SDO HMI 2014-05-19 04:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.46 | 252.59 | 24.72 | 147.01 | -24.44 | 190.84 | 23.24 | 223.27 | 0.5262 | 668.9 | 321.8 | |
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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 |
| 40.21 | 235.31 | 23.42 | 137.09 | -24.36 | 191.14 | 23.54 | 223.76 | 0.5282 | 1196.1 | 375.5 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -21.00 | 190.33 | 22.73 | 227.99 | 0.4874 | -726.0 | -608.4 | |
| 2.25 | -1.00 | 1.30 | -1.00 | -24.08 | 190.40 | 22.80 | 223.32 | 0.5177 | 934.5 | 999999 | |
| 0.00 | 3.42 | 0.00 | 2.01 | -26.22 | 190.61 | 23.00 | 220.56 | 0.5413 | 32.0 | 178.5 | |
| 0.00 | 1.26 | 0.00 | 0.73 | -24.15 | 189.95 | 22.34 | 222.68 | 0.5138 | 806.0 | 660.7 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -24.25 | 189.78 | 22.18 | 222.34 | 0.5132 | 824.0 | 614.7 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -22.32 | 187.27 | 19.67 | 221.99 | 0.4674 | -604.0 | -419.4 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -24.55 | 186.21 | 18.61 | 217.23 | 0.4816 | -571.0 | -468.9 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -27.14 | 185.77 | 18.17 | 213.25 | 0.5081 | -572.0 | -501.0 | |
| 0.00 | 2.88 | 0.00 | 1.64 | -26.35 | 185.25 | 17.65 | 213.49 | 0.4943 | -835.0 | -742.3 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -28.77 | 185.47 | 17.87 | 210.94 | 0.5252 | -594.0 | -517.5 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -27.45 | 185.21 | 17.61 | 212.10 | 0.5073 | -856.0 | -816.6 | |
| 0.00 | 1.35 | 0.00 | 0.77 | -27.13 | 184.19 | 16.59 | 211.02 | 0.4952 | -891.0 | -718.8 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -27.17 | 183.03 | 15.43 | 209.22 | 0.4868 | -676.0 | -475.8 | |
| 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. | |