SDO HMI 2014-07-29 06:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.78 | 0.00 | 11.07 | 11.23 | 258.35 | -48.58 | 79.72 | 0.7470 | 244.0 | 224.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.74 | 13.70 | 269.54 | -37.39 | 74.75 | 0.6137 | -440.0 | -328.3 | |
| 0.00 | 0.91 | 0.00 | 0.58 | 14.42 | 268.08 | -38.85 | 73.96 | 0.6344 | -688.0 | -569.3 | |
| 0.00 | 1.27 | 0.00 | 0.82 | 12.21 | 266.84 | -40.09 | 77.63 | 0.6466 | -589.0 | -528.1 | |
| 0.00 | 0.63 | 0.00 | 0.47 | 10.88 | 258.66 | -48.27 | 80.37 | 0.7456 | 641.0 | 445.6 | |
| 0.00 | 1.90 | 0.00 | 1.41 | 8.62 | 258.53 | -48.40 | 83.40 | 0.7465 | 541.0 | 446.0 | |
| 0.00 | 1.18 | 0.00 | 0.89 | 10.32 | 257.78 | -49.14 | 81.15 | 0.7553 | 581.0 | 420.1 | |
| 0.00 | 1.63 | 0.00 | 1.25 | 9.83 | 256.93 | -50.00 | 81.82 | 0.7648 | 635.0 | 514.9 | |
| 0.00 | 1.27 | 0.00 | 0.99 | 12.74 | 256.23 | -50.70 | 78.06 | 0.7737 | 245.0 | 273.5 | |
| 0.00 | 0.73 | 0.00 | 0.56 | 9.62 | 256.63 | -50.30 | 82.10 | 0.7681 | 490.0 | 426.6 | |
| 0.00 | 1.45 | 0.00 | 1.16 | 12.96 | 255.06 | -51.87 | 77.86 | 0.7863 | 368.0 | 250.2 | |
| 0.00 | 0.54 | 0.00 | 0.44 | 11.12 | 253.93 | -53.00 | 80.25 | 0.7973 | 410.0 | 333.5 | |
| 0.00 | 0.91 | 0.00 | 0.75 | 10.02 | 253.63 | -53.30 | 81.64 | 0.8002 | 464.0 | 371.7 | |
| 0.00 | 1.18 | 0.00 | 1.01 | 11.51 | 251.80 | -55.13 | 79.83 | 0.8189 | 514.0 | 404.5 | |
| 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. | |