SDO HMI 2014-05-13 18:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.73 | 62.95 | 27.50 | 64.47 | 10.59 | 179.45 | -59.82 | 76.25 | 0.8765 | 81.1 | 137.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.28 | 30.49 | 6.17 | 30.07 | 10.32 | 180.73 | -58.54 | 76.31 | 0.8657 | -526.9 | 9.5 | |
| 6.55 | -1.00 | 6.44 | -1.00 | 9.95 | 180.66 | -58.61 | 76.74 | 0.8658 | -488.8 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.91 | 9.87 | 179.72 | -59.55 | 77.01 | 0.8736 | 255.0 | 234.1 | |
| 0.00 | 1.08 | 0.00 | 1.11 | 11.13 | 179.25 | -60.01 | 75.67 | 0.8791 | 359.0 | 293.2 | |
| 0.00 | 1.61 | 0.00 | 1.67 | 10.92 | 179.20 | -60.07 | 75.92 | 0.8792 | 301.0 | 358.9 | |
| 0.00 | 1.43 | 0.00 | 1.49 | 11.36 | 179.05 | -60.22 | 75.45 | 0.8810 | 272.0 | 221.9 | |
| 0.00 | 1.52 | 0.00 | 1.61 | 11.32 | 178.62 | -60.64 | 75.58 | 0.8844 | 397.0 | 462.6 | |
| 2.78 | 20.81 | 2.94 | 22.27 | 11.08 | 178.45 | -60.81 | 75.88 | 0.8854 | 594.6 | 373.6 | |
| 0.00 | 1.26 | 0.00 | 1.29 | 9.31 | 179.01 | -60.25 | 77.76 | 0.8786 | 284.0 | 199.8 | |
| 0.00 | 1.79 | 0.00 | 1.87 | 9.64 | 178.73 | -60.53 | 77.44 | 0.8813 | -438.0 | -251.4 | |
| 7.62 | -8.00 | 8.19 | -8.00 | 11.41 | 178.01 | -61.26 | 75.59 | 0.8893 | 528.4 | 999999 | |
| 3.50 | -8.00 | 3.76 | -8.00 | 11.10 | 177.93 | -61.34 | 75.94 | 0.8895 | 473.4 | 999999 | |
| 0.00 | 2.06 | 0.00 | 2.18 | 10.15 | 178.25 | -61.01 | 76.94 | 0.8858 | -6.0 | 72.3 | |
| 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. | |