SDO HMI 2013-09-21 10:59:04 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.89 | 415.51 | 48.66 | 263.30 | -17.69 | 58.40 | -29.84 | 130.40 | 0.6246 | 781.3 | 285.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.62 | -18.79 | 59.01 | -29.23 | 132.33 | 0.6277 | -98.0 | -67.5 | |
| 72.10 | 400.19 | 45.50 | 252.88 | -17.65 | 58.64 | -29.60 | 130.55 | 0.6218 | 1065.3 | 307.2 | |
| 2.66 | -2.00 | 1.69 | -2.00 | -18.20 | 58.24 | -30.00 | 130.88 | 0.6305 | 487.1 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.53 | -20.08 | 56.66 | -31.58 | 131.75 | 0.6616 | -608.0 | -516.0 | |
| 0.00 | 1.59 | 0.00 | 1.03 | -18.19 | 56.95 | -31.29 | 129.70 | 0.6435 | 553.0 | 422.1 | |
| 0.00 | 0.71 | 0.00 | 0.46 | -16.54 | 54.66 | -33.57 | 125.68 | 0.6549 | -560.0 | -427.9 | |
| 0.00 | 0.97 | 0.00 | 0.67 | -19.74 | 52.97 | -35.26 | 128.33 | 0.6950 | -551.0 | -483.9 | |
| 0.00 | 2.04 | 0.00 | 1.39 | -18.73 | 52.60 | -35.64 | 126.83 | 0.6917 | -660.0 | -495.3 | |
| 0.00 | 0.71 | 0.00 | 0.50 | -21.16 | 51.95 | -36.29 | 129.23 | 0.7149 | -533.0 | -433.9 | |
| 0.80 | 2.13 | 0.54 | 1.44 | -16.81 | 52.23 | -36.01 | 124.18 | 0.6826 | -742.1 | -629.3 | |
| 0.62 | 1.95 | 0.42 | 1.32 | -16.58 | 51.89 | -36.35 | 123.64 | 0.6847 | -736.7 | -587.8 | |
| 0.00 | 0.97 | 0.00 | 0.66 | -15.61 | 51.28 | -36.96 | 121.99 | 0.6851 | -715.0 | -564.1 | |
| 0.71 | 2.48 | 0.51 | 1.80 | -19.23 | 48.80 | -39.44 | 124.77 | 0.7325 | 738.5 | 607.0 | |
| 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. | |