 7.52 | 24.27 | 75.40 | -66.42 | 65.56 | 0.9194 | 500.7 | 292.3 | |
| 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. | |