SDO HMI 2014-03-30 11:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.35 | 22.96 | 0.20 | 12.92 | 17.80 | 89.97 | -14.32 | 29.79 | 0.4753 | -456.4 | -451.4 | |
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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 | 0.50 | 20.53 | 91.66 | -12.63 | 24.30 | 0.4998 | 624.0 | 435.6 | |
| 0.00 | 3.77 | 0.00 | 2.11 | 17.88 | 91.18 | -13.11 | 27.66 | 0.4669 | -699.0 | -668.8 | |
| 0.00 | 2.89 | 0.00 | 1.62 | 17.68 | 91.07 | -13.22 | 28.07 | 0.4651 | -952.0 | -799.4 | |
| 0.35 | 1.49 | 0.20 | 0.83 | 17.42 | 91.02 | -13.27 | 28.43 | 0.4619 | -1011.8 | -899.5 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 17.53 | 90.82 | -13.47 | 28.68 | 0.4648 | -841.0 | -694.9 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 17.83 | 90.57 | -13.72 | 28.79 | 0.4707 | -564.0 | -442.3 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 17.51 | 90.37 | -13.92 | 29.50 | 0.4679 | -765.0 | -623.2 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 17.84 | 90.28 | -14.01 | 29.29 | 0.4730 | -523.0 | -393.2 | |
| 0.00 | 1.84 | 0.00 | 1.03 | 17.46 | 89.95 | -14.34 | 30.28 | 0.4704 | -826.0 | -694.2 | |
| 0.00 | 2.10 | 0.00 | 1.18 | 17.23 | 89.81 | -14.48 | 30.79 | 0.4686 | -729.0 | -584.8 | |
| 0.00 | 3.86 | 0.00 | 2.17 | 17.76 | 89.73 | -14.56 | 30.32 | 0.4761 | -751.0 | -430.6 | |
| 0.00 | 1.40 | 0.00 | 0.81 | 18.04 | 85.53 | -18.76 | 36.62 | 0.5147 | 523.0 | 506.9 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 18.08 | 85.39 | -18.90 | 36.77 | 0.5164 | 692.0 | 563.7 | |
| 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. | |