SDO HMI 2011-10-22 21:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.57 | 23.14 | 0.80 | 11.74 | 17.26 | 322.76 | 1.27 | 353.98 | 0.2186 | 538.7 | 510.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.96 | 0.00 | 0.49 | 17.06 | 326.28 | 4.80 | 338.61 | 0.2205 | -794.0 | -647.1 | |
| 0.00 | 1.74 | 0.00 | 0.87 | 14.22 | 325.88 | 4.40 | 334.45 | 0.1731 | 1030.0 | 673.9 | |
| 0.00 | 2.44 | 0.00 | 1.22 | 14.25 | 325.29 | 3.81 | 337.56 | 0.1695 | 807.0 | 678.8 | |
| 0.00 | 3.39 | 0.00 | 1.72 | 17.92 | 324.96 | 3.47 | 345.25 | 0.2274 | 957.0 | 699.5 | |
| 0.00 | 1.74 | 0.00 | 0.88 | 17.77 | 324.77 | 3.28 | 345.85 | 0.2241 | 941.0 | 788.1 | |
| 0.00 | 2.17 | 0.00 | 1.11 | 18.02 | 324.39 | 2.91 | 347.65 | 0.2267 | 768.0 | 750.3 | |
| 1.57 | 1.65 | 0.80 | 0.84 | 18.94 | 324.25 | 2.77 | 349.05 | 0.2416 | 948.2 | 890.0 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 18.20 | 324.24 | 2.76 | 348.45 | 0.2293 | 930.0 | 775.9 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 18.82 | 324.09 | 2.61 | 349.57 | 0.2390 | 1033.0 | 766.0 | |
| 0.00 | 1.74 | 0.00 | 0.90 | 21.35 | 320.80 | -0.68 | 2.28 | 0.2782 | 844.0 | 669.5 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 16.76 | 317.02 | -4.46 | 20.51 | 0.2136 | -900.0 | -676.2 | |
| 0.00 | 1.65 | 0.00 | 0.84 | 16.58 | 316.90 | -4.58 | 21.34 | 0.2114 | -880.0 | -608.4 | |
| 0.00 | 1.57 | 0.00 | 0.79 | 15.69 | 315.89 | -5.59 | 27.39 | 0.2047 | 992.0 | 816.5 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 15.99 | 315.54 | -5.94 | 28.12 | 0.2120 | 948.0 | 665.4 | |
| 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. | |