SDO HMI 2014-01-15 09:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.33 | 395.57 | 40.54 | 204.93 | -16.38 | 12.67 | 12.48 | 225.07 | 0.2939 | 1145.8 | 444.6 | |
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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 | 1.19 | 0.00 | 0.61 | -14.71 | 13.31 | 13.12 | 230.97 | 0.2839 | -702.0 | -610.9 | |
| 38.70 | 246.73 | 20.11 | 128.26 | -16.58 | 13.40 | 13.21 | 226.22 | 0.3047 | 1405.8 | 441.9 | |
| 4.42 | -2.00 | 2.29 | -2.00 | -16.71 | 12.75 | 12.55 | 224.49 | 0.2984 | 1156.6 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -16.08 | 12.33 | 12.14 | 225.13 | 0.2863 | 953.0 | 755.6 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -15.48 | 12.26 | 12.07 | 226.56 | 0.2788 | 611.0 | 592.1 | |
| 0.00 | 1.87 | 0.00 | 0.97 | -16.47 | 12.29 | 12.10 | 224.04 | 0.2904 | 813.0 | 646.6 | |
| 0.00 | 4.25 | 0.00 | 2.19 | -15.24 | 12.00 | 11.81 | 226.60 | 0.2729 | 1012.0 | 807.0 | |
| 0.00 | 1.79 | 0.00 | 0.92 | -16.93 | 12.00 | 11.81 | 222.26 | 0.2925 | 402.0 | 464.9 | |
| 0.00 | 1.87 | 0.00 | 0.96 | -15.40 | 11.82 | 11.63 | 225.75 | 0.2725 | 620.0 | 554.2 | |
| 35.21 | 129.87 | 18.14 | 66.90 | -15.97 | 11.63 | 11.44 | 223.77 | 0.2769 | 1356.0 | 471.0 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -18.69 | 11.80 | 11.61 | 217.85 | 0.3121 | 849.0 | 730.3 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -19.00 | 11.41 | 11.22 | 216.29 | 0.3122 | 690.0 | 503.2 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -15.87 | 7.49 | 7.30 | 211.90 | 0.2324 | -934.0 | -695.5 | |
| 0.00 | 2.21 | 0.00 | 1.13 | -17.81 | 6.16 | 5.97 | 203.37 | 0.2509 | -777.0 | -564.1 | |
| 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. | |