SDO HMI 2014-04-01 00:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.60 | 0.00 | 13.01 | -16.25 | 119.61 | 35.67 | 249.18 | 0.5944 | -222.7 | -216.0 | |
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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 | 0.88 | 0.00 | 0.76 | -7.47 | 139.29 | 55.35 | 265.47 | 0.8204 | 446.0 | 391.8 | |
| 0.00 | 1.49 | 0.00 | 1.17 | -7.69 | 135.20 | 51.27 | 265.42 | 0.7778 | 594.0 | 494.6 | |
| 0.00 | 1.40 | 0.00 | 1.06 | -10.52 | 133.50 | 49.56 | 261.75 | 0.7584 | 470.0 | 303.6 | |
| 0.00 | 0.61 | 0.00 | 0.48 | -16.33 | 134.43 | 50.49 | 254.20 | 0.7718 | 473.0 | 410.9 | |
| 0.00 | 1.14 | 0.00 | 0.88 | -18.61 | 133.81 | 49.87 | 251.17 | 0.7679 | 516.0 | 410.5 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -11.00 | 119.06 | 35.12 | 260.18 | 0.5753 | 539.0 | 473.9 | |
| 0.00 | 3.07 | 0.00 | 1.80 | -19.00 | 114.69 | 30.75 | 244.51 | 0.5377 | -509.0 | -530.7 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -18.73 | 114.49 | 30.55 | 244.88 | 0.5338 | -718.0 | -620.8 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -20.20 | 114.65 | 30.71 | 242.37 | 0.5430 | -535.0 | -421.1 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -18.86 | 114.36 | 30.43 | 244.58 | 0.5327 | -807.0 | -631.1 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -19.96 | 110.31 | 26.37 | 239.81 | 0.4850 | -791.0 | -578.0 | |
| 0.00 | 2.54 | 0.00 | 1.38 | -10.66 | 108.25 | 24.31 | 258.64 | 0.4144 | -1026.0 | -822.9 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -22.81 | 109.34 | 25.41 | 233.76 | 0.4923 | -523.0 | -389.2 | |
| 0.00 | 1.49 | 0.00 | 0.85 | -23.70 | 108.51 | 24.57 | 231.40 | 0.4893 | -745.0 | -603.5 | |
| 0.00 | 2.11 | 0.00 | 1.19 | -23.77 | 108.20 | 24.27 | 230.96 | 0.4862 | -725.0 | -558.3 | |
| 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. | |