SDO HMI 2014-05-28 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.90 | 75.85 | 13.23 | 40.38 | -19.24 | 51.70 | 11.43 | 210.83 | 0.3666 | 128.8 | 565.9 | |
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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 | 2.17 | 0.00 | 1.17 | -19.92 | 54.86 | 14.59 | 216.21 | 0.4025 | 631.0 | 428.1 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -19.41 | 53.42 | 13.15 | 214.27 | 0.3826 | 584.0 | 403.3 | |
| 10.83 | 41.86 | 5.78 | 22.33 | -19.06 | 52.90 | 12.62 | 213.76 | 0.3733 | 1181.6 | 836.0 | |
| 0.00 | 2.17 | 0.00 | 1.15 | -18.55 | 52.53 | 12.26 | 213.81 | 0.3632 | 1005.0 | 863.1 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -19.70 | 52.22 | 11.95 | 211.37 | 0.3759 | 657.0 | 527.7 | |
| 0.00 | 1.62 | 0.00 | 0.86 | -18.49 | 52.10 | 11.83 | 212.99 | 0.3585 | 895.0 | 763.9 | |
| 0.00 | 1.62 | 0.00 | 0.87 | -19.35 | 52.03 | 11.76 | 211.50 | 0.3695 | 832.0 | 714.9 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -18.40 | 51.77 | 11.49 | 212.41 | 0.3543 | 849.0 | 709.2 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -17.28 | 51.51 | 11.23 | 213.65 | 0.3369 | 781.0 | 559.3 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -16.97 | 50.61 | 10.33 | 212.06 | 0.3246 | 751.0 | 619.8 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -19.07 | 50.25 | 9.97 | 207.91 | 0.3511 | -756.0 | -617.2 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -19.52 | 49.52 | 9.24 | 205.58 | 0.3522 | -852.0 | -669.9 | |
| 14.07 | 18.04 | 7.45 | 9.55 | -19.77 | 49.05 | 8.77 | 204.11 | 0.3527 | -1083.0 | -730.1 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -22.27 | 41.84 | 1.56 | 183.99 | 0.3637 | -888.0 | -724.5 | |
| 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. | |