SDO HMI 2014-06-08 15:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.91 | 0.00 | 13.65 | 5.33 | 264.16 | 7.23 | 293.43 | 0.1970 | 50.2 | 4.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.81 | 0.00 | 0.94 | 4.27 | 274.18 | 17.26 | 283.46 | 0.3055 | -669.0 | -486.0 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 4.42 | 273.99 | 17.07 | 284.09 | 0.3030 | -904.0 | -720.4 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 4.85 | 273.36 | 16.44 | 286.00 | 0.2947 | -665.0 | -619.4 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 4.52 | 272.34 | 15.42 | 285.81 | 0.2766 | -917.0 | -795.3 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 4.49 | 272.12 | 15.19 | 285.92 | 0.2729 | -966.0 | -775.0 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 6.08 | 272.06 | 15.14 | 291.47 | 0.2803 | -810.0 | -581.1 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 4.28 | 271.80 | 14.87 | 285.47 | 0.2668 | -787.0 | -628.2 | |
| 0.00 | 2.81 | 0.00 | 1.42 | 3.68 | 267.35 | 10.42 | 288.46 | 0.1912 | -697.0 | -553.8 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 6.89 | 261.19 | 4.27 | 327.53 | 0.1383 | 708.0 | 472.9 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 5.92 | 259.93 | 3.00 | 332.27 | 0.1126 | 935.0 | 731.7 | |
| 0.00 | 1.90 | 0.00 | 0.95 | 6.59 | 259.81 | 2.89 | 335.71 | 0.1222 | 796.0 | 632.9 | |
| 0.00 | 3.53 | 0.00 | 1.78 | 10.62 | 257.46 | 0.54 | 357.07 | 0.1815 | 839.0 | 646.6 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 4.33 | 256.68 | -0.24 | 3.32 | 0.0721 | 861.0 | 614.1 | |
| 0.00 | 1.18 | 0.00 | 0.58 | -1.72 | 256.65 | -0.28 | 171.92 | 0.0345 | 920.0 | 693.5 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 6.66 | 255.19 | -1.74 | 15.05 | 0.1165 | 771.0 | 539.1 | |
| 0.00 | 0.81 | 0.00 | 0.40 | -0.17 | 254.79 | -2.13 | 100.46 | 0.0380 | 774.0 | 665.8 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 5.72 | 243.42 | -13.51 | 67.59 | 0.2525 | 665.0 | 523.0 | |
| 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. | |