SDO HMI 2014-05-16 06:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.29 | 24.82 | 7.08 | 27.46 | -18.22 | 143.44 | -62.74 | 109.17 | 0.8947 | 276.6 | 148.4 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.85 | -16.46 | 152.30 | -53.89 | 108.42 | 0.8187 | 371.0 | 333.3 | |
| 0.00 | 1.53 | 0.00 | 1.55 | -19.26 | 146.32 | -59.87 | 110.70 | 0.8747 | 535.0 | 476.1 | |
| 0.00 | 1.17 | 0.00 | 1.16 | -16.74 | 146.78 | -59.40 | 107.89 | 0.8682 | 551.0 | 391.4 | |
| 0.00 | 0.90 | 0.00 | 0.96 | -18.58 | 144.49 | -61.70 | 109.68 | 0.8882 | 151.0 | 144.9 | |
| 0.00 | 2.34 | 0.00 | 2.51 | -18.35 | 144.36 | -61.83 | 109.40 | 0.8890 | 333.0 | 158.5 | |
| 0.00 | 1.98 | 0.00 | 2.12 | -18.04 | 144.35 | -61.83 | 109.05 | 0.8887 | 149.0 | 117.8 | |
| 0.00 | 1.44 | 0.00 | 1.59 | -18.39 | 143.51 | -62.68 | 109.33 | 0.8953 | 208.0 | 213.3 | |
| 6.29 | 11.05 | 7.08 | 12.45 | -18.30 | 142.93 | -63.26 | 109.17 | 0.8995 | 426.5 | 248.9 | |
| 0.00 | 2.70 | 0.00 | 3.08 | -18.15 | 142.45 | -63.74 | 108.95 | 0.9028 | -252.0 | -230.8 | |
| 0.00 | 0.27 | 0.00 | 0.43 | -18.37 | 134.20 | -71.99 | 108.49 | 0.9530 | -174.0 | -159.7 | |
| 0.00 | 0.45 | 0.00 | 0.76 | -18.55 | 133.25 | -72.94 | 108.63 | 0.9577 | -168.0 | -171.4 | |
| 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. | |