SDO HMI 2011-10-22 18:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.65 | 444.53 | 109.02 | 789.53 | 7.64 | 249.00 | -74.14 | 83.59 | 0.9566 | -241.6 | -52.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.13 | 0.00 | 1.43 | 10.94 | 255.60 | -67.54 | 80.35 | 0.9221 | -214.0 | -192.5 | |
| 25.65 | 273.05 | 33.61 | 367.85 | 6.24 | 255.01 | -68.13 | 85.41 | 0.9271 | -843.8 | -167.0 | |
| 15.48 | -2.00 | 21.10 | -2.00 | 6.12 | 254.04 | -69.10 | 85.48 | 0.9334 | -385.1 | 999999 | |
| 0.00 | 1.13 | 0.00 | 1.73 | 11.15 | 251.31 | -71.83 | 80.00 | 0.9480 | -73.0 | -58.8 | |
| 1.22 | -2.00 | 1.71 | -2.00 | 5.88 | 253.33 | -69.81 | 85.69 | 0.9378 | 146.7 | 999999 | |
| 0.00 | 1.22 | 0.00 | 2.05 | 5.73 | 249.91 | -73.23 | 85.62 | 0.9568 | -321.0 | -272.5 | |
| 0.00 | 1.91 | 0.00 | 3.28 | 5.71 | 249.60 | -73.54 | 85.63 | 0.9583 | -68.0 | 29.7 | |
| 2.26 | 7.74 | 4.26 | 14.62 | 6.64 | 247.87 | -75.27 | 84.54 | 0.9662 | 434.0 | 419.8 | |
| 4.52 | 147.48 | 10.59 | 374.86 | 10.25 | 244.57 | -78.57 | 80.63 | 0.9785 | 432.3 | 16.7 | |
| 2.96 | -9.00 | 6.92 | -9.00 | 9.83 | 244.63 | -78.51 | 81.06 | 0.9784 | 383.5 | 999999 | |
| 1.91 | -9.00 | 4.72 | -9.00 | 9.59 | 244.04 | -79.10 | 81.27 | 0.9805 | 309.1 | 999999 | |
| 0.00 | 10.87 | 0.00 | 23.71 | 6.51 | 245.73 | -77.41 | 84.53 | 0.9751 | 370.0 | 318.0 | |
| 5.22 | -9.00 | 13.83 | -9.00 | 8.40 | 243.21 | -79.93 | 82.43 | 0.9834 | 214.7 | 999999 | |
| 4.43 | -9.00 | 12.28 | -9.00 | 8.58 | 242.87 | -80.27 | 82.22 | 0.9844 | -367.5 | 999999 | |
| 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. | |