SDO HMI 2014-02-24 19:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.30 | 128.95 | 26.27 | 119.12 | 8.23 | 132.58 | -55.42 | 75.41 | 0.8437 | 357.2 | 115.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.06 | 0.00 | 1.54 | 7.34 | 141.68 | -46.31 | 73.54 | 0.7502 | -734.0 | -532.9 | |
| 0.00 | 1.72 | 0.00 | 1.32 | 8.18 | 140.55 | -47.45 | 72.90 | 0.7652 | -707.0 | -607.0 | |
| 0.00 | 0.60 | 0.00 | 0.46 | 8.49 | 140.45 | -47.54 | 72.54 | 0.7673 | -603.0 | -531.0 | |
| 0.00 | 2.15 | 0.00 | 1.71 | 9.18 | 139.07 | -48.93 | 72.21 | 0.7840 | -563.0 | -435.2 | |
| 0.00 | 0.95 | 0.00 | 0.75 | 8.87 | 139.03 | -48.97 | 72.59 | 0.7834 | -588.0 | -560.0 | |
| 0.00 | 1.03 | 0.00 | 0.82 | 8.72 | 138.73 | -49.26 | 72.89 | 0.7860 | -419.0 | -320.2 | |
| 0.00 | 1.38 | 0.00 | 1.21 | 7.01 | 133.88 | -54.12 | 76.48 | 0.8293 | -526.0 | -415.2 | |
| 7.66 | 110.81 | 7.10 | 103.75 | 8.85 | 132.36 | -55.64 | 74.78 | 0.8474 | 862.3 | 179.1 | |
| 3.01 | -8.00 | 2.75 | -8.00 | 7.66 | 132.61 | -55.39 | 76.08 | 0.8425 | 701.9 | 999999 | |
| 1.72 | 4.90 | 1.56 | 4.45 | 6.83 | 132.71 | -55.29 | 77.01 | 0.8398 | -278.4 | 67.0 | |
| 1.03 | -8.00 | 0.95 | -8.00 | 7.84 | 132.36 | -55.64 | 75.94 | 0.8451 | 706.8 | 999999 | |
| 14.11 | -8.00 | 13.20 | -8.00 | 8.23 | 131.85 | -56.15 | 75.63 | 0.8506 | 631.1 | 999999 | |
| 0.77 | 2.75 | 0.71 | 2.54 | 6.92 | 132.11 | -55.89 | 77.07 | 0.8454 | -127.1 | 71.8 | |
| 0.00 | 0.60 | 0.00 | 0.57 | 6.89 | 131.30 | -56.70 | 77.32 | 0.8526 | -149.0 | -109.3 | |
| 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. | |