SDO HMI 2014-05-27 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.44 | 21.34 | 0.76 | 11.33 | -20.00 | 49.19 | -8.20 | 158.22 | 0.3525 | 323.3 | 298.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.71 | 0.00 | 0.90 | -19.03 | 52.48 | -4.90 | 165.21 | 0.3178 | 748.0 | 609.5 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -18.81 | 52.36 | -5.02 | 164.67 | 0.3147 | 742.0 | 564.9 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -18.87 | 51.62 | -5.77 | 162.60 | 0.3192 | 858.0 | 738.1 | |
| 0.54 | 3.88 | 0.28 | 2.03 | -19.06 | 51.54 | -5.84 | 162.59 | 0.3226 | 964.3 | 729.1 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -19.64 | 51.26 | -6.12 | 162.38 | 0.3330 | 806.0 | 590.2 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -19.83 | 51.13 | -6.26 | 162.20 | 0.3367 | 738.0 | 659.5 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -17.60 | 51.05 | -6.33 | 159.56 | 0.3023 | 812.0 | 619.2 | |
| 0.00 | 1.35 | 0.00 | 0.71 | -20.15 | 50.43 | -6.95 | 160.70 | 0.3453 | 864.0 | 723.3 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -20.28 | 49.84 | -7.55 | 159.33 | 0.3505 | 743.0 | 598.3 | |
| 0.90 | 1.98 | 0.48 | 1.05 | -19.57 | 49.48 | -7.90 | 157.64 | 0.3420 | -852.9 | -765.8 | |
| 0.00 | 1.89 | 0.00 | 1.01 | -21.85 | 48.79 | -8.59 | 158.54 | 0.3804 | 793.0 | 620.0 | |
| 0.00 | 1.44 | 0.00 | 0.78 | -20.61 | 45.14 | -12.24 | 149.15 | 0.3887 | -741.0 | -564.2 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -21.89 | 42.54 | -14.85 | 146.08 | 0.4278 | -769.0 | -525.5 | |
| 0.00 | 1.98 | 0.00 | 1.09 | -22.37 | 41.84 | -15.55 | 145.56 | 0.4401 | -794.0 | -565.7 | |
| 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. | |