SDO HMI 2014-09-29 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.60 | 92.92 | 22.25 | 95.70 | -9.53 | 266.90 | 59.07 | 254.93 | 0.8754 | 277.1 | 144.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.47 | 54.71 | 9.69 | 62.43 | -8.16 | 270.60 | 62.77 | 257.53 | 0.9033 | 601.1 | 206.1 | |
| 1.15 | -1.00 | 1.29 | -1.00 | -8.12 | 270.19 | 62.36 | 257.49 | 0.9002 | 884.3 | 999999 | |
| 0.00 | 1.06 | 0.00 | 1.09 | -8.22 | 267.37 | 59.55 | 256.72 | 0.8786 | 472.0 | 406.6 | |
| 0.00 | 1.06 | 0.00 | 0.96 | -10.45 | 262.14 | 54.32 | 252.75 | 0.8385 | 321.0 | 268.9 | |
| 0.00 | 3.97 | 0.00 | 3.56 | -10.63 | 261.77 | 53.94 | 252.42 | 0.8356 | 573.0 | 370.3 | |
| 3.62 | 14.74 | 3.23 | 13.10 | -11.28 | 261.37 | 53.54 | 251.54 | 0.8337 | 598.8 | 491.2 | |
| 4.24 | -6.00 | 3.75 | -6.00 | -11.34 | 261.02 | 53.20 | 251.36 | 0.8307 | 744.6 | 999999 | |
| 0.88 | 3.44 | 0.75 | 2.91 | -11.95 | 258.92 | 51.09 | 249.91 | 0.8128 | -581.4 | -401.8 | |
| 1.68 | 3.26 | 1.44 | 2.81 | -13.52 | 259.16 | 51.34 | 248.17 | 0.8201 | -576.7 | -424.8 | |
| 0.00 | 1.06 | 0.00 | 0.89 | -11.70 | 258.61 | 50.78 | 250.10 | 0.8091 | -267.0 | -290.8 | |
| 0.00 | 0.97 | 0.00 | 0.83 | -13.73 | 258.98 | 51.15 | 247.86 | 0.8190 | -588.0 | -547.1 | |
| 0.00 | 1.06 | 0.00 | 0.88 | -14.33 | 257.26 | 49.43 | 246.48 | 0.8049 | -600.0 | -561.8 | |
| 0.00 | 0.53 | 0.00 | 0.45 | -16.10 | 257.68 | 49.86 | 244.60 | 0.8152 | -613.0 | -595.8 | |
| 2.56 | 7.06 | 2.10 | 5.79 | -14.42 | 256.62 | 48.80 | 246.10 | 0.7992 | -771.3 | -558.6 | |
| 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. | |