| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.46 | 177.63 | 37.95 | 111.41 | 33.98 | 267.87 | 8.65 | 348.26 | 0.6160 | -18.9 | -40.3 | |
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back to the solar disc SDO HMI 2010-12-31 16:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.44 | 105.89 | 0.91 | 66.48 | 33.93 | 270.02 | 10.80 | 345.45 | 0.6213 | -515.3 | -316.8 | |
| 27.60 | -1.00 | 17.32 | -1.00 | 33.70 | 269.52 | 10.30 | 345.98 | 0.6166 | -1108.7 | 999999 | |
| 0.00 | 1.78 | 0.00 | 1.12 | 33.95 | 268.54 | 9.32 | 347.37 | 0.6168 | -688.0 | -533.0 | |
| 0.93 | 1.61 | 0.59 | 1.02 | 34.28 | 268.36 | 9.15 | 347.74 | 0.6207 | -553.9 | -630.4 | |
| 0.00 | 0.51 | 0.00 | 0.32 | 34.69 | 268.08 | 8.86 | 348.27 | 0.6253 | -454.0 | -435.7 | |
| 0.00 | 1.36 | 0.00 | 0.84 | 33.09 | 266.88 | 7.67 | 349.23 | 0.6005 | 793.0 | 537.0 | |
| 0.00 | 2.72 | 0.00 | 1.68 | 33.31 | 266.55 | 7.33 | 349.77 | 0.6027 | 550.0 | 389.3 | |
| 0.00 | 2.55 | 0.00 | 1.58 | 33.56 | 266.07 | 6.85 | 350.51 | 0.6050 | 690.0 | 504.4 | |
| 1.87 | 6.62 | 1.18 | 4.19 | 35.01 | 265.39 | 6.17 | 351.84 | 0.6231 | 680.5 | 620.1 | |
| 0.00 | 1.53 | 0.00 | 0.95 | 33.45 | 265.24 | 6.02 | 351.60 | 0.6016 | 768.0 | 502.8 | |
| 0.00 | 1.10 | 0.00 | 0.70 | 35.42 | 265.35 | 6.13 | 352.01 | 0.6286 | 450.0 | 396.5 | |
| 2.04 | -9.00 | 1.29 | -9.00 | 35.12 | 265.22 | 6.00 | 352.10 | 0.6243 | 795.3 | 999999 | |
| 21.57 | 49.42 | 13.50 | 30.92 | 34.33 | 265.09 | 5.87 | 352.05 | 0.6134 | 947.2 | 620.0 | |
| 1.27 | 1.44 | 0.81 | 0.91 | 35.30 | 265.05 | 5.83 | 352.36 | 0.6265 | 578.9 | 560.0 | |
| 0.00 | 1.10 | 0.00 | 0.70 | 35.57 | 265.03 | 5.82 | 352.45 | 0.6300 | 414.0 | 307.4 | |
| 3.74 | -13.00 | 2.35 | -13.00 | 34.81 | 264.76 | 5.55 | 352.61 | 0.6194 | 647.4 | 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. | |