SDO HMI 2014-09-29 19:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.86 | 216.86 | 29.42 | 163.34 | -1.30 | 152.38 | -48.30 | 97.72 | 0.7554 | 624.3 | 333.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.08 | 186.20 | 19.47 | 139.15 | -1.29 | 152.82 | -47.86 | 97.81 | 0.7506 | 1095.2 | 372.7 | |
| 3.61 | -1.00 | 2.72 | -1.00 | -1.77 | 152.53 | -48.15 | 98.37 | 0.7548 | 721.9 | 999999 | |
| 0.97 | -1.00 | 0.73 | -1.00 | -1.04 | 152.51 | -48.17 | 97.41 | 0.7536 | 622.8 | 999999 | |
| 0.00 | 1.41 | 0.00 | 1.06 | 1.35 | 151.87 | -48.81 | 94.14 | 0.7566 | 294.0 | 312.8 | |
| 2.47 | 7.93 | 1.90 | 6.10 | -0.70 | 151.28 | -49.40 | 96.69 | 0.7667 | 667.4 | 448.2 | |
| 0.00 | 0.97 | 0.00 | 0.75 | -1.74 | 151.21 | -49.48 | 98.01 | 0.7696 | 289.0 | 284.9 | |
| 0.00 | 1.06 | 0.00 | 0.81 | -0.05 | 151.10 | -49.58 | 95.81 | 0.7675 | 490.0 | 379.1 | |
| 0.00 | 1.41 | 0.00 | 1.10 | -2.05 | 150.73 | -49.96 | 98.30 | 0.7754 | 429.0 | 408.5 | |
| 0.00 | 1.06 | 0.00 | 0.82 | -0.32 | 150.77 | -49.91 | 96.10 | 0.7716 | 250.0 | 197.2 | |
| 0.00 | 1.67 | 0.00 | 1.32 | -0.51 | 150.06 | -50.62 | 96.19 | 0.7797 | -242.0 | -228.6 | |
| 0.00 | 1.85 | 0.00 | 1.47 | -2.09 | 150.01 | -50.67 | 98.18 | 0.7832 | -240.0 | -210.7 | |
| 5.73 | 11.63 | 4.60 | 9.35 | -1.09 | 149.28 | -51.40 | 96.77 | 0.7891 | -517.6 | -317.5 | |
| 0.00 | 0.88 | 0.00 | 0.74 | -3.50 | 147.92 | -52.76 | 99.43 | 0.8077 | -478.0 | -361.9 | |
| 0.00 | 0.79 | 0.00 | 0.67 | -3.33 | 147.53 | -53.15 | 99.13 | 0.8113 | 564.0 | 475.1 | |
| 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. | |