| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.29 | 380.76 | 31.00 | 216.96 | 16.16 | 63.85 | 26.95 | 298.19 | 0.4959 | -799.8 | -341.4 | |
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back to the solar disc SDO HMI 2011-11-13 11:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.95 | 0.00 | 0.58 | 21.18 | 68.42 | 31.51 | 303.14 | 0.5843 | -505.0 | -335.1 | |
| 52.91 | 355.72 | 30.22 | 203.10 | 16.03 | 64.23 | 27.33 | 297.55 | 0.4997 | -1313.8 | -392.8 | |
| 0.00 | 1.81 | 0.00 | 1.05 | 18.82 | 64.65 | 27.75 | 302.17 | 0.5228 | -791.0 | -576.2 | |
| 1.38 | -2.00 | 0.78 | -2.00 | 15.96 | 63.56 | 26.66 | 297.92 | 0.4902 | -1067.4 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 14.19 | 62.61 | 25.70 | 295.22 | 0.4667 | -682.0 | -511.9 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 14.10 | 62.39 | 25.49 | 295.21 | 0.4632 | -913.0 | -811.4 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 17.09 | 62.17 | 25.27 | 301.21 | 0.4791 | -648.0 | -601.2 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 11.02 | 61.40 | 24.50 | 289.38 | 0.4332 | 684.0 | 566.6 | |
| 0.00 | 3.96 | 0.00 | 2.20 | 17.91 | 59.70 | 22.80 | 305.21 | 0.4531 | 522.0 | 482.6 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 18.71 | 59.74 | 22.84 | 306.66 | 0.4602 | 804.0 | 645.4 | |
| 0.00 | 3.27 | 0.00 | 1.79 | 17.88 | 57.78 | 20.88 | 307.38 | 0.4286 | 841.0 | 659.3 | |
| 0.00 | 2.06 | 0.00 | 1.12 | 16.46 | 56.92 | 20.02 | 305.57 | 0.4053 | 793.0 | 669.0 | |
| 0.00 | 1.63 | 0.00 | 0.89 | 18.39 | 56.74 | 19.84 | 309.70 | 0.4204 | 644.0 | 571.6 | |
| 0.00 | 1.81 | 0.00 | 0.99 | 21.08 | 55.81 | 18.91 | 315.88 | 0.4363 | 820.0 | 642.0 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 20.66 | 54.79 | 17.89 | 316.67 | 0.4206 | 830.0 | 639.9 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 22.75 | 54.96 | 18.06 | 319.89 | 0.4456 | 683.0 | 644.7 | |
| 0.00 | 3.10 | 0.00 | 1.65 | 20.06 | 50.39 | 13.48 | 323.29 | 0.3680 | 665.0 | 501.0 | |
| 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. | |