SDO HMI 2011-10-24 01:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.64 | 0.00 | 10.41 | 18.00 | 321.66 | 15.57 | 310.48 | 0.3514 | 807.6 | 666.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.30 | 0.00 | 0.69 | 14.45 | 325.45 | 19.36 | 297.34 | 0.3630 | 855.0 | 642.3 | |
| 0.00 | 1.30 | 0.00 | 0.70 | 17.17 | 324.83 | 18.74 | 304.66 | 0.3748 | 803.0 | 679.7 | |
| 0.00 | 2.43 | 0.00 | 1.30 | 16.91 | 324.48 | 18.38 | 304.52 | 0.3679 | 783.0 | 615.1 | |
| 0.00 | 1.30 | 0.00 | 0.70 | 17.79 | 324.37 | 18.28 | 306.71 | 0.3741 | 932.0 | 764.0 | |
| 0.00 | 1.13 | 0.00 | 0.60 | 19.19 | 323.76 | 17.67 | 310.65 | 0.3795 | 668.0 | 515.1 | |
| 0.00 | 2.00 | 0.00 | 1.04 | 12.91 | 321.85 | 15.76 | 297.50 | 0.2998 | 919.0 | 829.1 | |
| 0.00 | 2.78 | 0.00 | 1.44 | 12.62 | 321.71 | 15.62 | 296.79 | 0.2956 | 1013.0 | 765.0 | |
| 0.00 | 0.26 | 0.00 | 0.14 | 19.68 | 321.60 | 15.51 | 315.18 | 0.3588 | 685.0 | 632.3 | |
| 0.00 | 1.48 | 0.00 | 0.77 | 16.50 | 321.03 | 14.93 | 308.88 | 0.3188 | 825.0 | 647.5 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 19.75 | 319.64 | 13.55 | 319.02 | 0.3378 | 802.0 | 641.4 | |
| 0.00 | 1.65 | 0.00 | 0.88 | 22.46 | 319.10 | 13.01 | 325.18 | 0.3660 | 796.0 | 640.1 | |
| 0.00 | 0.78 | 0.00 | 0.41 | 21.29 | 318.60 | 12.51 | 324.16 | 0.3462 | 769.0 | 622.6 | |
| 0.00 | 1.57 | 0.00 | 0.85 | 26.05 | 318.02 | 11.93 | 332.58 | 0.4050 | 779.0 | 582.1 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 27.85 | 313.90 | 7.81 | 342.72 | 0.4061 | 678.0 | 520.9 | |
| 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. | |