SDO HMI 2011-08-29 19:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.08 | 81.06 | 19.54 | 84.49 | -20.37 | 259.28 | -56.02 | 117.85 | 0.8810 | 304.1 | -23.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 1.00 | -21.34 | 260.50 | -54.80 | 119.34 | 0.8751 | 544.0 | 475.9 | |
| 2.33 | 19.26 | 2.34 | 19.36 | -20.59 | 260.63 | -54.67 | 118.59 | 0.8718 | 876.4 | 592.1 | |
| 2.06 | -2.00 | 2.08 | -2.00 | -20.48 | 260.35 | -54.96 | 118.37 | 0.8736 | 581.8 | 999999 | |
| 14.69 | 33.05 | 15.12 | 34.22 | -21.03 | 259.93 | -55.37 | 118.79 | 0.8783 | 571.6 | -44.0 | |
| 0.00 | 1.70 | 0.00 | 1.71 | -20.14 | 260.42 | -54.89 | 118.03 | 0.8720 | 400.0 | 403.5 | |
| 0.00 | 1.25 | 0.00 | 1.32 | -20.54 | 258.87 | -56.43 | 117.87 | 0.8845 | 280.0 | 226.8 | |
| 0.00 | 18.72 | 0.00 | 20.08 | -19.48 | 257.86 | -57.44 | 116.38 | 0.8888 | -891.0 | -422.9 | |
| 0.00 | 0.63 | 0.00 | 0.72 | -20.21 | 256.14 | -59.17 | 116.55 | 0.9026 | -218.0 | -220.6 | |
| 0.00 | 1.07 | 0.00 | 1.22 | -19.67 | 256.15 | -59.16 | 115.99 | 0.9012 | -436.0 | -367.4 | |
| 0.00 | 0.81 | 0.00 | 0.87 | -18.19 | 257.00 | -58.31 | 114.70 | 0.8917 | -452.0 | -390.7 | |
| 0.00 | 0.54 | 0.00 | 0.58 | -18.02 | 257.09 | -58.22 | 114.55 | 0.8905 | -544.0 | -508.0 | |
| 0.00 | 1.16 | 0.00 | 1.29 | -18.83 | 256.58 | -58.72 | 115.24 | 0.8962 | -451.0 | -418.9 | |
| 0.00 | 1.07 | 0.00 | 1.20 | -18.93 | 256.28 | -59.03 | 115.24 | 0.8985 | -509.0 | -438.4 | |
| 0.00 | 0.81 | 0.00 | 0.92 | -19.32 | 255.80 | -59.51 | 115.49 | 0.9027 | -339.0 | -229.8 | |
| 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. | |