SDO HMI 2014-08-04 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.79 | 0.00 | 11.21 | 14.26 | 257.49 | 37.08 | 286.33 | 0.6116 | 456.7 | 401.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 1.15 | 16.47 | 268.96 | 48.55 | 286.67 | 0.7526 | -567.0 | -442.6 | |
| 0.00 | 0.45 | 0.00 | 0.32 | 16.11 | 266.22 | 45.81 | 286.63 | 0.7213 | -732.0 | -643.4 | |
| 0.00 | 1.08 | 0.00 | 0.70 | 9.20 | 260.23 | 39.82 | 277.15 | 0.6394 | 566.0 | 455.2 | |
| 0.00 | 1.27 | 0.00 | 0.81 | 9.34 | 259.97 | 39.56 | 277.39 | 0.6360 | 467.0 | 431.1 | |
| 0.00 | 0.99 | 0.00 | 0.63 | 8.94 | 259.44 | 39.03 | 276.79 | 0.6287 | 488.0 | 469.9 | |
| 0.00 | 0.99 | 0.00 | 0.63 | 7.13 | 259.11 | 38.70 | 273.89 | 0.6241 | 651.0 | 587.9 | |
| 0.00 | 1.08 | 0.00 | 0.70 | 16.40 | 259.53 | 39.12 | 288.50 | 0.6405 | 521.0 | 382.2 | |
| 0.00 | 0.99 | 0.00 | 0.62 | 9.25 | 257.48 | 37.07 | 277.40 | 0.6022 | 591.0 | 509.0 | |
| 0.00 | 1.54 | 0.00 | 0.95 | 13.26 | 257.19 | 36.78 | 284.09 | 0.6031 | 722.0 | 531.9 | |
| 0.00 | 1.54 | 0.00 | 0.97 | 17.13 | 257.80 | 37.39 | 290.17 | 0.6205 | 657.0 | 562.5 | |
| 0.00 | 0.90 | 0.00 | 0.55 | 14.61 | 255.84 | 35.44 | 286.68 | 0.5879 | 631.0 | 539.9 | |
| 0.00 | 0.99 | 0.00 | 0.60 | 11.22 | 254.80 | 34.39 | 281.09 | 0.5667 | 657.0 | 466.0 | |
| 0.00 | 1.18 | 0.00 | 0.71 | 14.94 | 254.91 | 34.50 | 287.53 | 0.5761 | 702.0 | 532.5 | |
| 0.00 | 1.08 | 0.00 | 0.66 | 23.56 | 252.18 | 31.77 | 303.19 | 0.5789 | 606.0 | 538.3 | |
| 0.00 | 2.17 | 0.00 | 1.21 | 20.06 | 244.48 | 24.07 | 303.23 | 0.4599 | 891.0 | 779.2 | |
| 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. | |