SDO HMI 2014-04-05 19:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.31 | 286.97 | 36.17 | 158.97 | 10.51 | 0.31 | -20.41 | 49.98 | 0.4469 | -297.7 | -144.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.49 | 130.47 | 0.81 | 70.39 | 10.37 | 4.62 | -16.11 | 44.03 | 0.3945 | -1028.6 | -436.7 | |
| 9.23 | -1.00 | 4.98 | -1.00 | 10.35 | 4.27 | -16.46 | 44.68 | 0.3981 | -1184.3 | 999999 | |
| 3.87 | -1.00 | 2.08 | -1.00 | 10.17 | 4.28 | -16.45 | 45.00 | 0.3959 | -1324.0 | 999999 | |
| 16.44 | -1.00 | 8.89 | -1.00 | 10.37 | 3.88 | -16.84 | 45.32 | 0.4026 | -1103.1 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 10.54 | 3.52 | -17.20 | 45.62 | 0.4086 | -450.0 | -407.5 | |
| 1.05 | 8.35 | 0.57 | 4.53 | 10.35 | 3.37 | -17.35 | 46.20 | 0.4083 | -1022.4 | -689.6 | |
| 0.70 | -6.00 | 0.38 | -6.00 | 10.23 | 3.29 | -17.44 | 46.57 | 0.4080 | -961.8 | 999999 | |
| 0.00 | 1.49 | 0.00 | 0.81 | 10.49 | 2.98 | -17.75 | 46.59 | 0.4143 | -580.0 | -542.2 | |
| 0.00 | 2.11 | 0.00 | 1.14 | 8.60 | 2.92 | -17.80 | 50.24 | 0.3950 | -853.0 | -691.5 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 9.38 | 2.79 | -17.94 | 48.95 | 0.4047 | -832.0 | -727.0 | |
| 0.00 | 1.49 | 0.00 | 0.82 | 11.39 | 2.48 | -18.25 | 45.84 | 0.4298 | -697.0 | -534.7 | |
| 0.00 | 1.85 | 0.00 | 1.01 | 10.51 | 2.40 | -18.32 | 47.47 | 0.4212 | -808.0 | -576.0 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 9.99 | 2.31 | -18.42 | 48.58 | 0.4168 | -876.0 | -811.4 | |
| 0.00 | 1.23 | 0.00 | 0.68 | 11.57 | 1.98 | -18.75 | 46.31 | 0.4373 | -817.0 | -576.6 | |
| 0.00 | 1.41 | 0.00 | 0.77 | 10.22 | 1.88 | -18.85 | 48.81 | 0.4244 | -929.0 | -717.9 | |
| 0.00 | 1.85 | 0.00 | 1.02 | 11.93 | 1.60 | -19.13 | 46.28 | 0.4455 | -888.0 | -596.6 | |
| 0.00 | 2.11 | 0.00 | 1.17 | 12.32 | 1.34 | -19.39 | 46.03 | 0.4525 | -800.0 | -687.0 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 11.57 | 1.11 | -19.62 | 47.61 | 0.4473 | -745.0 | -526.8 | |
| 0.00 | 1.41 | 0.00 | 0.78 | 12.39 | 0.95 | -19.78 | 46.48 | 0.4578 | -714.0 | -564.2 | |
| 0.00 | 2.02 | 0.00 | 1.13 | 12.33 | 0.17 | -20.56 | 47.69 | 0.4659 | -572.0 | -432.6 | |
| 0.00 | 0.97 | 0.00 | 0.54 | 9.79 | 359.50 | -21.23 | 52.94 | 0.4490 | 808.0 | 629.7 | |
| 0.00 | 5.98 | 0.00 | 3.34 | 10.17 | 358.59 | -22.14 | 53.42 | 0.4638 | 1061.0 | 862.7 | |
| 0.00 | 1.23 | 0.00 | 0.69 | 10.58 | 358.43 | -22.30 | 52.91 | 0.4696 | 859.0 | 682.7 | |
| 0.00 | 0.62 | 0.00 | 0.35 | 10.74 | 358.28 | -22.45 | 52.80 | 0.4728 | 621.0 | 473.3 | |
| 0.00 | 1.41 | 0.00 | 0.79 | 11.60 | 358.08 | -22.65 | 51.61 | 0.4832 | 742.0 | 570.0 | |
| 5.71 | 8.18 | 3.21 | 4.59 | 10.02 | 357.81 | -22.92 | 54.64 | 0.4722 | 1029.4 | 683.5 | |
| 0.00 | 0.97 | 0.00 | 0.55 | 12.25 | 357.59 | -23.14 | 51.15 | 0.4951 | 743.0 | 650.4 | |
| 0.00 | 0.70 | 0.00 | 0.40 | 11.28 | 356.78 | -23.95 | 53.69 | 0.4961 | 603.0 | 482.2 | |
| 3.52 | 83.78 | 1.99 | 47.62 | 10.31 | 356.76 | -23.97 | 55.34 | 0.4879 | 1079.9 | 93.0 | |
| 10.90 | -29.00 | 6.18 | -29.00 | 10.13 | 356.64 | -24.09 | 55.79 | 0.4879 | 1086.5 | 999999 | |
| 2.99 | -29.00 | 1.70 | -29.00 | 10.45 | 356.58 | -24.15 | 55.32 | 0.4913 | 657.5 | 999999 | |
| 5.01 | -29.00 | 2.86 | -29.00 | 10.33 | 355.82 | -24.91 | 56.35 | 0.4998 | -1148.1 | 999999 | |
| 3.96 | -29.00 | 2.26 | -29.00 | 10.52 | 355.80 | -24.93 | 56.05 | 0.5016 | -1048.9 | 999999 | |
| 0.00 | 2.64 | 0.00 | 1.52 | 11.54 | 355.37 | -25.36 | 54.82 | 0.5154 | -827.0 | -634.0 | |
| 0.00 | 1.49 | 0.00 | 0.86 | 11.42 | 355.28 | -25.45 | 55.12 | 0.5155 | -723.0 | -597.5 | |
| 0.00 | 3.08 | 0.00 | 1.80 | 11.68 | 353.92 | -26.81 | 56.09 | 0.5342 | 683.0 | 675.1 | |
| 0.44 | 16.00 | 0.26 | 9.41 | 12.04 | 353.71 | -27.02 | 55.74 | 0.5396 | 833.6 | 707.3 | |
| 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. | |