SDO HMI 2011-12-02 07:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.19 | 179.81 | 20.37 | 130.34 | 19.40 | 104.69 | -43.96 | 63.74 | 0.7325 | -735.4 | -269.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.73 | 0.00 | 2.02 | 23.59 | 105.33 | -43.32 | 58.10 | 0.7429 | -763.0 | -619.0 | |
| 0.00 | 1.28 | 0.00 | 0.95 | 23.84 | 105.09 | -43.56 | 57.90 | 0.7464 | -652.0 | -490.3 | |
| 0.00 | 1.03 | 0.00 | 0.76 | 23.33 | 105.13 | -43.52 | 58.52 | 0.7438 | -669.0 | -554.7 | |
| 0.00 | 0.94 | 0.00 | 0.69 | 23.04 | 104.98 | -43.67 | 58.95 | 0.7440 | -584.0 | -466.4 | |
| 0.00 | 1.96 | 0.00 | 1.47 | 23.52 | 104.60 | -44.05 | 58.53 | 0.7499 | -709.0 | -563.2 | |
| 0.00 | 1.37 | 0.00 | 1.05 | 24.67 | 103.45 | -45.20 | 57.62 | 0.7659 | -675.0 | -470.8 | |
| 0.00 | 1.20 | 0.00 | 0.94 | 26.10 | 102.56 | -46.09 | 56.29 | 0.7800 | -516.0 | -358.4 | |
| 0.94 | 158.97 | 0.67 | 114.74 | 19.00 | 105.24 | -43.42 | 64.04 | 0.7251 | -1197.3 | -273.4 | |
| 0.00 | 1.79 | 0.00 | 1.34 | 22.14 | 103.82 | -44.83 | 60.59 | 0.7520 | -506.0 | -477.3 | |
| 26.14 | -8.00 | 18.87 | -8.00 | 18.96 | 104.77 | -43.88 | 64.27 | 0.7300 | -956.5 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.71 | 22.42 | 103.21 | -45.45 | 60.50 | 0.7592 | 625.0 | 605.4 | |
| 1.11 | 5.21 | 0.83 | 3.89 | 21.47 | 103.55 | -45.10 | 61.55 | 0.7521 | 525.3 | 361.6 | |
| 0.00 | 1.54 | 0.00 | 1.15 | 20.45 | 103.27 | -45.39 | 62.94 | 0.7513 | -717.0 | -590.1 | |
| 0.00 | 0.85 | 0.00 | 0.63 | 18.92 | 103.07 | -45.59 | 64.98 | 0.7481 | 512.0 | 398.5 | |
| 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. | |