SDO HMI 2014-08-02 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.93 | 117.37 | 34.55 | 252.75 | 9.08 | 172.36 | -77.27 | 82.03 | 0.9731 | 178.2 | 52.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 1.13 | 11.14 | 179.81 | -69.82 | 80.29 | 0.9358 | 199.0 | 117.2 | |
| 0.00 | 0.27 | 0.00 | 0.36 | 7.82 | 180.92 | -68.70 | 83.91 | 0.9299 | -272.0 | -260.7 | |
| 2.08 | 12.76 | 3.16 | 19.26 | 10.16 | 177.95 | -71.67 | 81.25 | 0.9468 | -572.0 | -456.8 | |
| 0.00 | 1.18 | 0.00 | 2.02 | 10.39 | 175.58 | -74.05 | 80.88 | 0.9591 | 183.0 | 160.9 | |
| 0.00 | 0.81 | 0.00 | 1.59 | 11.03 | 173.53 | -76.10 | 80.10 | 0.9683 | 278.0 | 307.0 | |
| 0.00 | 0.63 | 0.00 | 1.23 | 10.72 | 173.51 | -76.12 | 80.42 | 0.9684 | 436.0 | 393.4 | |
| 0.00 | 1.09 | 0.00 | 2.20 | 11.31 | 172.89 | -76.73 | 79.78 | 0.9709 | 109.0 | 94.8 | |
| 0.00 | 7.78 | 0.00 | 14.94 | 9.24 | 173.91 | -75.72 | 81.98 | 0.9671 | 436.0 | 426.2 | |
| 0.00 | 1.99 | 0.00 | 4.32 | 11.41 | 171.95 | -77.68 | 79.63 | 0.9746 | 418.0 | 356.9 | |
| 0.00 | 6.70 | 0.00 | 13.61 | 8.72 | 173.06 | -76.57 | 82.45 | 0.9709 | 485.0 | 390.0 | |
| 0.00 | 1.54 | 0.00 | 3.37 | 9.02 | 172.01 | -77.62 | 82.07 | 0.9750 | 370.0 | 405.5 | |
| 3.53 | 36.20 | 7.62 | 82.53 | 8.60 | 172.16 | -77.47 | 82.51 | 0.9745 | 438.2 | 58.0 | |
| 6.24 | 45.61 | 14.22 | 106.19 | 9.21 | 171.42 | -78.21 | 81.84 | 0.9771 | 286.5 | -14.1 | |
| 3.08 | -12.00 | 7.16 | -12.00 | 8.33 | 171.30 | -78.33 | 82.73 | 0.9778 | 26.9 | 999999 | |
| 1.00 | -13.00 | 2.39 | -13.00 | 8.78 | 170.80 | -78.82 | 82.23 | 0.9794 | -209.4 | 999999 | |
| 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. | |