SDO HMI 2011-10-22 17:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.09 | 21.80 | 1.06 | 11.05 | 16.69 | 322.33 | -1.36 | 4.95 | 0.2095 | 534.6 | 455.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.00 | 0.00 | 1.00 | 14.24 | 326.05 | 2.36 | 345.59 | 0.1613 | 775.0 | 604.9 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 13.84 | 325.84 | 2.14 | 346.28 | 0.1538 | 858.0 | 639.6 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 12.91 | 325.77 | 2.07 | 345.10 | 0.1379 | 881.0 | 685.6 | |
| 0.00 | 1.48 | 0.00 | 0.74 | 13.84 | 325.62 | 1.93 | 347.61 | 0.1530 | 907.0 | 761.6 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 18.00 | 324.94 | 1.25 | 354.62 | 0.2220 | 1063.0 | 821.4 | |
| 2.09 | 2.26 | 1.06 | 1.15 | 18.95 | 324.22 | 0.53 | 357.88 | 0.2374 | 977.0 | 865.5 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 18.83 | 324.00 | 0.31 | 358.75 | 0.2352 | 984.0 | 854.3 | |
| 0.00 | 1.48 | 0.00 | 0.75 | 18.68 | 323.87 | 0.18 | 359.25 | 0.2326 | 988.0 | 856.1 | |
| 0.00 | 2.43 | 0.00 | 1.24 | 18.68 | 322.80 | -0.89 | 3.63 | 0.2330 | 934.0 | 638.4 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 16.90 | 321.88 | -1.81 | 8.55 | 0.2045 | 825.0 | 645.9 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 16.75 | 316.88 | -6.81 | 29.68 | 0.2303 | -1073.0 | -805.1 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 16.50 | 316.80 | -6.89 | 30.54 | 0.2275 | -915.0 | -816.9 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 16.75 | 316.70 | -7.00 | 30.35 | 0.2319 | -771.0 | -580.2 | |
| 0.00 | 2.17 | 0.00 | 1.11 | 15.86 | 315.82 | -7.87 | 35.58 | 0.2274 | 1025.0 | 772.0 | |
| 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. | |