SDO HMI 2014-05-27 20:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.97 | 155.11 | 14.67 | 87.80 | -8.84 | 24.85 | -28.11 | 106.24 | 0.4867 | 683.1 | 420.7 | |
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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 |
| 1.98 | 135.92 | 1.12 | 76.58 | -8.61 | 25.53 | -27.42 | 106.07 | 0.4758 | 1200.9 | 471.7 | |
| 20.20 | -1.00 | 11.39 | -1.00 | -8.85 | 25.34 | -27.62 | 106.47 | 0.4796 | 1191.1 | 999999 | |
| 3.25 | -1.00 | 1.84 | -1.00 | -8.81 | 24.96 | -28.00 | 106.21 | 0.4850 | 799.3 | 999999 | |
| 0.00 | 2.07 | 0.00 | 1.18 | -8.84 | 24.47 | -28.49 | 106.03 | 0.4923 | 602.0 | 446.3 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -8.07 | 24.43 | -28.53 | 104.48 | 0.4904 | 728.0 | 537.9 | |
| 0.00 | 1.53 | 0.00 | 0.87 | -8.01 | 24.15 | -28.80 | 104.24 | 0.4942 | 706.0 | 565.7 | |
| 0.54 | 5.32 | 0.32 | 3.09 | -9.61 | 22.23 | -30.72 | 106.49 | 0.5274 | 709.7 | 725.3 | |
| 0.00 | 1.53 | 0.00 | 0.89 | -9.40 | 22.18 | -30.77 | 106.07 | 0.5274 | 765.0 | 698.2 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -5.86 | 20.61 | -32.35 | 99.01 | 0.5410 | -632.0 | -413.6 | |
| 0.00 | 2.53 | 0.00 | 1.51 | -9.64 | 19.61 | -33.35 | 105.49 | 0.5645 | -581.0 | -612.0 | |
| 0.00 | 1.17 | 0.00 | 0.70 | -9.46 | 19.63 | -33.33 | 105.17 | 0.5637 | -727.0 | -669.0 | |
| 0.00 | 1.80 | 0.00 | 1.08 | -8.91 | 19.65 | -33.30 | 104.22 | 0.5617 | -777.0 | -599.8 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -9.49 | 19.40 | -33.55 | 105.14 | 0.5669 | -550.0 | -506.4 | |
| 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. | |