| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.16 | 120.29 | 17.63 | 72.66 | 17.96 | 223.80 | 31.23 | 300.55 | 0.5750 | -532.3 | -326.6 | |
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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 | 0.43 | 0.00 | 0.28 | 22.34 | 229.07 | 36.50 | 303.52 | 0.6623 | -404.0 | -317.4 | |
| 0.00 | 1.37 | 0.00 | 0.85 | 19.86 | 225.88 | 33.31 | 302.02 | 0.6115 | 700.0 | 537.2 | |
| 1.20 | 33.51 | 0.73 | 20.38 | 17.97 | 224.53 | 31.97 | 300.07 | 0.5841 | -655.4 | -409.4 | |
| 5.73 | -3.00 | 3.48 | -3.00 | 17.76 | 224.42 | 31.85 | 299.81 | 0.5814 | -925.4 | 999999 | |
| 1.80 | -3.00 | 1.09 | -3.00 | 18.07 | 224.44 | 31.88 | 300.28 | 0.5836 | -697.8 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.15 | 14.18 | 223.75 | 31.18 | 294.38 | 0.5533 | 712.0 | 630.0 | |
| 0.00 | 1.88 | 0.00 | 1.14 | 17.45 | 223.99 | 31.42 | 299.62 | 0.5744 | -918.0 | -801.6 | |
| 0.00 | 1.54 | 0.00 | 0.93 | 18.10 | 224.05 | 31.48 | 300.61 | 0.5789 | -581.0 | -419.4 | |
| 0.00 | 2.05 | 0.00 | 1.24 | 17.83 | 223.85 | 31.28 | 300.31 | 0.5748 | -841.0 | -723.9 | |
| 0.00 | 1.62 | 0.00 | 0.98 | 17.46 | 223.70 | 31.13 | 299.83 | 0.5708 | -395.0 | -407.6 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 15.44 | 223.23 | 30.67 | 296.83 | 0.5531 | 510.0 | 393.9 | |
| 0.00 | 1.88 | 0.00 | 1.13 | 17.43 | 223.48 | 30.91 | 299.94 | 0.5678 | -460.0 | -458.7 | |
| 20.43 | 67.37 | 12.33 | 40.65 | 18.20 | 223.59 | 31.02 | 301.08 | 0.5739 | -1004.9 | -375.3 | |
| 0.00 | 3.59 | 0.00 | 2.13 | 16.20 | 223.08 | 30.51 | 298.22 | 0.5555 | -18.0 | 0.6 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 15.16 | 222.87 | 30.30 | 296.61 | 0.5469 | 760.0 | 616.5 | |
| 0.00 | 1.97 | 0.00 | 1.14 | 16.78 | 220.66 | 28.09 | 301.00 | 0.5281 | 688.0 | 535.5 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 17.67 | 220.25 | 27.68 | 302.86 | 0.5290 | 793.0 | 569.5 | |
| 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. | |