| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.15 | 386.48 | 28.77 | 221.48 | 16.11 | 64.05 | 27.70 | 297.45 | 0.5054 | -909.2 | -371.5 | |
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back to the solar disc SDO HMI 2011-11-13 12:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.29 | 371.50 | 0.74 | 213.10 | 15.79 | 64.66 | 28.31 | 296.40 | 0.5115 | -887.4 | -388.2 | |
| 47.57 | -1.00 | 27.30 | -1.00 | 16.05 | 64.24 | 27.89 | 297.16 | 0.5073 | -1322.3 | 999999 | |
| 0.00 | 1.98 | 0.00 | 1.15 | 18.80 | 64.67 | 28.32 | 301.69 | 0.5299 | -801.0 | -572.6 | |
| 0.69 | -1.00 | 0.39 | -1.00 | 15.72 | 63.88 | 27.53 | 296.82 | 0.5006 | -1286.2 | 999999 | |
| 0.60 | -1.00 | 0.34 | -1.00 | 15.88 | 63.73 | 27.38 | 297.23 | 0.4994 | -1277.3 | 999999 | |
| 0.00 | 2.24 | 0.00 | 1.25 | 14.06 | 62.35 | 25.99 | 294.74 | 0.4701 | -919.0 | -784.9 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 18.81 | 63.01 | 26.66 | 303.09 | 0.5090 | -719.0 | -568.0 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 17.04 | 62.21 | 25.85 | 300.61 | 0.4864 | -609.0 | -563.8 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 17.44 | 62.23 | 25.88 | 301.33 | 0.4895 | -747.0 | -589.7 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 18.76 | 59.75 | 23.40 | 306.15 | 0.4676 | 709.0 | 562.3 | |
| 0.00 | 1.38 | 0.00 | 0.76 | 17.90 | 57.91 | 21.55 | 306.60 | 0.4373 | 855.0 | 655.8 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 16.48 | 56.97 | 20.62 | 304.87 | 0.4133 | 851.0 | 725.8 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 22.03 | 56.11 | 19.76 | 316.31 | 0.4555 | 645.0 | 415.5 | |
| 0.00 | 2.15 | 0.00 | 1.19 | 21.09 | 55.84 | 19.49 | 315.11 | 0.4429 | 821.0 | 659.4 | |
| 0.00 | 0.77 | 0.00 | 0.42 | 20.67 | 54.81 | 18.46 | 315.85 | 0.4271 | 750.0 | 550.7 | |
| 0.00 | 0.43 | 0.00 | 0.23 | 21.03 | 54.12 | 17.77 | 317.50 | 0.4234 | 532.0 | 554.0 | |
| 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. | |