| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.18 | 164.30 | 45.72 | 184.03 | 7.72 | 129.48 | -63.64 | 81.98 | 0.8977 | -90.3 | -140.7 | |
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back to the solar disc SDO HMI 2011-11-28 22:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.82 | 0.00 | 2.97 | 9.25 | 131.35 | -61.77 | 80.16 | 0.8845 | 446.0 | 393.1 | |
| 16.07 | 87.71 | 16.77 | 91.34 | 7.55 | 131.57 | -61.55 | 82.07 | 0.8820 | -700.9 | -317.7 | |
| 1.28 | 2.05 | 1.37 | 2.19 | 5.48 | 130.74 | -62.38 | 84.45 | 0.8881 | -489.9 | -449.4 | |
| 0.00 | 1.03 | 0.00 | 1.11 | 7.14 | 130.31 | -62.81 | 82.60 | 0.8919 | -541.0 | -419.3 | |
| 4.53 | 5.56 | 4.90 | 6.00 | 6.39 | 130.42 | -62.70 | 83.43 | 0.8908 | -417.0 | -339.2 | |
| 0.00 | 0.85 | 0.00 | 0.93 | 6.66 | 130.30 | -62.82 | 83.14 | 0.8919 | -219.0 | -206.6 | |
| 0.00 | 2.74 | 0.00 | 3.01 | 7.07 | 130.00 | -63.12 | 82.69 | 0.8943 | -274.0 | -193.7 | |
| 0.00 | 1.45 | 0.00 | 1.62 | 7.39 | 129.65 | -63.47 | 82.34 | 0.8971 | -417.0 | -324.8 | |
| 1.97 | 2.99 | 2.22 | 3.38 | 6.94 | 129.15 | -63.97 | 82.87 | 0.9008 | -325.5 | -68.4 | |
| 1.62 | 8.46 | 1.85 | 9.59 | 7.47 | 129.01 | -64.11 | 82.28 | 0.9020 | 283.1 | -149.6 | |
| 0.00 | 1.20 | 0.00 | 1.38 | 8.03 | 128.57 | -64.54 | 81.68 | 0.9054 | -278.0 | -209.5 | |
| 0.00 | 0.94 | 0.00 | 1.10 | 8.21 | 128.24 | -64.88 | 81.51 | 0.9079 | -313.0 | -261.0 | |
| 3.42 | 6.92 | 4.12 | 8.32 | 8.79 | 127.47 | -65.65 | 80.90 | 0.9136 | 476.4 | 498.9 | |
| 0.00 | 1.71 | 0.00 | 2.13 | 8.92 | 126.68 | -66.44 | 80.79 | 0.9191 | 380.0 | 330.0 | |
| 7.44 | 36.67 | 9.47 | 47.44 | 8.25 | 126.07 | -67.05 | 81.55 | 0.9230 | 655.7 | 118.2 | |
| 0.00 | 1.20 | 0.00 | 1.52 | 7.81 | 126.14 | -66.98 | 82.03 | 0.9224 | 570.0 | 460.1 | |
| 3.85 | -15.00 | 5.02 | -15.00 | 7.94 | 125.47 | -67.65 | 81.91 | 0.9269 | 438.3 | 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. | |