SDO HMI 2011-08-17 21:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.92 | 35.46 | 4.32 | 19.37 | -17.96 | 113.95 | 1.19 | 182.63 | 0.4213 | -217.0 | -256.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.15 | 5.76 | 1.73 | 3.16 | -18.43 | 116.94 | 4.17 | 189.21 | 0.4326 | 919.5 | 943.6 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -18.39 | 116.33 | 3.56 | 187.89 | 0.4306 | 914.0 | 740.7 | |
| 0.00 | 2.16 | 0.00 | 1.19 | -18.55 | 115.59 | 2.82 | 186.24 | 0.4317 | 1070.0 | 748.6 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -18.15 | 114.82 | 2.05 | 184.62 | 0.4241 | 765.0 | 591.4 | |
| 0.00 | 2.16 | 0.00 | 1.17 | -17.51 | 114.17 | 1.41 | 183.26 | 0.4133 | -983.0 | -833.1 | |
| 0.45 | 2.16 | 0.24 | 1.18 | -17.71 | 113.76 | 0.99 | 182.29 | 0.4162 | -1044.0 | -895.0 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -18.48 | 113.67 | 0.90 | 182.01 | 0.4283 | -804.0 | -644.6 | |
| 0.00 | 1.71 | 0.00 | 0.94 | -18.48 | 113.51 | 0.74 | 181.65 | 0.4283 | -710.0 | -542.4 | |
| 2.70 | 9.63 | 1.47 | 5.26 | -17.91 | 113.44 | 0.68 | 181.54 | 0.4192 | -1015.3 | -799.8 | |
| 1.62 | 3.15 | 0.88 | 1.71 | -17.01 | 113.00 | 0.23 | 180.54 | 0.4047 | 928.7 | 980.6 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -18.95 | 112.74 | -0.03 | 179.95 | 0.4355 | -793.0 | -609.8 | |
| 0.00 | 2.25 | 0.00 | 1.22 | -17.58 | 111.12 | -1.65 | 176.19 | 0.4146 | -794.0 | -632.7 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -16.94 | 111.03 | -1.74 | 175.87 | 0.4047 | -806.0 | -644.2 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -17.48 | 110.48 | -2.28 | 174.71 | 0.4139 | -804.0 | -662.1 | |
| 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. | |