SDO HMI 2011-06-19 18:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.78 | 0.00 | 32.64 | -14.87 | 245.52 | 70.52 | 253.77 | 0.9501 | 160.7 | 252.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 1.74 | -14.63 | 247.54 | 72.54 | 254.26 | 0.9602 | 391.0 | 331.2 | |
| 0.00 | 0.73 | 0.00 | 1.21 | -14.51 | 246.72 | 71.71 | 254.29 | 0.9562 | 86.0 | 190.5 | |
| 0.00 | 3.63 | 0.00 | 5.89 | -14.37 | 246.21 | 71.20 | 254.38 | 0.9535 | 659.0 | 541.7 | |
| 0.00 | 1.90 | 0.00 | 3.15 | -15.11 | 246.49 | 71.48 | 253.64 | 0.9554 | 549.0 | 464.2 | |
| 0.00 | 1.54 | 0.00 | 2.55 | -15.36 | 246.50 | 71.49 | 253.38 | 0.9556 | 130.0 | 220.5 | |
| 0.00 | 1.27 | 0.00 | 1.96 | -13.94 | 245.31 | 70.30 | 254.73 | 0.9486 | 7.0 | 34.9 | |
| 0.00 | 1.09 | 0.00 | 1.82 | -15.68 | 246.56 | 71.56 | 253.05 | 0.9561 | 398.0 | 386.0 | |
| 0.00 | 2.45 | 0.00 | 3.79 | -14.51 | 245.24 | 70.24 | 254.13 | 0.9486 | 424.0 | 376.7 | |
| 0.00 | 1.45 | 0.00 | 2.19 | -14.56 | 244.72 | 69.72 | 254.01 | 0.9458 | 311.0 | 299.3 | |
| 0.00 | 1.27 | 0.00 | 1.88 | -14.30 | 244.45 | 69.44 | 254.25 | 0.9441 | -46.0 | -41.8 | |
| 0.00 | 1.54 | 0.00 | 2.34 | -14.94 | 244.81 | 69.81 | 253.62 | 0.9466 | 345.0 | 313.4 | |
| 0.00 | 0.82 | 0.00 | 1.22 | -15.69 | 244.36 | 69.36 | 252.77 | 0.9447 | -126.0 | -122.8 | |
| 0.00 | 0.82 | 0.00 | 1.13 | -16.12 | 242.66 | 67.66 | 252.08 | 0.9354 | -401.0 | -399.0 | |
| 0.00 | 1.27 | 0.00 | 1.77 | -16.35 | 242.74 | 67.74 | 251.85 | 0.9360 | -477.0 | -396.0 | |
| 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. | |