| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.72 | 39.70 | 11.23 | 30.39 | -23.26 | 94.91 | -44.40 | 122.53 | 0.7645 | -11.2 | 104.3 | |
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back to the solar disc SDO HMI 2014-11-28 01:00:25 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.94 | 5.82 | 2.91 | 4.31 | -23.27 | 96.85 | -42.47 | 123.48 | 0.7460 | 824.8 | 554.8 | |
| 0.00 | 2.48 | 0.00 | 1.84 | -23.01 | 96.64 | -42.67 | 123.06 | 0.7467 | 466.0 | 361.2 | |
| 3.17 | 10.27 | 2.38 | 7.73 | -23.93 | 96.18 | -43.13 | 123.94 | 0.7556 | 819.9 | 565.8 | |
| 0.00 | 1.28 | 0.00 | 0.96 | -23.51 | 96.09 | -43.22 | 123.39 | 0.7545 | 801.0 | 579.9 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -23.82 | 95.38 | -43.93 | 123.40 | 0.7626 | 232.0 | 329.7 | |
| 0.00 | 0.68 | 0.00 | 0.52 | -23.17 | 94.88 | -44.43 | 122.39 | 0.7644 | 264.0 | 224.4 | |
| 0.00 | 1.03 | 0.00 | 0.79 | -23.80 | 94.57 | -44.74 | 122.98 | 0.7702 | 181.0 | 191.6 | |
| 5.13 | 6.93 | 3.97 | 5.36 | -23.22 | 94.23 | -45.08 | 122.13 | 0.7708 | -757.9 | -541.8 | |
| 0.00 | 1.28 | 0.00 | 1.01 | -22.84 | 93.19 | -46.12 | 121.21 | 0.7790 | -153.0 | -233.3 | |
| 2.48 | 5.39 | 1.97 | 4.29 | -23.14 | 92.73 | -46.58 | 121.37 | 0.7845 | -597.2 | -424.8 | |
| 0.00 | 1.37 | 0.00 | 1.05 | -20.94 | 93.58 | -45.74 | 119.08 | 0.7676 | -681.0 | -527.6 | |
| 0.00 | 1.20 | 0.00 | 0.95 | -22.56 | 92.80 | -46.51 | 120.70 | 0.7815 | -461.0 | -291.1 | |
| 0.00 | 0.94 | 0.00 | 0.74 | -21.24 | 92.81 | -46.50 | 119.12 | 0.7762 | -533.0 | -413.7 | |
| 0.00 | 0.77 | 0.00 | 0.64 | -23.73 | 90.77 | -48.54 | 121.23 | 0.8046 | -519.0 | -395.3 | |
| 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. | |