SDO HMI 2011-08-08 21:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.97 | 24.00 | 2.18 | 13.19 | -16.22 | 243.14 | 11.39 | 206.41 | 0.4296 | -67.1 | -197.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.97 | 4.60 | 2.18 | 2.53 | -14.73 | 246.29 | 14.55 | 214.36 | 0.4321 | 995.0 | 777.3 | |
| 0.00 | 1.81 | 0.00 | 1.00 | -15.35 | 246.21 | 14.46 | 213.39 | 0.4394 | 717.0 | 631.1 | |
| 0.00 | 2.08 | 0.00 | 1.14 | -14.69 | 245.74 | 13.99 | 213.40 | 0.4267 | 950.0 | 657.1 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -15.95 | 245.24 | 13.49 | 210.86 | 0.4391 | 911.0 | 822.2 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -16.00 | 244.95 | 13.21 | 210.25 | 0.4376 | 843.0 | 714.1 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -17.36 | 242.38 | 10.63 | 203.80 | 0.4382 | -687.0 | -539.2 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -17.55 | 241.77 | 10.03 | 202.42 | 0.4372 | -754.0 | -605.0 | |
| 0.00 | 3.70 | 0.00 | 2.03 | -17.34 | 241.37 | 9.63 | 201.79 | 0.4318 | -803.0 | -612.6 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -16.81 | 241.15 | 9.41 | 201.82 | 0.4227 | -798.0 | -630.0 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -17.07 | 241.17 | 9.42 | 201.61 | 0.4266 | -815.0 | -668.7 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -17.06 | 240.46 | 8.71 | 200.13 | 0.4225 | -1022.0 | -775.4 | |
| 0.00 | 1.63 | 0.00 | 0.89 | -17.16 | 240.30 | 8.56 | 199.72 | 0.4231 | -940.0 | -796.1 | |
| 0.00 | 1.99 | 0.00 | 1.08 | -16.73 | 238.65 | 6.90 | 196.43 | 0.4086 | -723.0 | -696.2 | |
| 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. | |