SDO HMI 2014-03-30 02:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 11.91 | 0.00 | 6.61 | -25.55 | 91.15 | -18.07 | 141.97 | 0.4349 | 470.4 | 430.8 | |
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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 | 0.61 | 0.00 | 0.32 | -25.27 | 101.89 | -7.33 | 160.17 | 0.3415 | 482.0 | 527.0 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -23.19 | 101.72 | -7.50 | 157.20 | 0.3110 | 692.0 | 571.1 | |
| 0.00 | 1.84 | 0.00 | 0.95 | -21.30 | 100.10 | -9.12 | 149.83 | 0.2951 | 896.0 | 705.3 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -20.61 | 98.07 | -11.15 | 143.31 | 0.3044 | 667.0 | 466.6 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -25.69 | 92.93 | -16.29 | 142.57 | 0.4176 | 710.0 | 479.6 | |
| 0.00 | 1.31 | 0.00 | 0.73 | -27.02 | 90.83 | -18.39 | 141.49 | 0.4533 | 837.0 | 736.6 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -27.02 | 89.94 | -19.28 | 140.26 | 0.4619 | 829.0 | 739.8 | |
| 0.00 | 1.31 | 0.00 | 0.74 | -27.01 | 89.51 | -19.70 | 139.66 | 0.4660 | 748.0 | 593.0 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -25.98 | 87.02 | -22.19 | 134.91 | 0.4815 | 666.0 | 589.6 | |
| 0.00 | 1.05 | 0.00 | 0.66 | -30.03 | 77.93 | -31.28 | 132.45 | 0.6115 | -793.0 | -607.2 | |
| 0.00 | 0.61 | 0.00 | 0.39 | -27.30 | 74.42 | -34.80 | 126.18 | 0.6305 | -560.0 | -503.9 | |
| 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. | |