| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.63 | 165.26 | 42.29 | 180.67 | 7.67 | 129.64 | -62.93 | 82.00 | 0.8923 | -95.2 | -156.8 | |
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back to the solar disc SDO HMI 2011-11-28 23:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.80 | 0.00 | 1.85 | 9.23 | 131.50 | -61.06 | 80.13 | 0.8788 | 385.0 | 363.5 | |
| 14.28 | 91.39 | 14.63 | 93.39 | 7.53 | 131.59 | -60.98 | 82.06 | 0.8773 | -723.1 | -331.1 | |
| 0.00 | 1.11 | 0.00 | 1.17 | 8.74 | 130.76 | -61.80 | 80.74 | 0.8846 | 470.0 | 417.5 | |
| 0.00 | 0.94 | 0.00 | 0.99 | 6.85 | 130.67 | -61.89 | 82.87 | 0.8845 | -304.0 | -338.8 | |
| 0.00 | 1.71 | 0.00 | 1.79 | 5.49 | 130.76 | -61.80 | 84.42 | 0.8834 | -518.0 | -450.6 | |
| 0.00 | 1.20 | 0.00 | 1.27 | 7.09 | 130.36 | -62.20 | 82.62 | 0.8871 | -431.0 | -367.5 | |
| 3.08 | 6.50 | 3.26 | 6.89 | 6.37 | 130.46 | -62.11 | 83.43 | 0.8861 | -502.9 | -288.5 | |
| 0.00 | 1.88 | 0.00 | 2.02 | 6.96 | 130.07 | -62.50 | 82.78 | 0.8894 | -165.0 | -143.2 | |
| 0.00 | 1.28 | 0.00 | 1.39 | 7.34 | 129.71 | -62.85 | 82.37 | 0.8923 | -422.0 | -314.9 | |
| 3.08 | 8.04 | 3.40 | 8.91 | 7.58 | 129.32 | -63.25 | 82.12 | 0.8955 | -416.6 | 19.1 | |
| 1.20 | -10.00 | 1.33 | -10.00 | 7.45 | 129.15 | -63.42 | 82.27 | 0.8967 | 272.9 | 999999 | |
| 1.88 | 4.45 | 2.08 | 4.93 | 6.95 | 129.15 | -63.42 | 82.84 | 0.8966 | -350.6 | -89.1 | |
| 0.00 | 1.28 | 0.00 | 1.45 | 8.04 | 128.65 | -63.92 | 81.64 | 0.9008 | -247.0 | -187.5 | |
| 0.00 | 0.68 | 0.00 | 0.78 | 8.15 | 128.27 | -64.30 | 81.53 | 0.9036 | -263.0 | -167.5 | |
| 1.54 | 6.24 | 1.82 | 7.35 | 8.80 | 127.50 | -65.07 | 80.86 | 0.9095 | 629.8 | 480.3 | |
| 8.38 | 36.76 | 10.44 | 46.49 | 8.20 | 126.08 | -66.49 | 81.58 | 0.9192 | 671.4 | 147.2 | |
| 4.19 | -16.00 | 5.33 | -16.00 | 7.98 | 125.54 | -67.03 | 81.84 | 0.9228 | 461.4 | 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. | |