SDO HMI 2011-04-27 05:59:06 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.90 | 234.42 | 46.81 | 142.59 | 20.68 | 188.53 | 25.26 | 316.53 | 0.5818 | -228.4 | -32.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.14 | 0.00 | 1.34 | 21.33 | 191.39 | 28.12 | 314.28 | 0.6155 | -557.0 | -447.4 | |
| 0.00 | 0.98 | 0.00 | 0.62 | 21.76 | 191.33 | 28.07 | 314.87 | 0.6188 | -361.0 | -285.4 | |
| 0.00 | 2.67 | 0.00 | 1.67 | 21.52 | 191.17 | 27.91 | 314.73 | 0.6151 | -620.0 | -547.2 | |
| 19.59 | 102.20 | 12.12 | 63.26 | 20.34 | 190.86 | 27.59 | 313.55 | 0.6015 | -1100.7 | -398.4 | |
| 6.32 | -4.00 | 3.93 | -4.00 | 20.91 | 190.86 | 27.60 | 314.27 | 0.6065 | -849.1 | 999999 | |
| 2.58 | -4.00 | 1.60 | -4.00 | 20.64 | 190.66 | 27.40 | 314.12 | 0.6021 | -1025.2 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.61 | 21.53 | 190.40 | 27.14 | 315.50 | 0.6076 | -470.0 | -421.7 | |
| 7.83 | -4.00 | 4.83 | -4.00 | 20.72 | 190.17 | 26.90 | 314.72 | 0.5979 | -1042.3 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.66 | 21.59 | 190.19 | 26.93 | 315.79 | 0.6062 | -643.0 | -542.9 | |
| 0.89 | -4.00 | 0.55 | -4.00 | 20.91 | 189.95 | 26.69 | 315.19 | 0.5975 | -641.5 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.77 | 21.61 | 189.98 | 26.72 | 316.04 | 0.6044 | -662.0 | -546.7 | |
| 0.00 | 2.14 | 0.00 | 1.31 | 20.10 | 189.69 | 26.43 | 314.43 | 0.5875 | -537.0 | -465.2 | |
| 3.92 | 18.34 | 2.36 | 11.06 | 19.76 | 188.60 | 25.33 | 315.16 | 0.5732 | -867.4 | -419.6 | |
| 1.69 | -13.00 | 1.02 | -13.00 | 19.72 | 188.34 | 25.08 | 315.38 | 0.5702 | -936.0 | 999999 | |
| 1.60 | -13.00 | 0.97 | -13.00 | 19.98 | 188.35 | 25.09 | 315.72 | 0.5729 | 366.1 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.65 | 21.43 | 188.61 | 25.34 | 317.26 | 0.5894 | -634.0 | -450.2 | |
| 0.00 | 2.31 | 0.00 | 1.39 | 19.35 | 188.21 | 24.94 | 315.05 | 0.5654 | -888.0 | -660.7 | |
| 0.00 | 2.23 | 0.00 | 1.36 | 21.51 | 188.27 | 25.00 | 317.75 | 0.5870 | -869.0 | -664.0 | |
| 0.00 | 2.40 | 0.00 | 1.47 | 21.95 | 188.28 | 25.01 | 318.27 | 0.5914 | 707.0 | 503.4 | |
| 3.92 | 5.88 | 2.39 | 3.58 | 21.61 | 188.00 | 24.73 | 318.16 | 0.5853 | -826.0 | -588.1 | |
| 0.00 | 1.51 | 0.00 | 0.90 | 19.18 | 187.09 | 23.83 | 316.10 | 0.5524 | 672.0 | 571.4 | |
| 4.36 | 4.99 | 2.66 | 3.04 | 22.09 | 187.41 | 24.14 | 319.41 | 0.5847 | 697.3 | 417.4 | |
| 0.00 | 0.71 | 0.00 | 0.43 | 21.78 | 187.14 | 23.87 | 319.34 | 0.5790 | -602.0 | -570.8 | |
| 0.00 | 1.16 | 0.00 | 0.68 | 19.42 | 186.47 | 23.20 | 317.16 | 0.5485 | 701.0 | 509.5 | |
| 0.00 | 0.80 | 0.00 | 0.48 | 20.18 | 186.44 | 23.18 | 318.17 | 0.5561 | 646.0 | 518.8 | |
| 0.00 | 1.34 | 0.00 | 0.79 | 19.61 | 186.22 | 22.95 | 317.71 | 0.5480 | 798.0 | 681.5 | |
| 0.00 | 1.16 | 0.00 | 0.69 | 19.94 | 186.16 | 22.90 | 318.20 | 0.5509 | 650.0 | 483.2 | |
| 0.00 | 1.16 | 0.00 | 0.68 | 19.51 | 185.96 | 22.69 | 317.88 | 0.5444 | 804.0 | 575.2 | |
| 2.31 | 32.67 | 1.38 | 19.51 | 21.14 | 186.00 | 22.74 | 319.90 | 0.5618 | 771.6 | 557.8 | |
| 0.00 | 0.89 | 0.00 | 0.53 | 21.40 | 185.83 | 22.57 | 320.42 | 0.5630 | 502.0 | 404.3 | |
| 7.75 | -29.00 | 4.61 | -29.00 | 20.93 | 185.72 | 22.46 | 319.98 | 0.5570 | 998.3 | 999999 | |
| 5.07 | 14.51 | 3.03 | 8.66 | 21.56 | 185.54 | 22.28 | 320.97 | 0.5620 | 577.9 | 706.6 | |
| 5.96 | 22.52 | 3.52 | 13.29 | 20.31 | 185.28 | 22.01 | 319.76 | 0.5463 | 1084.9 | 634.8 | |
| 1.60 | 5.34 | 0.95 | 3.16 | 20.78 | 185.17 | 21.91 | 320.47 | 0.5503 | 902.5 | 712.6 | |
| 1.51 | -34.00 | 0.89 | -34.00 | 20.70 | 184.99 | 21.73 | 320.61 | 0.5478 | 795.1 | 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. | |