SDO HMI 2011-11-14 00:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.96 | 232.42 | 62.97 | 495.73 | 19.04 | 106.57 | 76.83 | 288.87 | 0.9733 | -250.7 | -143.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.57 | 115.27 | 18.46 | 283.20 | 19.10 | 108.44 | 78.70 | 288.89 | 0.9803 | 346.8 | 121.2 | |
| 13.25 | -1.00 | 31.04 | -1.00 | 19.07 | 107.90 | 78.16 | 288.86 | 0.9785 | -415.3 | 999999 | |
| 0.00 | 2.41 | 0.00 | 5.18 | 18.81 | 106.74 | 77.01 | 288.62 | 0.9743 | -530.0 | -494.4 | |
| 0.00 | 4.13 | 0.00 | 8.62 | 19.34 | 106.27 | 76.53 | 289.17 | 0.9726 | -558.0 | -468.9 | |
| 2.15 | 86.10 | 4.18 | 155.36 | 18.61 | 105.12 | 75.38 | 288.46 | 0.9679 | -427.8 | -470.2 | |
| 0.00 | 1.12 | 0.00 | 1.90 | 17.03 | 102.94 | 73.20 | 286.89 | 0.9579 | -165.0 | -152.9 | |
| 4.65 | -5.00 | 8.66 | -5.00 | 18.48 | 104.47 | 74.73 | 288.35 | 0.9651 | -632.3 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.55 | 18.79 | 103.90 | 74.16 | 288.69 | 0.9627 | -585.0 | -592.0 | |
| 0.34 | -5.00 | 0.63 | -5.00 | 19.51 | 103.97 | 74.23 | 289.43 | 0.9631 | -398.8 | 999999 | |
| 0.00 | 4.47 | 0.00 | 8.00 | 20.12 | 103.70 | 73.96 | 290.08 | 0.9621 | -548.0 | -544.0 | |
| 0.00 | 5.42 | 0.00 | 10.47 | 21.33 | 105.02 | 75.28 | 291.27 | 0.9680 | -527.0 | -400.3 | |
| 0.00 | 1.72 | 0.00 | 2.96 | 19.90 | 103.08 | 73.34 | 289.88 | 0.9592 | -539.0 | -478.5 | |
| 0.00 | 10.92 | 0.00 | 18.49 | 20.52 | 102.73 | 72.99 | 290.54 | 0.9577 | -335.0 | -325.8 | |
| 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. | |