SDO HMI 2014-07-10 02:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.54 | 35.60 | 4.33 | 28.32 | 7.87 | 252.10 | 51.59 | 277.03 | 0.7841 | 317.6 | 171.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 1.19 | 6.92 | 256.11 | 55.60 | 275.77 | 0.8254 | -408.0 | -340.3 | |
| 0.00 | 0.64 | 0.00 | 0.54 | 6.81 | 255.27 | 54.77 | 275.64 | 0.8172 | -589.0 | -486.4 | |
| 0.00 | 2.72 | 0.00 | 2.32 | 7.07 | 255.10 | 54.60 | 275.96 | 0.8155 | -621.0 | -557.0 | |
| 0.00 | 2.63 | 0.00 | 2.23 | 8.12 | 254.88 | 54.37 | 277.26 | 0.8133 | -608.0 | -529.8 | |
| 3.00 | 4.72 | 2.34 | 3.69 | 7.27 | 251.31 | 50.81 | 276.27 | 0.7756 | 637.2 | 430.8 | |
| 0.00 | 0.91 | 0.00 | 0.71 | 8.82 | 251.59 | 51.08 | 278.26 | 0.7791 | 419.0 | 318.9 | |
| 0.00 | 0.64 | 0.00 | 0.50 | 8.67 | 251.56 | 51.05 | 278.06 | 0.7787 | 381.0 | 376.0 | |
| 0.00 | 1.27 | 0.00 | 0.99 | 7.06 | 251.23 | 50.72 | 276.00 | 0.7747 | 607.0 | 520.7 | |
| 0.00 | 2.36 | 0.00 | 1.86 | 8.98 | 251.52 | 51.01 | 278.46 | 0.7785 | 591.0 | 463.2 | |
| 1.54 | 9.35 | 1.21 | 7.32 | 8.40 | 251.36 | 50.85 | 277.73 | 0.7765 | 549.7 | 314.8 | |
| 0.00 | 1.18 | 0.00 | 0.93 | 9.41 | 251.56 | 51.05 | 279.01 | 0.7791 | 440.0 | 352.1 | |
| 0.00 | 1.36 | 0.00 | 1.06 | 8.84 | 251.20 | 50.69 | 278.30 | 0.7749 | 502.0 | 509.7 | |
| 1.00 | 2.00 | 0.78 | 1.55 | 8.26 | 251.04 | 50.53 | 277.56 | 0.7730 | 666.7 | 582.9 | |
| 0.00 | 1.09 | 0.00 | 0.85 | 8.51 | 250.94 | 50.43 | 277.90 | 0.7719 | 689.0 | 523.8 | |
| 0.00 | 0.82 | 0.00 | 0.63 | 5.87 | 250.39 | 49.88 | 274.46 | 0.7653 | 508.0 | 450.1 | |
| 0.00 | 1.09 | 0.00 | 0.84 | 6.09 | 250.42 | 49.91 | 274.74 | 0.7656 | 549.0 | 440.2 | |
| 0.00 | 0.82 | 0.00 | 0.62 | 5.95 | 250.16 | 49.65 | 274.56 | 0.7627 | 448.0 | 501.2 | |
| 0.00 | 0.64 | 0.00 | 0.49 | 6.47 | 250.18 | 49.67 | 275.24 | 0.7630 | 555.0 | 490.6 | |
| 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. | |