| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.21 | 98.41 | 24.20 | 72.80 | 19.95 | 64.36 | 40.44 | 304.88 | 0.7448 | 155.9 | 306.0 | |
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back to the solar disc SDO HMI 2011-02-14 21:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.79 | 25.78 | 10.88 | 20.37 | 19.31 | 68.55 | 44.63 | 301.61 | 0.7807 | -706.1 | -196.9 | |
| 0.00 | 0.34 | 0.00 | 0.27 | 19.04 | 68.15 | 44.23 | 301.52 | 0.7757 | -640.0 | -674.2 | |
| 0.00 | 0.77 | 0.00 | 0.60 | 20.94 | 67.32 | 43.40 | 304.15 | 0.7778 | -441.0 | -366.6 | |
| 0.00 | 0.94 | 0.00 | 0.70 | 18.84 | 65.76 | 41.84 | 302.64 | 0.7520 | 553.0 | 441.7 | |
| 0.00 | 0.86 | 0.00 | 0.64 | 18.66 | 65.58 | 41.66 | 302.53 | 0.7493 | 592.0 | 487.5 | |
| 0.00 | 2.23 | 0.00 | 1.62 | 19.27 | 63.85 | 39.93 | 304.31 | 0.7360 | 676.0 | 572.2 | |
| 0.00 | 1.03 | 0.00 | 0.75 | 19.97 | 63.57 | 39.65 | 305.32 | 0.7374 | 415.0 | 412.0 | |
| 1.46 | 3.00 | 1.09 | 2.24 | 21.88 | 63.81 | 39.89 | 307.37 | 0.7511 | -501.2 | -467.3 | |
| 1.54 | 56.61 | 1.12 | 40.77 | 19.93 | 63.03 | 39.11 | 305.62 | 0.7319 | 544.1 | 465.6 | |
| 5.57 | -9.00 | 4.00 | -9.00 | 19.77 | 62.69 | 38.77 | 305.66 | 0.7277 | 1000.6 | 999999 | |
| 9.85 | -9.00 | 7.11 | -9.00 | 20.16 | 62.69 | 38.77 | 306.13 | 0.7301 | 760.5 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.80 | 21.04 | 61.62 | 37.70 | 307.88 | 0.7255 | 309.0 | 407.7 | |
| 0.00 | 2.31 | 0.00 | 1.68 | 23.24 | 61.06 | 37.14 | 310.79 | 0.7351 | 711.0 | 555.1 | |
| 0.00 | 2.23 | 0.00 | 1.54 | 20.52 | 59.57 | 35.65 | 308.76 | 0.7024 | 734.0 | 576.6 | |
| 0.00 | 1.20 | 0.00 | 0.82 | 21.50 | 57.98 | 34.06 | 311.15 | 0.6943 | 633.0 | 477.3 | |
| 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. | |