SDO HMI 2014-05-19 02:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.32 | 44.88 | 10.34 | 34.89 | -18.19 | 217.50 | 48.80 | 248.08 | 0.7726 | -260.1 | -102.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.81 | 2.07 | 0.64 | 1.63 | -17.82 | 218.18 | 49.48 | 248.73 | 0.7788 | 726.0 | 627.1 | |
| 4.23 | 20.59 | 3.34 | 16.28 | -18.38 | 218.35 | 49.64 | 248.06 | 0.7818 | 529.4 | 76.3 | |
| 0.36 | -2.00 | 0.29 | -2.00 | -18.64 | 218.35 | 49.64 | 247.75 | 0.7824 | -452.5 | 999999 | |
| 0.00 | 2.16 | 0.00 | 1.71 | -18.86 | 218.29 | 49.59 | 247.45 | 0.7824 | -507.0 | -415.9 | |
| 1.17 | -2.00 | 0.92 | -2.00 | -18.74 | 218.04 | 49.34 | 247.53 | 0.7796 | -157.4 | 999999 | |
| 0.00 | 1.80 | 0.00 | 1.40 | -18.88 | 217.41 | 48.71 | 247.18 | 0.7736 | -559.0 | -466.3 | |
| 0.00 | 0.90 | 0.00 | 0.70 | -18.66 | 217.28 | 48.58 | 247.42 | 0.7716 | -266.0 | -330.3 | |
| 0.00 | 1.35 | 0.00 | 1.01 | -15.98 | 216.11 | 47.41 | 250.56 | 0.7528 | -563.0 | -518.9 | |
| 5.22 | 8.72 | 4.01 | 6.71 | -18.49 | 216.87 | 48.17 | 247.53 | 0.7670 | -641.4 | -420.7 | |
| 0.45 | 1.44 | 0.34 | 1.08 | -16.61 | 216.12 | 47.42 | 249.74 | 0.7544 | -421.6 | -390.5 | |
| 0.54 | 3.15 | 0.40 | 2.36 | -16.90 | 215.79 | 47.09 | 249.27 | 0.7516 | -222.0 | 60.7 | |
| 0.00 | 1.26 | 0.00 | 0.94 | -17.19 | 215.75 | 47.05 | 248.89 | 0.7518 | -445.0 | -282.7 | |
| 0.54 | 1.44 | 0.40 | 1.07 | -17.42 | 215.40 | 46.70 | 248.49 | 0.7487 | -533.5 | -505.0 | |
| 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. | |