SDO HMI 2014-05-29 06:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.11 | 55.23 | 13.24 | 30.28 | -19.74 | 51.10 | 16.90 | 219.95 | 0.4286 | 355.0 | 269.6 | |
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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 | 0.81 | 0.00 | 0.45 | -18.62 | 53.84 | 19.64 | 226.38 | 0.4417 | 730.0 | 649.7 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -18.65 | 53.71 | 19.51 | 226.14 | 0.4406 | 805.0 | 566.6 | |
| 18.06 | 27.72 | 9.97 | 15.31 | -19.23 | 53.47 | 19.27 | 224.82 | 0.4439 | 1014.8 | 780.1 | |
| 0.00 | 2.44 | 0.00 | 1.34 | -18.97 | 53.10 | 18.90 | 224.72 | 0.4371 | 414.0 | 571.7 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -19.39 | 52.57 | 18.37 | 223.23 | 0.4358 | 732.0 | 676.7 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -18.92 | 51.84 | 17.64 | 222.93 | 0.4226 | 858.0 | 688.0 | |
| 0.00 | 3.79 | 0.00 | 2.08 | -20.69 | 50.92 | 16.72 | 218.58 | 0.4333 | 709.0 | 683.7 | |
| 0.00 | 1.44 | 0.00 | 0.79 | -20.43 | 50.59 | 16.38 | 218.44 | 0.4270 | 800.0 | 676.7 | |
| 0.63 | 2.80 | 0.34 | 1.51 | -19.57 | 48.89 | 14.69 | 216.85 | 0.4000 | -1092.7 | -912.9 | |
| 5.42 | 7.58 | 2.93 | 4.10 | -19.82 | 48.65 | 14.44 | 216.00 | 0.4009 | -1023.6 | -827.8 | |
| 0.00 | 3.07 | 0.00 | 1.64 | -21.90 | 42.37 | 8.16 | 200.26 | 0.3819 | -773.0 | -714.4 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -21.97 | 40.35 | 6.15 | 195.52 | 0.3729 | -772.0 | -494.6 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -26.34 | 35.60 | 1.40 | 182.92 | 0.4301 | -553.0 | -478.5 | |
| 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. | |