SDO HMI 2014-07-10 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.35 | 29.08 | 2.73 | 23.71 | 7.83 | 252.07 | 52.66 | 276.95 | 0.7954 | 211.7 | 171.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.82 | 0.00 | 0.74 | 6.92 | 256.19 | 56.78 | 275.77 | 0.8368 | -336.0 | -325.0 | |
| 0.54 | 2.27 | 0.48 | 1.99 | 7.10 | 255.17 | 55.76 | 275.99 | 0.8270 | -581.2 | -537.7 | |
| 0.00 | 0.73 | 0.00 | 0.64 | 7.62 | 255.21 | 55.80 | 276.61 | 0.8274 | -398.0 | -395.8 | |
| 0.00 | 0.64 | 0.00 | 0.55 | 6.17 | 254.79 | 55.38 | 274.86 | 0.8232 | -454.0 | -433.1 | |
| 0.00 | 1.91 | 0.00 | 1.66 | 8.07 | 254.92 | 55.51 | 277.16 | 0.8246 | -623.0 | -532.6 | |
| 2.00 | 4.18 | 1.60 | 3.34 | 7.25 | 251.31 | 51.91 | 276.21 | 0.7875 | 717.8 | 496.8 | |
| 0.00 | 1.45 | 0.00 | 1.16 | 7.04 | 251.28 | 51.87 | 275.94 | 0.7871 | 540.0 | 413.4 | |
| 0.00 | 3.00 | 0.00 | 2.41 | 8.93 | 251.47 | 52.07 | 278.34 | 0.7897 | 591.0 | 446.8 | |
| 0.45 | 10.99 | 0.36 | 8.78 | 8.30 | 251.15 | 51.74 | 277.56 | 0.7860 | 511.0 | 299.5 | |
| 0.00 | 0.54 | 0.00 | 0.44 | 8.89 | 251.16 | 51.75 | 278.30 | 0.7864 | 406.0 | 449.5 | |
| 0.36 | -9.00 | 0.29 | -9.00 | 8.31 | 250.95 | 51.54 | 277.58 | 0.7839 | 726.5 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.72 | 8.53 | 250.89 | 51.49 | 277.86 | 0.7834 | 602.0 | 518.1 | |
| 0.00 | 0.82 | 0.00 | 0.64 | 6.01 | 250.44 | 51.03 | 274.63 | 0.7779 | 472.0 | 401.0 | |
| 0.00 | 0.82 | 0.00 | 0.64 | 6.45 | 250.11 | 50.70 | 275.21 | 0.7743 | 610.0 | 524.9 | |
| 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. | |