SDO HMI 2014-10-07 06:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.36 | 145.98 | 37.61 | 179.47 | -12.37 | 165.97 | 63.71 | 253.38 | 0.9148 | 222.1 | 38.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.95 | 115.59 | 21.66 | 147.96 | -12.52 | 167.12 | 64.86 | 253.51 | 0.9233 | 535.1 | 76.6 | |
| 5.53 | -1.00 | 6.89 | -1.00 | -12.12 | 166.57 | 64.31 | 253.81 | 0.9192 | 737.5 | 999999 | |
| 0.00 | 1.67 | 0.00 | 2.04 | -12.01 | 166.10 | 63.84 | 253.82 | 0.9159 | 589.0 | 458.7 | |
| 0.53 | 2.72 | 0.64 | 3.28 | -12.03 | 165.69 | 63.43 | 253.70 | 0.9131 | 687.2 | 530.4 | |
| 0.00 | 1.41 | 0.00 | 1.60 | -13.86 | 163.61 | 61.35 | 251.21 | 0.9018 | -336.0 | -279.3 | |
| 0.00 | 0.97 | 0.00 | 1.03 | -11.68 | 162.29 | 60.03 | 253.22 | 0.8879 | 311.0 | 239.9 | |
| 0.00 | 0.97 | 0.00 | 1.04 | -12.26 | 162.44 | 60.18 | 252.63 | 0.8902 | 74.0 | 201.0 | |
| 0.00 | 1.14 | 0.00 | 1.18 | -11.50 | 161.13 | 58.87 | 253.11 | 0.8786 | -248.0 | -207.4 | |
| 5.36 | 8.78 | 5.45 | 8.94 | -11.62 | 160.76 | 58.50 | 252.88 | 0.8758 | -632.4 | -451.4 | |
| 0.00 | 1.23 | 0.00 | 1.24 | -11.95 | 160.22 | 57.96 | 252.37 | 0.8722 | -344.0 | -318.6 | |
| 2.99 | 5.18 | 2.97 | 5.16 | -11.98 | 159.88 | 57.62 | 252.24 | 0.8695 | -571.7 | -396.1 | |
| 0.00 | 1.58 | 0.00 | 1.51 | -12.33 | 158.36 | 56.10 | 251.40 | 0.8576 | -423.0 | -363.5 | |
| 0.00 | 2.81 | 0.00 | 2.66 | -12.47 | 157.86 | 55.59 | 251.09 | 0.8537 | -630.0 | -548.5 | |
| 0.00 | 1.93 | 0.00 | 1.83 | -13.31 | 157.76 | 55.49 | 250.11 | 0.8549 | -608.0 | -485.9 | |
| 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. | |