SDO HMI 2011-11-14 05:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.07 | 170.36 | 77.01 | 454.78 | 19.08 | 106.51 | 79.51 | 288.87 | 0.9824 | -156.8 | -48.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.60 | 89.57 | 26.44 | 280.89 | 19.10 | 108.14 | 81.14 | 288.87 | 0.9875 | 410.4 | 188.3 | |
| 8.86 | -1.00 | 25.87 | -1.00 | 19.06 | 107.65 | 80.65 | 288.84 | 0.9862 | -310.0 | 999999 | |
| 0.00 | 1.38 | 0.00 | 3.55 | 18.94 | 106.29 | 79.30 | 288.72 | 0.9822 | -349.0 | -306.8 | |
| 0.43 | 50.76 | 1.00 | 109.57 | 18.62 | 105.09 | 78.09 | 288.42 | 0.9782 | -443.2 | -441.6 | |
| 0.00 | 2.15 | 0.00 | 5.51 | 19.42 | 106.15 | 79.16 | 289.21 | 0.9818 | -467.0 | -415.9 | |
| 4.04 | -4.00 | 9.01 | -4.00 | 18.53 | 104.48 | 77.48 | 288.33 | 0.9761 | -573.1 | 999999 | |
| 0.00 | 1.03 | 0.00 | 2.64 | 20.27 | 106.24 | 79.24 | 290.08 | 0.9821 | -339.0 | -273.9 | |
| 7.14 | 11.79 | 14.69 | 24.42 | 19.47 | 103.22 | 76.22 | 289.33 | 0.9715 | -504.5 | -467.4 | |
| 0.00 | 1.98 | 0.00 | 4.15 | 20.15 | 103.56 | 76.56 | 290.01 | 0.9729 | -564.0 | -522.9 | |
| 0.00 | 3.36 | 0.00 | 7.81 | 21.38 | 104.93 | 77.93 | 291.24 | 0.9779 | -401.0 | -317.0 | |
| 0.00 | 1.81 | 0.00 | 3.60 | 20.22 | 102.72 | 75.73 | 290.12 | 0.9696 | -416.0 | -386.6 | |
| 0.00 | 1.63 | 0.00 | 3.25 | 20.44 | 102.66 | 75.67 | 290.35 | 0.9694 | -385.0 | -375.6 | |
| 0.00 | 2.15 | 0.00 | 4.25 | 20.73 | 102.57 | 75.58 | 290.65 | 0.9691 | -369.0 | -319.6 | |
| 0.00 | 2.75 | 0.00 | 5.14 | 20.11 | 101.69 | 74.69 | 290.05 | 0.9653 | -12.0 | -24.0 | |
| 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. | |