SDO HMI 2014-07-06 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.18 | 0.00 | 12.75 | 10.18 | 307.86 | 53.86 | 280.16 | 0.8093 | 273.6 | 201.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.91 | 0.00 | 0.86 | 11.27 | 312.63 | 58.63 | 281.14 | 0.8555 | -372.0 | -364.9 | |
| 0.00 | 1.73 | 0.00 | 1.56 | 9.05 | 310.76 | 56.77 | 278.60 | 0.8375 | -453.0 | -364.2 | |
| 0.00 | 1.09 | 0.00 | 0.95 | 8.12 | 309.49 | 55.50 | 277.53 | 0.8251 | -559.0 | -493.2 | |
| 0.00 | 0.73 | 0.00 | 0.62 | 9.35 | 308.26 | 54.26 | 279.09 | 0.8132 | 467.0 | 411.9 | |
| 0.00 | 1.54 | 0.00 | 1.28 | 10.01 | 307.36 | 53.36 | 279.96 | 0.8045 | 303.0 | 237.6 | |
| 0.00 | 0.73 | 0.00 | 0.60 | 10.24 | 307.10 | 53.10 | 280.26 | 0.8020 | 434.0 | 336.9 | |
| 0.00 | 1.54 | 0.00 | 1.27 | 10.34 | 306.97 | 52.97 | 280.40 | 0.8007 | 425.0 | 387.5 | |
| 0.00 | 0.82 | 0.00 | 0.67 | 10.29 | 306.80 | 52.80 | 280.34 | 0.7989 | 434.0 | 378.1 | |
| 0.00 | 1.27 | 0.00 | 1.04 | 9.99 | 306.63 | 52.63 | 279.98 | 0.7969 | 592.0 | 471.4 | |
| 0.00 | 1.82 | 0.00 | 1.48 | 10.14 | 306.61 | 52.61 | 280.17 | 0.7969 | 668.0 | 547.3 | |
| 0.00 | 0.73 | 0.00 | 0.59 | 10.54 | 306.61 | 52.61 | 280.68 | 0.7971 | 620.0 | 523.9 | |
| 0.00 | 1.09 | 0.00 | 0.88 | 11.62 | 306.17 | 52.17 | 282.07 | 0.7933 | 435.0 | 362.0 | |
| 0.00 | 1.18 | 0.00 | 0.95 | 12.33 | 305.55 | 51.55 | 283.03 | 0.7876 | 563.0 | 508.8 | |
| 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. | |