SDO HMI 2014-05-19 00:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.01 | 246.92 | 22.94 | 141.49 | -24.39 | 190.94 | 21.13 | 220.85 | 0.5040 | 650.0 | 346.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.44 | 228.20 | 0.82 | 130.91 | -23.89 | 191.42 | 21.62 | 222.20 | 0.5034 | 978.1 | 404.0 | |
| 36.95 | -1.00 | 21.20 | -1.00 | -24.32 | 191.25 | 21.44 | 221.36 | 0.5061 | 1173.1 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -23.38 | 190.45 | 20.64 | 221.72 | 0.4882 | 271.0 | 224.5 | |
| 1.62 | -1.00 | 0.92 | -1.00 | -24.03 | 190.48 | 20.68 | 220.81 | 0.4955 | 975.6 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.84 | -26.58 | 190.58 | 20.77 | 217.44 | 0.5239 | 125.0 | 189.8 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -24.11 | 190.04 | 20.23 | 220.12 | 0.4918 | 746.0 | 687.0 | |
| 0.00 | 1.44 | 0.00 | 0.82 | -24.24 | 189.88 | 20.07 | 219.72 | 0.4917 | 620.0 | 558.9 | |
| 0.00 | 1.80 | 0.00 | 1.03 | -25.09 | 189.67 | 19.86 | 218.24 | 0.4991 | 748.0 | 479.0 | |
| 0.00 | 1.62 | 0.00 | 0.90 | -23.74 | 187.28 | 17.47 | 216.74 | 0.4613 | -547.0 | -493.1 | |
| 0.00 | 2.16 | 0.00 | 1.21 | -25.79 | 186.06 | 16.26 | 212.16 | 0.4755 | -822.0 | -610.7 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -24.51 | 185.89 | 16.08 | 213.54 | 0.4581 | -794.0 | -562.9 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -27.13 | 185.97 | 16.17 | 210.42 | 0.4915 | -694.0 | -554.8 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -24.74 | 185.61 | 15.80 | 212.78 | 0.4586 | -774.0 | -627.2 | |
| 0.00 | 1.53 | 0.00 | 0.86 | -26.33 | 185.37 | 15.56 | 210.42 | 0.4767 | -951.0 | -808.9 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -27.50 | 185.35 | 15.55 | 209.05 | 0.4915 | -260.0 | -473.5 | |
| 0.00 | 2.34 | 0.00 | 1.33 | -27.37 | 185.30 | 15.49 | 209.12 | 0.4894 | -878.0 | -710.7 | |
| 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. | |