SDO HMI 2014-07-06 00:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.71 | 0.00 | 13.09 | 10.71 | 308.00 | 53.45 | 280.84 | 0.8053 | 160.9 | 166.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.27 | 0.00 | 0.27 | 11.11 | 314.35 | 59.80 | 280.89 | 0.8656 | -400.0 | -410.7 | |
| 0.00 | 1.36 | 0.00 | 1.28 | 11.29 | 312.65 | 58.10 | 281.20 | 0.8507 | -405.0 | -345.9 | |
| 0.00 | 1.45 | 0.00 | 1.28 | 8.86 | 310.54 | 55.99 | 278.41 | 0.8301 | -303.0 | -357.2 | |
| 0.00 | 0.27 | 0.00 | 0.24 | 8.07 | 309.81 | 55.26 | 277.47 | 0.8228 | -505.0 | -417.0 | |
| 0.00 | 1.09 | 0.00 | 0.93 | 12.99 | 309.01 | 54.47 | 283.54 | 0.8178 | -386.0 | -318.1 | |
| 0.00 | 0.54 | 0.00 | 0.45 | 9.97 | 307.33 | 52.78 | 279.95 | 0.7985 | 251.0 | 278.7 | |
| 0.00 | 1.91 | 0.00 | 1.55 | 10.26 | 307.09 | 52.54 | 280.33 | 0.7962 | 395.0 | 310.0 | |
| 0.00 | 1.09 | 0.00 | 0.89 | 10.48 | 306.99 | 52.44 | 280.62 | 0.7953 | 269.0 | 296.1 | |
| 0.00 | 1.18 | 0.00 | 0.96 | 10.36 | 306.91 | 52.36 | 280.48 | 0.7943 | 538.0 | 473.7 | |
| 0.00 | 0.36 | 0.00 | 0.29 | 8.75 | 306.35 | 51.80 | 278.48 | 0.7875 | 414.0 | 427.0 | |
| 0.00 | 1.91 | 0.00 | 1.54 | 10.16 | 306.55 | 52.01 | 280.25 | 0.7905 | 608.0 | 549.4 | |
| 0.00 | 1.00 | 0.00 | 0.80 | 10.56 | 306.55 | 52.00 | 280.76 | 0.7907 | 578.0 | 527.0 | |
| 0.00 | 1.73 | 0.00 | 1.39 | 11.49 | 306.53 | 51.98 | 281.94 | 0.7913 | 388.0 | 307.3 | |
| 0.00 | 0.82 | 0.00 | 0.65 | 12.42 | 305.92 | 51.37 | 283.18 | 0.7858 | 350.0 | 218.3 | |
| 0.00 | 0.73 | 0.00 | 0.57 | 12.31 | 305.54 | 50.99 | 283.09 | 0.7817 | 622.0 | 531.2 | |
| 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. | |