SDO HMI 2014-05-19 12:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.83 | 237.90 | 24.64 | 143.41 | -24.59 | 190.60 | 27.38 | 227.29 | 0.5713 | 745.9 | 293.1 | |
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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 |
| 39.21 | 222.33 | 23.67 | 134.23 | -24.45 | 190.96 | 27.74 | 227.87 | 0.5734 | 1187.8 | 357.7 | |
| 1.62 | -1.00 | 0.97 | -1.00 | -24.26 | 190.46 | 27.24 | 227.68 | 0.5665 | 1188.3 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.83 | -26.84 | 190.60 | 27.39 | 224.25 | 0.5903 | 478.0 | 425.5 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -22.35 | 189.56 | 26.35 | 229.65 | 0.5406 | -414.0 | -320.0 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -25.94 | 186.16 | 22.94 | 220.82 | 0.5383 | -780.0 | -688.8 | |
| 0.00 | 1.35 | 0.00 | 0.79 | -26.31 | 185.91 | 22.69 | 220.03 | 0.5397 | -644.0 | -519.7 | |
| 0.00 | 1.89 | 0.00 | 1.11 | -25.98 | 185.73 | 22.51 | 220.27 | 0.5346 | -875.0 | -749.4 | |
| 0.00 | 5.04 | 0.00 | 2.97 | -27.18 | 185.46 | 22.24 | 218.37 | 0.5446 | -515.0 | -643.8 | |
| 0.00 | 1.53 | 0.00 | 0.90 | -27.59 | 185.25 | 22.03 | 217.60 | 0.5470 | -545.0 | -465.4 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -28.98 | 185.37 | 22.15 | 216.03 | 0.5629 | -550.0 | -442.6 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -27.82 | 179.59 | 16.37 | 209.87 | 0.5027 | -332.0 | -362.7 | |
| 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. | |