SDO HMI 2014-05-19 09:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.36 | 186.85 | 30.99 | 110.62 | -16.87 | 195.04 | 30.18 | 241.74 | 0.5479 | 60.3 | -0.0 | |
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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 | 0.27 | 0.00 | 0.17 | -16.31 | 198.98 | 34.12 | 245.05 | 0.5959 | -504.0 | -480.7 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -19.17 | 197.94 | 33.07 | 239.96 | 0.5976 | 651.0 | 524.1 | |
| 0.00 | 2.61 | 0.00 | 1.57 | -17.17 | 196.80 | 31.94 | 242.41 | 0.5724 | 720.0 | 595.5 | |
| 22.49 | 90.86 | 13.60 | 54.93 | -17.86 | 196.71 | 31.85 | 241.23 | 0.5751 | 1003.6 | 349.4 | |
| 4.23 | -4.00 | 2.54 | -4.00 | -17.24 | 196.33 | 31.46 | 241.99 | 0.5668 | 1001.1 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -17.22 | 195.36 | 30.50 | 241.37 | 0.5544 | 701.0 | 602.3 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -16.79 | 194.91 | 30.05 | 241.79 | 0.5462 | 896.0 | 813.2 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -16.44 | 193.65 | 28.79 | 241.50 | 0.5277 | -213.0 | -268.1 | |
| 9.63 | 85.19 | 5.57 | 49.34 | -15.57 | 193.37 | 28.51 | 242.83 | 0.5189 | -1094.9 | -421.8 | |
| 16.01 | -9.00 | 9.28 | -9.00 | -16.13 | 193.28 | 28.42 | 241.76 | 0.5210 | -1022.2 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -14.92 | 192.81 | 27.95 | 243.60 | 0.5077 | 452.0 | 338.5 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -15.51 | 192.79 | 27.93 | 242.50 | 0.5108 | -369.0 | -419.4 | |
| 0.00 | 2.70 | 0.00 | 1.54 | -15.91 | 191.54 | 26.67 | 240.80 | 0.4965 | -531.0 | -375.5 | |
| 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. | |