SDO HMI 2014-03-25 06:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.17 | 46.52 | 8.80 | 28.71 | 3.01 | 137.61 | -35.36 | 75.41 | 0.5992 | 94.1 | -67.8 | |
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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 |
| 2.45 | 6.99 | 1.47 | 4.20 | 3.71 | 140.21 | -32.76 | 73.04 | 0.5666 | -926.9 | -794.8 | |
| 1.05 | 6.29 | 0.63 | 3.77 | 3.17 | 140.06 | -32.91 | 74.03 | 0.5665 | -889.2 | -748.8 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 3.14 | 139.66 | -33.31 | 74.29 | 0.5718 | -551.0 | -425.0 | |
| 0.00 | 1.75 | 0.00 | 1.05 | 2.84 | 139.64 | -33.33 | 74.81 | 0.5709 | -773.0 | -641.2 | |
| 0.00 | 0.79 | 0.00 | 0.47 | 2.94 | 139.49 | -33.48 | 74.72 | 0.5733 | -645.0 | -552.1 | |
| 2.54 | 4.55 | 1.54 | 2.76 | 3.74 | 139.28 | -33.69 | 73.48 | 0.5795 | -793.5 | -460.3 | |
| 0.00 | 1.05 | 0.00 | 0.65 | 5.33 | 138.32 | -34.65 | 71.42 | 0.5994 | -708.0 | -548.9 | |
| 0.44 | 1.66 | 0.27 | 1.02 | 3.62 | 138.01 | -34.96 | 74.32 | 0.5962 | 728.2 | 647.8 | |
| 0.00 | 0.70 | 0.00 | 0.43 | 3.51 | 137.83 | -35.14 | 74.58 | 0.5981 | 654.0 | 519.8 | |
| 0.00 | 1.40 | 0.00 | 0.87 | 5.25 | 137.70 | -35.27 | 71.88 | 0.6072 | -660.0 | -542.1 | |
| 0.00 | 1.05 | 0.00 | 0.66 | 1.60 | 135.77 | -37.19 | 78.50 | 0.6189 | 754.0 | 675.3 | |
| 0.00 | 2.89 | 0.00 | 1.82 | 2.55 | 135.64 | -37.33 | 77.06 | 0.6239 | 713.0 | 722.8 | |
| 0.00 | 1.05 | 0.00 | 0.66 | 2.35 | 135.49 | -37.48 | 77.43 | 0.6251 | 913.0 | 743.8 | |
| 7.69 | 13.11 | 4.89 | 8.33 | 2.19 | 135.16 | -37.81 | 77.81 | 0.6291 | 794.5 | 656.8 | |
| 0.00 | 2.19 | 0.00 | 1.39 | 2.47 | 135.03 | -37.94 | 77.42 | 0.6316 | 502.0 | 384.6 | |
| 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. | |