SDO HMI 2014-03-18 13:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.46 | 157.52 | 20.62 | 95.23 | -11.36 | 296.38 | 34.94 | 260.10 | 0.5709 | -197.4 | -146.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.61 | 0.00 | 0.50 | -21.65 | 314.22 | 52.79 | 248.15 | 0.7997 | -453.0 | -431.4 | |
| 0.00 | 1.04 | 0.00 | 0.77 | -9.42 | 309.92 | 48.49 | 263.67 | 0.7455 | 562.0 | 506.2 | |
| 0.00 | 5.14 | 0.00 | 3.80 | -9.78 | 309.94 | 48.51 | 263.19 | 0.7457 | 725.0 | 534.8 | |
| 0.00 | 0.96 | 0.00 | 0.68 | -8.88 | 307.59 | 46.15 | 264.48 | 0.7182 | 583.0 | 478.5 | |
| 0.00 | 1.65 | 0.00 | 1.17 | -12.02 | 307.22 | 45.78 | 260.09 | 0.7140 | 772.0 | 542.8 | |
| 0.00 | 1.04 | 0.00 | 0.72 | -10.64 | 305.99 | 44.55 | 262.00 | 0.6986 | 786.0 | 762.4 | |
| 0.00 | 0.61 | 0.00 | 0.39 | -6.63 | 301.86 | 40.43 | 268.11 | 0.6468 | 473.0 | 378.9 | |
| 0.00 | 2.00 | 0.00 | 1.23 | -8.23 | 298.12 | 36.69 | 265.73 | 0.5952 | -667.0 | -583.7 | |
| 0.00 | 1.91 | 0.00 | 1.18 | -8.56 | 298.05 | 36.61 | 265.16 | 0.5941 | -780.0 | -596.4 | |
| 0.00 | 2.96 | 0.00 | 1.82 | -10.39 | 298.01 | 36.57 | 262.07 | 0.5940 | 710.0 | 632.7 | |
| 5.40 | 11.40 | 3.30 | 6.96 | -10.58 | 297.54 | 36.11 | 261.72 | 0.5876 | 918.5 | 716.7 | |
| 6.44 | 22.81 | 3.93 | 13.91 | -11.49 | 297.44 | 36.01 | 260.16 | 0.5870 | 912.5 | 733.8 | |
| 1.91 | -11.00 | 1.17 | -11.00 | -10.60 | 297.21 | 35.77 | 261.66 | 0.5830 | 959.8 | 999999 | |
| 0.00 | 3.39 | 0.00 | 2.05 | -10.04 | 296.69 | 35.25 | 262.60 | 0.5753 | 733.0 | 649.0 | |
| 0.00 | 1.65 | 0.00 | 0.99 | -11.15 | 296.16 | 34.73 | 260.60 | 0.5687 | 894.0 | 748.1 | |
| 0.00 | 1.91 | 0.00 | 1.15 | -12.81 | 295.70 | 34.26 | 257.60 | 0.5643 | -841.0 | -676.9 | |
| 0.00 | 1.13 | 0.00 | 0.67 | -11.23 | 294.96 | 33.53 | 260.31 | 0.5517 | -325.0 | -230.2 | |
| 9.23 | 26.37 | 5.46 | 15.60 | -11.79 | 294.78 | 33.34 | 259.28 | 0.5498 | -855.7 | -291.7 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -11.04 | 294.68 | 33.25 | 260.62 | 0.5475 | -332.0 | -319.4 | |
| 0.00 | 2.09 | 0.00 | 1.24 | -11.37 | 294.72 | 33.29 | 260.03 | 0.5485 | -608.0 | -521.8 | |
| 0.00 | 0.70 | 0.00 | 0.41 | -14.33 | 295.02 | 33.58 | 254.74 | 0.5577 | -569.0 | -507.9 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -10.16 | 294.39 | 32.96 | 262.21 | 0.5426 | -574.0 | -437.8 | |
| 2.87 | 48.48 | 1.69 | 28.48 | -10.85 | 294.36 | 32.93 | 260.93 | 0.5428 | -822.2 | -663.8 | |
| 0.00 | 1.83 | 0.00 | 1.09 | -14.65 | 294.77 | 33.34 | 254.11 | 0.5551 | -709.0 | -611.3 | |
| 6.79 | -23.00 | 3.99 | -23.00 | -10.69 | 294.13 | 32.69 | 261.21 | 0.5392 | -1003.7 | 999999 | |
| 0.00 | 2.44 | 0.00 | 1.43 | -11.43 | 294.18 | 32.75 | 259.83 | 0.5408 | -843.0 | -724.7 | |
| 0.78 | 2.87 | 0.47 | 1.71 | -14.87 | 294.66 | 33.23 | 253.69 | 0.5541 | -798.6 | -611.4 | |
| 0.00 | 2.70 | 0.00 | 1.61 | -15.47 | 294.77 | 33.34 | 252.65 | 0.5571 | -567.0 | -435.8 | |
| 1.04 | -23.00 | 0.61 | -23.00 | -10.53 | 293.85 | 32.42 | 261.48 | 0.5351 | -984.0 | 999999 | |
| 0.00 | 1.22 | 0.00 | 0.72 | -12.29 | 294.04 | 32.61 | 258.23 | 0.5400 | -765.0 | -542.6 | |
| 0.00 | 2.18 | 0.00 | 1.28 | -14.79 | 294.02 | 32.59 | 253.64 | 0.5449 | -748.0 | -506.5 | |
| 0.00 | 1.13 | 0.00 | 0.67 | -15.86 | 293.95 | 32.52 | 251.69 | 0.5469 | -621.0 | -518.7 | |
| 0.00 | 1.13 | 0.00 | 0.66 | -15.27 | 293.56 | 32.12 | 252.60 | 0.5397 | -799.0 | -691.4 | |
| 0.00 | 1.22 | 0.00 | 0.67 | -14.66 | 286.15 | 24.72 | 250.55 | 0.4308 | -806.0 | -676.7 | |
| 0.00 | 1.13 | 0.00 | 0.59 | -13.75 | 279.19 | 17.75 | 247.64 | 0.3217 | -727.0 | -595.8 | |
| 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. | |