SDO HMI 2014-05-20 00:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.43 | 228.39 | 23.50 | 147.04 | -24.66 | 190.44 | 33.86 | 232.45 | 0.6410 | 574.4 | 303.6 | |
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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 |
| 36.43 | 212.10 | 23.50 | 136.80 | -24.51 | 190.71 | 34.13 | 232.86 | 0.6427 | 1058.8 | 351.6 | |
| 0.00 | 1.17 | 0.00 | 0.76 | -26.37 | 190.58 | 34.00 | 230.27 | 0.6537 | 559.0 | 514.3 | |
| 0.00 | 1.89 | 0.00 | 1.23 | -26.61 | 190.45 | 33.87 | 229.87 | 0.6540 | 621.0 | 554.7 | |
| 0.00 | 1.71 | 0.00 | 1.10 | -25.62 | 190.12 | 33.55 | 230.96 | 0.6439 | 130.0 | 206.6 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -24.66 | 185.84 | 29.26 | 228.90 | 0.5917 | -586.0 | -486.4 | |
| 0.00 | 1.08 | 0.00 | 0.66 | -24.47 | 185.71 | 29.14 | 229.06 | 0.5888 | -638.0 | -495.2 | |
| 0.00 | 1.35 | 0.00 | 0.84 | -26.35 | 185.79 | 29.21 | 226.53 | 0.6048 | -726.0 | -540.8 | |
| 0.00 | 2.16 | 0.00 | 1.34 | -26.56 | 185.61 | 29.04 | 226.10 | 0.6047 | -739.0 | -575.2 | |
| 0.00 | 1.98 | 0.00 | 1.24 | -27.33 | 185.56 | 28.98 | 225.03 | 0.6106 | -460.0 | -400.1 | |
| 0.00 | 1.35 | 0.00 | 0.84 | -27.91 | 185.10 | 28.52 | 223.87 | 0.6111 | -577.0 | -404.5 | |
| 0.00 | 0.72 | 0.00 | 0.45 | -27.57 | 185.00 | 28.43 | 224.22 | 0.6073 | -704.0 | -592.1 | |
| 0.00 | 0.81 | 0.00 | 0.50 | -26.98 | 183.99 | 27.41 | 224.05 | 0.5923 | -628.0 | -544.8 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -28.57 | 184.27 | 27.69 | 222.27 | 0.6090 | -742.0 | -615.2 | |
| 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. | |