SDO HMI 2014-07-09 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.77 | 384.24 | 46.84 | 301.06 | -19.14 | 254.35 | 46.10 | 241.46 | 0.7770 | 858.1 | 253.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.64 | 0.00 | 1.57 | -20.74 | 263.02 | 54.77 | 243.03 | 0.8591 | 495.0 | 449.3 | |
| 0.00 | 0.82 | 0.00 | 0.68 | -21.15 | 256.32 | 48.06 | 239.99 | 0.8034 | -208.0 | -224.3 | |
| 56.59 | 370.51 | 44.37 | 290.27 | -19.06 | 254.39 | 46.14 | 241.58 | 0.7771 | 1117.2 | 264.2 | |
| 1.27 | -3.00 | 0.98 | -3.00 | -19.09 | 253.71 | 45.45 | 241.23 | 0.7705 | 1218.6 | 999999 | |
| 1.91 | 4.54 | 1.49 | 3.54 | -21.42 | 253.09 | 44.83 | 238.16 | 0.7749 | 738.0 | 451.3 | |
| 0.00 | 1.09 | 0.00 | 0.82 | -19.35 | 252.20 | 43.94 | 240.19 | 0.7568 | 353.0 | 324.0 | |
| 0.00 | 0.64 | 0.00 | 0.50 | -22.34 | 252.76 | 44.51 | 236.91 | 0.7761 | -335.0 | -306.9 | |
| 0.00 | 0.82 | 0.00 | 0.63 | -22.45 | 252.25 | 44.00 | 236.52 | 0.7719 | -571.0 | -459.2 | |
| 0.00 | 0.82 | 0.00 | 0.63 | -22.40 | 251.82 | 43.56 | 236.35 | 0.7676 | -497.0 | -417.1 | |
| 0.00 | 0.36 | 0.00 | 0.28 | -22.26 | 251.72 | 43.46 | 236.46 | 0.7660 | -637.0 | -598.2 | |
| 0.00 | 0.82 | 0.00 | 0.60 | -20.62 | 250.31 | 42.06 | 237.67 | 0.7443 | -650.0 | -606.1 | |
| 0.00 | 0.91 | 0.00 | 0.65 | -20.57 | 248.65 | 40.39 | 236.78 | 0.7275 | -605.0 | -538.7 | |
| 0.00 | 1.27 | 0.00 | 0.89 | -20.77 | 247.05 | 38.80 | 235.58 | 0.7125 | -434.0 | -343.2 | |
| 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. | |