SDO HMI 2014-05-18 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 |
| 42.70 | 266.67 | 23.59 | 147.27 | -24.23 | 191.19 | 14.74 | 211.72 | 0.4434 | 657.6 | 309.8 | |
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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 |
| 0.00 | 1.08 | 0.00 | 0.60 | -20.43 | 195.75 | 19.31 | 224.66 | 0.4426 | -653.0 | -565.7 | |
| 9.53 | 246.24 | 5.27 | 136.10 | -24.22 | 191.80 | 15.36 | 212.79 | 0.4477 | 1163.5 | 393.0 | |
| 15.10 | -2.00 | 8.33 | -2.00 | -23.96 | 191.53 | 15.08 | 212.69 | 0.4422 | 1388.5 | 999999 | |
| 18.07 | -2.00 | 9.99 | -2.00 | -24.32 | 191.40 | 14.95 | 211.99 | 0.4457 | 1213.2 | 999999 | |
| 0.00 | 2.25 | 0.00 | 1.23 | -24.13 | 190.04 | 13.59 | 209.89 | 0.4323 | 665.0 | 584.3 | |
| 0.00 | 2.34 | 0.00 | 1.27 | -24.12 | 187.18 | 10.74 | 204.53 | 0.4113 | -786.0 | -493.4 | |
| 0.00 | 3.42 | 0.00 | 1.86 | -24.52 | 186.51 | 10.06 | 202.75 | 0.4126 | -762.0 | -698.5 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -24.32 | 186.42 | 9.98 | 202.79 | 0.4093 | -985.0 | -789.8 | |
| 0.00 | 3.06 | 0.00 | 1.66 | -24.45 | 186.26 | 9.82 | 202.33 | 0.4102 | -640.0 | -782.4 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -25.67 | 186.16 | 9.71 | 200.93 | 0.4273 | -803.0 | -658.7 | |
| 0.00 | 2.43 | 0.00 | 1.33 | -25.84 | 185.66 | 9.21 | 199.80 | 0.4270 | -842.0 | -673.0 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -27.30 | 185.57 | 9.12 | 198.40 | 0.4481 | -754.0 | -616.6 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -27.95 | 184.55 | 8.10 | 196.02 | 0.4528 | -763.0 | -676.9 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -27.18 | 184.18 | 7.73 | 195.86 | 0.4398 | -746.0 | -689.7 | |
| 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. | |