SDO HMI 2011-10-23 02:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.48 | 23.51 | 0.75 | 11.95 | 17.12 | 323.78 | 5.05 | 337.92 | 0.2287 | 611.1 | 498.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.48 | 1.65 | 0.75 | 0.83 | 13.15 | 326.03 | 7.30 | 318.08 | 0.1861 | 893.2 | 996.5 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 17.66 | 325.91 | 7.18 | 331.06 | 0.2473 | -881.0 | -668.2 | |
| 0.00 | 1.22 | 0.00 | 0.61 | 13.93 | 325.62 | 6.89 | 322.42 | 0.1919 | 800.0 | 579.6 | |
| 0.00 | 1.83 | 0.00 | 0.92 | 13.88 | 325.47 | 6.74 | 322.85 | 0.1895 | 695.0 | 575.6 | |
| 0.00 | 1.74 | 0.00 | 0.89 | 17.80 | 324.97 | 6.24 | 334.55 | 0.2420 | 981.0 | 777.5 | |
| 0.00 | 2.00 | 0.00 | 1.02 | 17.68 | 324.68 | 5.95 | 335.36 | 0.2381 | 777.0 | 519.2 | |
| 0.00 | 2.00 | 0.00 | 1.02 | 17.89 | 324.60 | 5.87 | 336.06 | 0.2408 | 969.0 | 736.8 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 18.94 | 324.31 | 5.58 | 338.76 | 0.2552 | 978.0 | 804.8 | |
| 0.00 | 1.57 | 0.00 | 0.80 | 17.99 | 324.22 | 5.49 | 337.59 | 0.2397 | 908.0 | 705.3 | |
| 0.00 | 1.57 | 0.00 | 0.80 | 18.81 | 324.09 | 5.36 | 339.36 | 0.2519 | 929.0 | 748.5 | |
| 0.00 | 2.26 | 0.00 | 1.16 | 18.91 | 323.81 | 5.08 | 340.49 | 0.2518 | 484.0 | 514.8 | |
| 0.00 | 2.44 | 0.00 | 1.24 | 18.51 | 323.70 | 4.97 | 340.30 | 0.2448 | 906.0 | 737.8 | |
| 0.00 | 1.57 | 0.00 | 0.79 | 16.54 | 316.64 | -2.09 | 10.13 | 0.1996 | -809.0 | -638.8 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 15.78 | 316.06 | -2.67 | 13.80 | 0.1889 | 996.0 | 705.2 | |
| 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. | |