| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.43 | 164.94 | 33.82 | 101.76 | 19.93 | 64.07 | 25.32 | 317.54 | 0.5977 | 55.0 | 251.1 | |
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back to the solar disc SDO HMI 2011-02-13 18:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.91 | 39.63 | 15.76 | 25.06 | 19.47 | 67.35 | 28.60 | 313.49 | 0.6245 | -875.8 | -528.5 | |
| 0.00 | 0.94 | 0.00 | 0.61 | 21.32 | 67.26 | 28.51 | 315.79 | 0.6401 | -651.0 | -541.1 | |
| 0.00 | 1.11 | 0.00 | 0.70 | 19.20 | 66.80 | 28.06 | 313.71 | 0.6168 | -696.0 | -660.3 | |
| 0.00 | 1.63 | 0.00 | 1.03 | 20.11 | 66.58 | 27.84 | 315.04 | 0.6228 | -722.0 | -626.7 | |
| 1.11 | 3.25 | 0.69 | 2.02 | 18.64 | 66.09 | 27.35 | 313.72 | 0.6047 | -698.6 | -606.8 | |
| 0.00 | 2.48 | 0.00 | 1.54 | 18.75 | 65.80 | 27.05 | 314.17 | 0.6027 | -683.0 | -562.3 | |
| 0.00 | 2.31 | 0.00 | 1.42 | 18.82 | 64.69 | 25.95 | 315.43 | 0.5924 | 805.0 | 574.2 | |
| 2.91 | 3.34 | 1.78 | 2.04 | 18.94 | 64.36 | 25.62 | 315.93 | 0.5903 | 772.3 | 459.2 | |
| 0.00 | 1.11 | 0.00 | 0.68 | 19.61 | 63.54 | 24.79 | 317.68 | 0.5890 | 655.0 | 529.3 | |
| 1.20 | 97.41 | 0.73 | 59.41 | 19.72 | 63.10 | 24.36 | 318.31 | 0.5860 | 845.1 | 474.0 | |
| 0.94 | 1.37 | 0.59 | 0.86 | 21.98 | 63.50 | 24.76 | 320.47 | 0.6124 | -685.1 | -661.4 | |
| 0.00 | 2.74 | 0.00 | 1.68 | 20.55 | 63.10 | 24.36 | 319.29 | 0.5944 | 518.0 | 360.9 | |
| 5.73 | -10.00 | 3.49 | -10.00 | 19.74 | 62.80 | 24.05 | 318.68 | 0.5833 | 1213.8 | 999999 | |
| 12.84 | -10.00 | 7.83 | -10.00 | 20.13 | 62.65 | 23.91 | 319.31 | 0.5860 | 1101.1 | 999999 | |
| 2.48 | -10.00 | 1.51 | -10.00 | 20.18 | 62.25 | 23.50 | 319.84 | 0.5828 | 818.2 | 999999 | |
| 2.31 | 5.22 | 1.44 | 3.24 | 22.76 | 61.75 | 23.01 | 323.33 | 0.6058 | 665.7 | 447.0 | |
| 0.00 | 2.40 | 0.00 | 1.47 | 21.64 | 61.52 | 22.78 | 322.38 | 0.5918 | 719.0 | 553.8 | |
| 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. | |