SDO HMI 2014-05-28 23:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.57 | 73.36 | 18.03 | 39.38 | -19.79 | 50.53 | 12.47 | 212.00 | 0.3862 | 174.5 | 209.5 | |
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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 | 2.08 | 0.00 | 1.12 | -18.65 | 53.20 | 15.14 | 219.26 | 0.3926 | 923.0 | 762.1 | |
| 21.39 | 36.91 | 11.54 | 19.90 | -19.20 | 53.08 | 15.02 | 218.14 | 0.3980 | 1004.7 | 777.0 | |
| 0.00 | 2.80 | 0.00 | 1.51 | -19.42 | 52.27 | 14.21 | 216.28 | 0.3929 | 786.0 | 693.5 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -18.37 | 51.72 | 13.66 | 216.95 | 0.3744 | 831.0 | 677.4 | |
| 0.00 | 1.62 | 0.00 | 0.88 | -20.62 | 50.91 | 12.85 | 211.85 | 0.3961 | 730.0 | 622.9 | |
| 3.25 | 16.69 | 1.73 | 8.89 | -19.56 | 49.01 | 10.95 | 209.42 | 0.3660 | -1033.5 | -767.1 | |
| 8.93 | -6.00 | 4.76 | -6.00 | -19.82 | 48.83 | 10.77 | 208.66 | 0.3682 | -1026.0 | 999999 | |
| 0.00 | 2.08 | 0.00 | 1.13 | -23.35 | 48.56 | 10.50 | 203.79 | 0.4165 | 788.0 | 583.7 | |
| 0.00 | 2.53 | 0.00 | 1.34 | -20.14 | 45.67 | 7.61 | 200.83 | 0.3513 | -850.0 | -719.5 | |
| 0.00 | 1.71 | 0.00 | 0.91 | -21.92 | 42.60 | 4.54 | 191.66 | 0.3651 | -841.0 | -688.6 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -21.95 | 42.40 | 4.35 | 191.15 | 0.3650 | -774.0 | -653.6 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -22.05 | 42.21 | 4.15 | 190.61 | 0.3660 | -764.0 | -576.1 | |
| 0.00 | 3.79 | 0.00 | 2.02 | -22.31 | 41.79 | 3.73 | 189.43 | 0.3689 | -860.0 | -693.5 | |
| 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. | |