SDO HMI 2014-05-28 02:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.57 | 162.78 | 17.92 | 89.58 | -8.88 | 24.85 | -24.78 | 108.22 | 0.4377 | 759.9 | 417.7 | |
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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 |
| 25.45 | 140.51 | 13.95 | 76.99 | -8.85 | 25.39 | -24.24 | 108.46 | 0.4295 | 1251.0 | 450.6 | |
| 2.17 | -1.00 | 1.19 | -1.00 | -8.84 | 24.95 | -24.68 | 108.17 | 0.4361 | 850.8 | 999999 | |
| 1.53 | -1.00 | 0.85 | -1.00 | -8.81 | 24.72 | -24.92 | 107.96 | 0.4394 | 691.3 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -7.67 | 24.49 | -25.14 | 105.31 | 0.4384 | 772.0 | 595.7 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -7.95 | 24.27 | -25.36 | 105.80 | 0.4427 | 779.0 | 604.5 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -8.47 | 24.13 | -25.50 | 106.86 | 0.4468 | 656.0 | 476.6 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -8.25 | 23.74 | -25.90 | 106.17 | 0.4519 | 803.0 | 633.5 | |
| 1.71 | 11.37 | 0.96 | 6.40 | -9.65 | 22.63 | -27.01 | 108.49 | 0.4739 | 959.2 | 733.5 | |
| 1.71 | -8.00 | 0.97 | -8.00 | -9.58 | 22.32 | -27.31 | 108.19 | 0.4782 | 978.9 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.09 | -9.68 | 19.75 | -29.89 | 107.06 | 0.5158 | -831.0 | -691.3 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -8.76 | 19.80 | -29.83 | 105.34 | 0.5119 | -865.0 | -732.8 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -8.57 | 19.71 | -29.92 | 104.94 | 0.5126 | -723.0 | -541.2 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -8.44 | 18.97 | -30.66 | 104.40 | 0.5228 | -717.0 | -559.8 | |
| 0.00 | 0.36 | 0.00 | 0.21 | -9.15 | 18.55 | -31.09 | 105.54 | 0.5312 | -339.0 | -465.8 | |
| 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. | |