SDO HMI 2014-07-08 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.00 | 16.45 | 1.59 | 12.66 | 12.37 | 277.25 | 49.72 | 283.21 | 0.7674 | -156.2 | -121.1 | |
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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 | 0.82 | 0.00 | 0.68 | 7.49 | 281.03 | 53.50 | 276.65 | 0.8046 | -432.0 | -392.2 | |
| 0.00 | 0.64 | 0.00 | 0.52 | 8.49 | 280.04 | 52.51 | 277.94 | 0.7946 | -340.0 | -292.3 | |
| 2.00 | 3.00 | 1.59 | 2.39 | 11.59 | 279.03 | 51.50 | 281.94 | 0.7859 | -618.9 | -462.4 | |
| 0.00 | 1.45 | 0.00 | 1.14 | 12.59 | 278.35 | 50.82 | 283.29 | 0.7796 | -512.0 | -465.3 | |
| 0.00 | 1.18 | 0.00 | 0.93 | 12.38 | 278.24 | 50.71 | 283.03 | 0.7782 | -571.0 | -446.7 | |
| 0.00 | 3.36 | 0.00 | 2.60 | 12.31 | 277.58 | 50.06 | 283.03 | 0.7711 | -418.0 | -411.2 | |
| 0.00 | 0.82 | 0.00 | 0.64 | 15.37 | 277.56 | 50.03 | 286.97 | 0.7749 | -474.0 | -403.1 | |
| 0.00 | 1.63 | 0.00 | 1.20 | 13.03 | 274.87 | 47.34 | 284.36 | 0.7419 | 239.0 | 317.2 | |
| 0.00 | 0.82 | 0.00 | 0.59 | 14.04 | 274.02 | 46.50 | 285.87 | 0.7338 | 484.0 | 452.2 | |
| 0.00 | 0.73 | 0.00 | 0.53 | 14.50 | 274.01 | 46.49 | 286.50 | 0.7345 | 523.0 | 491.5 | |
| 0.00 | 2.00 | 0.00 | 1.44 | 13.92 | 273.72 | 46.19 | 285.77 | 0.7302 | 675.0 | 559.9 | |
| 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. | |