SDO HMI 2014-05-29 22:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.90 | 38.05 | 7.63 | 22.16 | -19.87 | 50.77 | 25.39 | 230.39 | 0.5236 | 51.2 | 103.7 | |
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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 |
| 11.10 | 17.78 | 6.61 | 10.59 | -19.51 | 54.17 | 28.79 | 234.81 | 0.5576 | 839.8 | 640.2 | |
| 0.00 | 4.60 | 0.00 | 2.72 | -18.90 | 53.54 | 28.16 | 235.23 | 0.5457 | 847.0 | 791.1 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -14.80 | 52.39 | 27.01 | 241.24 | 0.5029 | 819.0 | 636.3 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -19.20 | 52.18 | 26.80 | 233.53 | 0.5316 | 694.0 | 590.5 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -19.95 | 50.62 | 25.24 | 230.80 | 0.5193 | -512.0 | -452.5 | |
| 1.44 | 2.71 | 0.82 | 1.54 | -19.60 | 48.69 | 23.31 | 229.26 | 0.4939 | -924.6 | -761.3 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -19.86 | 48.41 | 23.03 | 228.52 | 0.4931 | -846.0 | -751.3 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -24.00 | 48.62 | 23.24 | 222.55 | 0.5351 | 669.0 | 578.1 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -19.77 | 46.00 | 20.62 | 225.68 | 0.4650 | -899.0 | -800.6 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -20.51 | 46.10 | 20.72 | 224.61 | 0.4737 | -643.0 | -459.8 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -21.92 | 42.59 | 17.21 | 217.44 | 0.4534 | -796.0 | -650.5 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -21.82 | 42.34 | 16.96 | 217.19 | 0.4499 | -702.0 | -590.0 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -22.28 | 41.23 | 15.85 | 214.75 | 0.4453 | -625.0 | -455.1 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -22.32 | 40.49 | 15.11 | 213.46 | 0.4391 | -796.0 | -641.7 | |
| 0.36 | 1.62 | 0.20 | 0.88 | -21.58 | 38.39 | 13.01 | 210.69 | 0.4117 | -789.0 | -656.6 | |
| 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. | |