SDO HMI 2014-11-13 15:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.48 | 44.22 | 11.05 | 26.53 | 8.69 | 3.45 | 34.08 | 281.03 | 0.5665 | 144.4 | -261.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.46 | 4.13 | 0.90 | 2.55 | 8.27 | 5.84 | 36.47 | 279.79 | 0.5992 | -802.3 | -591.5 | |
| 1.20 | 2.67 | 0.74 | 1.63 | 8.32 | 5.18 | 35.81 | 280.00 | 0.5901 | -799.9 | -669.1 | |
| 0.86 | 1.98 | 0.52 | 1.20 | 7.95 | 4.66 | 35.29 | 279.46 | 0.5823 | -772.0 | -616.3 | |
| 0.00 | 1.46 | 0.00 | 0.89 | 8.43 | 4.71 | 35.34 | 280.26 | 0.5837 | -517.0 | -508.7 | |
| 0.00 | 4.73 | 0.00 | 2.87 | 8.17 | 4.32 | 34.94 | 279.90 | 0.5777 | -563.0 | -719.1 | |
| 2.49 | 9.38 | 1.51 | 5.66 | 8.30 | 4.00 | 34.63 | 280.19 | 0.5735 | -910.8 | -700.3 | |
| 1.72 | -6.00 | 1.04 | -6.00 | 8.54 | 3.84 | 34.47 | 280.64 | 0.5717 | -756.2 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.47 | 9.36 | 3.60 | 34.23 | 282.12 | 0.5699 | 444.0 | 339.7 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 8.14 | 3.22 | 33.85 | 280.07 | 0.5622 | 301.0 | 303.6 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 10.07 | 2.60 | 33.23 | 283.66 | 0.5574 | 496.0 | 468.1 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 9.09 | 2.38 | 33.01 | 281.96 | 0.5520 | 280.0 | 363.2 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 9.43 | 2.27 | 32.90 | 282.59 | 0.5512 | 360.0 | 417.6 | |
| 1.55 | 2.92 | 0.92 | 1.73 | 9.78 | 2.28 | 32.91 | 283.23 | 0.5521 | 617.6 | 523.1 | |
| 9.20 | 12.22 | 5.42 | 7.19 | 9.05 | 1.70 | 32.33 | 282.07 | 0.5422 | 943.8 | 636.2 | |
| 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. | |