SDO HMI 2014-05-19 13:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.32 | 245.62 | 22.63 | 148.66 | -24.63 | 190.51 | 27.84 | 227.68 | 0.5765 | 553.0 | 280.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.32 | 225.37 | 22.63 | 136.69 | -24.44 | 190.93 | 28.26 | 228.36 | 0.5789 | 1201.3 | 372.0 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -22.31 | 189.59 | 26.92 | 230.26 | 0.5468 | -641.0 | -513.2 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -23.28 | 187.41 | 24.74 | 226.60 | 0.5311 | -347.0 | -410.3 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -26.30 | 186.12 | 23.45 | 220.92 | 0.5469 | -557.0 | -473.8 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -26.56 | 186.11 | 23.44 | 220.54 | 0.5494 | -625.0 | -515.5 | |
| 0.00 | 1.89 | 0.00 | 1.11 | -26.33 | 185.91 | 23.24 | 220.63 | 0.5452 | -686.0 | -539.6 | |
| 0.00 | 2.34 | 0.00 | 1.37 | -25.97 | 185.80 | 23.13 | 220.99 | 0.5404 | -958.0 | -781.1 | |
| 0.00 | 4.32 | 0.00 | 2.56 | -27.21 | 185.50 | 22.84 | 219.02 | 0.5503 | -707.0 | -649.6 | |
| 0.00 | 1.89 | 0.00 | 1.12 | -27.31 | 185.27 | 22.60 | 218.61 | 0.5492 | -725.0 | -628.7 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -27.41 | 185.10 | 22.44 | 218.29 | 0.5488 | -847.0 | -689.3 | |
| 0.00 | 1.26 | 0.00 | 0.76 | -29.07 | 185.32 | 22.66 | 216.49 | 0.5682 | -497.0 | -522.9 | |
| 0.00 | 2.43 | 0.00 | 1.45 | -28.33 | 185.01 | 22.34 | 217.03 | 0.5576 | -709.0 | -561.1 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -27.32 | 184.20 | 21.53 | 217.34 | 0.5397 | -736.0 | -554.3 | |
| 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. | |