| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.72 | 74.73 | 15.31 | 44.42 | -17.91 | 161.23 | 23.47 | 223.21 | 0.5562 | 492.1 | 409.9 | |
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back to the solar disc SDO HMI 2014-08-11 01:00:39 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.55 | -18.88 | 163.97 | 26.21 | 225.09 | 0.5923 | 644.0 | 542.8 | |
| 21.39 | 47.75 | 12.74 | 28.39 | -17.22 | 162.12 | 24.36 | 225.18 | 0.5576 | 887.4 | 563.7 | |
| 0.00 | 1.99 | 0.00 | 1.19 | -18.48 | 161.46 | 23.70 | 222.76 | 0.5637 | 402.0 | 358.7 | |
| 2.62 | 3.97 | 1.56 | 2.37 | -18.85 | 160.81 | 23.06 | 221.52 | 0.5613 | 811.5 | 684.7 | |
| 0.00 | 1.17 | 0.00 | 0.70 | -18.80 | 160.49 | 22.74 | 221.19 | 0.5577 | 845.0 | 682.5 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -17.42 | 160.20 | 22.45 | 222.59 | 0.5404 | -596.0 | -475.6 | |
| 0.00 | 2.80 | 0.00 | 1.68 | -19.90 | 160.13 | 22.37 | 219.41 | 0.5659 | 570.0 | 486.7 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -19.43 | 159.57 | 21.82 | 219.27 | 0.5558 | 669.0 | 689.3 | |
| 0.00 | 2.17 | 0.00 | 1.28 | -19.12 | 159.29 | 21.53 | 219.29 | 0.5498 | 740.0 | 673.1 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -19.32 | 159.28 | 21.52 | 219.03 | 0.5519 | 593.0 | 514.1 | |
| 1.35 | 2.98 | 0.79 | 1.74 | -17.69 | 158.76 | 21.00 | 220.38 | 0.5292 | -488.3 | -298.6 | |
| 0.00 | 3.25 | 0.00 | 1.90 | -18.45 | 158.61 | 20.86 | 219.22 | 0.5362 | 589.0 | 695.3 | |
| 0.36 | 1.90 | 0.22 | 1.14 | -21.51 | 158.87 | 21.11 | 215.98 | 0.5725 | -746.8 | -606.9 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -19.84 | 158.14 | 20.39 | 216.92 | 0.5475 | -554.0 | -384.6 | |
| 0.00 | 1.26 | 0.00 | 0.75 | -20.01 | 158.10 | 20.34 | 216.67 | 0.5490 | -671.0 | -457.7 | |
| 0.00 | 1.62 | 0.00 | 0.97 | -20.58 | 157.93 | 20.17 | 215.80 | 0.5541 | -573.0 | -460.5 | |
| 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. | |