SDO HMI 2014-05-27 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.16 | 139.52 | 15.24 | 81.59 | -8.78 | 24.95 | -31.33 | 104.70 | 0.5331 | 574.4 | 383.2 | |
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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 |
| 0.99 | 126.74 | 0.58 | 73.76 | -8.43 | 25.42 | -30.86 | 104.20 | 0.5255 | 820.7 | 441.7 | |
| 25.17 | -1.00 | 14.66 | -1.00 | -8.83 | 25.34 | -30.94 | 104.92 | 0.5278 | 1118.5 | 999999 | |
| 0.00 | 1.71 | 0.00 | 1.01 | -8.88 | 24.51 | -31.77 | 104.69 | 0.5399 | 682.0 | 588.6 | |
| 0.00 | 1.44 | 0.00 | 0.85 | -8.84 | 24.19 | -32.09 | 104.51 | 0.5444 | 522.0 | 440.2 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -4.26 | 23.95 | -32.33 | 96.02 | 0.5384 | -632.0 | -418.4 | |
| 0.00 | 1.17 | 0.00 | 0.71 | -9.07 | 22.44 | -33.84 | 104.29 | 0.5697 | 637.0 | 496.4 | |
| 0.00 | 1.26 | 0.00 | 0.77 | -9.09 | 21.76 | -34.52 | 104.10 | 0.5791 | 559.0 | 428.1 | |
| 0.00 | 0.72 | 0.00 | 0.44 | -7.15 | 20.76 | -35.52 | 100.53 | 0.5885 | -550.0 | -474.1 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -9.30 | 19.38 | -36.90 | 103.73 | 0.6122 | -617.0 | -524.3 | |
| 0.00 | 1.26 | 0.00 | 0.79 | -8.81 | 19.44 | -36.84 | 102.96 | 0.6102 | -652.0 | -451.9 | |
| 0.00 | 0.54 | 0.00 | 0.34 | -9.03 | 19.38 | -36.90 | 103.29 | 0.6115 | -631.0 | -535.3 | |
| 0.00 | 1.89 | 0.00 | 1.20 | -8.67 | 18.22 | -38.06 | 102.42 | 0.6263 | -498.0 | -402.4 | |
| 0.00 | 0.72 | 0.00 | 0.46 | -8.67 | 17.90 | -38.38 | 102.33 | 0.6305 | -620.0 | -545.5 | |
| 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. | |