SDO HMI 2014-05-19 09:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.13 | 245.33 | 23.30 | 145.78 | -24.58 | 190.65 | 25.79 | 225.77 | 0.5542 | 647.4 | 312.8 | |
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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 |
| 35.80 | 225.71 | 21.31 | 134.36 | -24.42 | 191.02 | 26.16 | 226.41 | 0.5563 | 1226.9 | 378.3 | |
| 0.00 | 1.53 | 0.00 | 0.90 | -23.35 | 190.72 | 25.85 | 227.68 | 0.5436 | 258.0 | 225.8 | |
| 3.33 | -1.00 | 1.99 | -1.00 | -24.92 | 190.91 | 26.05 | 225.60 | 0.5596 | 811.2 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.11 | -23.92 | 189.70 | 24.83 | 225.78 | 0.5378 | 634.0 | 457.7 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -24.24 | 189.69 | 24.83 | 225.30 | 0.5408 | 821.0 | 749.5 | |
| 0.00 | 1.80 | 0.00 | 1.04 | -24.38 | 186.96 | 22.10 | 222.01 | 0.5140 | -588.0 | -352.5 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -26.00 | 186.25 | 21.39 | 218.89 | 0.5241 | -790.0 | -640.8 | |
| 0.00 | 1.89 | 0.00 | 1.09 | -25.91 | 185.69 | 20.83 | 218.32 | 0.5179 | -912.0 | -751.2 | |
| 0.00 | 2.16 | 0.00 | 1.26 | -27.25 | 185.69 | 20.83 | 216.58 | 0.5325 | -618.0 | -486.7 | |
| 0.00 | 2.70 | 0.00 | 1.58 | -27.49 | 185.30 | 20.43 | 215.79 | 0.5317 | -688.0 | -525.6 | |
| 0.00 | 1.62 | 0.00 | 0.94 | -27.42 | 185.07 | 20.20 | 215.58 | 0.5290 | -908.0 | -736.1 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -27.10 | 184.21 | 19.35 | 214.87 | 0.5179 | -751.0 | -635.8 | |
| 0.00 | 1.80 | 0.00 | 1.04 | -26.90 | 183.60 | 18.73 | 214.29 | 0.5104 | -755.0 | -640.9 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -27.01 | 182.54 | 17.68 | 212.69 | 0.5029 | -610.0 | -387.0 | |
| 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. | |