SDO HMI 2014-05-19 11:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.04 | 239.72 | 23.45 | 143.78 | -24.64 | 190.59 | 26.82 | 226.70 | 0.5658 | 591.6 | 301.9 | |
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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 |
| 39.04 | 218.84 | 23.45 | 131.49 | -24.43 | 191.01 | 27.24 | 227.44 | 0.5679 | 1194.3 | 377.7 | |
| 0.00 | 2.16 | 0.00 | 1.32 | -26.79 | 190.64 | 26.87 | 223.83 | 0.5848 | 510.0 | 440.5 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -24.12 | 189.67 | 25.91 | 226.58 | 0.5511 | 637.0 | 493.8 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -24.32 | 189.68 | 25.91 | 226.30 | 0.5529 | 746.0 | 538.3 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -24.39 | 186.91 | 23.14 | 223.22 | 0.5248 | -649.0 | -539.9 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -25.95 | 186.20 | 22.43 | 220.21 | 0.5335 | -835.0 | -682.8 | |
| 0.00 | 1.98 | 0.00 | 1.16 | -27.19 | 185.61 | 21.84 | 217.88 | 0.5410 | -654.0 | -595.0 | |
| 0.00 | 2.16 | 0.00 | 1.27 | -27.06 | 185.36 | 21.59 | 217.75 | 0.5374 | -795.0 | -699.5 | |
| 0.00 | 2.25 | 0.00 | 1.32 | -27.57 | 185.28 | 21.51 | 217.01 | 0.5421 | -618.0 | -515.0 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -27.40 | 185.06 | 21.29 | 216.95 | 0.5384 | -760.0 | -721.8 | |
| 0.00 | 1.89 | 0.00 | 1.12 | -28.31 | 185.03 | 21.26 | 215.78 | 0.5481 | -662.0 | -590.4 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -28.58 | 184.97 | 21.21 | 215.39 | 0.5506 | -539.0 | -435.0 | |
| 0.00 | 1.44 | 0.00 | 0.84 | -27.11 | 184.31 | 20.54 | 216.39 | 0.5285 | -711.0 | -497.3 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -26.92 | 183.58 | 19.82 | 215.71 | 0.5200 | -784.0 | -608.7 | |
| 0.00 | 1.44 | 0.00 | 0.83 | -27.12 | 183.51 | 19.74 | 215.36 | 0.5217 | -737.0 | -520.3 | |
| 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. | |