SDO HMI 2014-04-18 00:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.52 | 224.50 | 43.75 | 141.75 | -12.78 | 181.35 | -38.20 | 103.82 | 0.6230 | 231.1 | -23.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.62 | 0.00 | 0.36 | -13.49 | 188.41 | -31.14 | 107.02 | 0.5280 | 665.0 | 547.9 | |
| 0.00 | 2.75 | 0.00 | 1.60 | -13.70 | 188.34 | -31.21 | 107.39 | 0.5296 | 641.0 | 538.9 | |
| 0.00 | 0.89 | 0.00 | 0.52 | -14.29 | 187.78 | -31.78 | 108.24 | 0.5394 | 661.0 | 509.4 | |
| 0.00 | 1.15 | 0.00 | 0.67 | -12.91 | 187.80 | -31.75 | 105.74 | 0.5350 | 469.0 | 363.5 | |
| 0.00 | 1.06 | 0.00 | 0.62 | -11.48 | 187.74 | -31.81 | 103.06 | 0.5323 | 700.0 | 528.8 | |
| 0.00 | 1.86 | 0.00 | 1.09 | -10.95 | 187.37 | -32.18 | 101.97 | 0.5366 | 610.0 | 552.2 | |
| 0.00 | 0.89 | 0.00 | 0.54 | -11.66 | 183.53 | -36.03 | 102.40 | 0.5920 | 598.0 | 481.3 | |
| 21.34 | 40.91 | 13.14 | 25.22 | -12.56 | 183.34 | -36.21 | 103.87 | 0.5961 | 936.7 | 308.0 | |
| 1.33 | -8.00 | 0.82 | -8.00 | -12.19 | 183.29 | -36.26 | 103.24 | 0.5962 | 834.5 | 999999 | |
| 3.10 | -8.00 | 1.91 | -8.00 | -12.33 | 183.11 | -36.44 | 103.44 | 0.5988 | 759.4 | 999999 | |
| 1.95 | -8.00 | 1.21 | -8.00 | -12.32 | 182.88 | -36.67 | 103.37 | 0.6019 | 603.9 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.60 | -11.35 | 182.92 | -36.63 | 101.77 | 0.5998 | 577.0 | 448.1 | |
| 0.00 | 0.44 | 0.00 | 0.28 | -12.56 | 182.34 | -37.21 | 103.66 | 0.6097 | 376.0 | 370.6 | |
| 0.00 | 1.42 | 0.00 | 0.89 | -12.26 | 181.85 | -37.70 | 103.06 | 0.6158 | 479.0 | 323.1 | |
| 0.00 | 1.24 | 0.00 | 0.78 | -12.64 | 181.59 | -37.97 | 103.63 | 0.6199 | -687.0 | -578.7 | |
| 16.74 | 152.94 | 10.59 | 97.40 | -13.42 | 181.36 | -38.19 | 104.83 | 0.6243 | 1094.1 | -77.4 | |
| 0.00 | 1.15 | 0.00 | 0.72 | -11.34 | 181.69 | -37.86 | 101.54 | 0.6165 | 529.0 | 389.2 | |
| 0.00 | 1.42 | 0.00 | 0.89 | -11.64 | 181.60 | -37.95 | 102.01 | 0.6181 | -200.0 | -161.5 | |
| 0.00 | 1.06 | 0.00 | 0.67 | -12.44 | 181.35 | -38.21 | 103.26 | 0.6228 | -456.0 | -428.0 | |
| 3.28 | -16.00 | 2.09 | -16.00 | -12.53 | 180.70 | -38.85 | 103.27 | 0.6315 | -963.6 | 999999 | |
| 1.59 | -16.00 | 1.02 | -16.00 | -12.90 | 180.31 | -39.24 | 103.78 | 0.6372 | -515.8 | 999999 | |
| 11.51 | -16.00 | 7.39 | -16.00 | -12.74 | 180.22 | -39.33 | 103.52 | 0.6381 | -1031.5 | 999999 | |
| 0.89 | 4.78 | 0.57 | 3.06 | -11.66 | 180.41 | -39.14 | 101.85 | 0.6339 | -845.8 | -666.2 | |
| 0.44 | -23.00 | 0.28 | -23.00 | -11.83 | 180.26 | -39.29 | 102.10 | 0.6361 | -734.0 | 999999 | |
| 3.54 | -16.00 | 2.28 | -16.00 | -13.03 | 179.92 | -39.63 | 103.91 | 0.6424 | -929.2 | 999999 | |
| 3.81 | -16.00 | 2.45 | -16.00 | -12.52 | 179.98 | -39.57 | 103.12 | 0.6408 | -760.5 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.17 | -15.35 | 179.26 | -40.29 | 107.31 | 0.6554 | 628.0 | 599.3 | |
| 0.00 | 1.24 | 0.00 | 0.80 | -12.02 | 179.87 | -39.68 | 102.33 | 0.6415 | -522.0 | -389.8 | |
| 0.00 | 1.68 | 0.00 | 1.08 | -12.17 | 179.80 | -39.75 | 102.55 | 0.6426 | -451.0 | -368.0 | |
| 0.00 | 0.89 | 0.00 | 0.57 | -12.77 | 179.65 | -39.90 | 103.46 | 0.6455 | -489.0 | -391.8 | |
| 0.00 | 1.51 | 0.00 | 0.97 | -12.09 | 179.54 | -40.01 | 102.39 | 0.6460 | -552.0 | -430.4 | |
| 0.00 | 1.59 | 0.00 | 1.02 | -9.08 | 179.97 | -39.58 | 97.74 | 0.6372 | 730.0 | 606.1 | |
| 0.00 | 0.97 | 0.00 | 0.66 | -7.63 | 176.17 | -43.38 | 95.41 | 0.6861 | 472.0 | 413.9 | |
| 0.00 | 0.80 | 0.00 | 0.57 | -13.26 | 173.35 | -46.20 | 103.21 | 0.7240 | -545.0 | -521.6 | |
| 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. | |