SDO HMI 2014-07-10 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.45 | 38.60 | 3.44 | 30.36 | 7.81 | 252.11 | 51.06 | 276.98 | 0.7782 | 178.1 | 184.6 | |
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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 | 1.63 | 0.00 | 1.41 | 6.89 | 256.05 | 55.00 | 275.74 | 0.8195 | -482.0 | -359.0 | |
| 0.00 | 0.91 | 0.00 | 0.78 | 6.96 | 255.80 | 54.74 | 275.83 | 0.8169 | -392.0 | -300.8 | |
| 0.00 | 0.91 | 0.00 | 0.77 | 6.87 | 255.25 | 54.19 | 275.72 | 0.8114 | -506.0 | -437.0 | |
| 0.00 | 1.73 | 0.00 | 1.45 | 7.09 | 255.08 | 54.02 | 276.00 | 0.8096 | -667.0 | -619.6 | |
| 0.00 | 2.91 | 0.00 | 2.43 | 8.12 | 254.80 | 53.74 | 277.28 | 0.8069 | -616.0 | -523.7 | |
| 0.00 | 1.00 | 0.00 | 0.78 | 8.28 | 251.74 | 50.69 | 277.59 | 0.7746 | -207.0 | -210.4 | |
| 0.00 | 3.72 | 0.00 | 2.89 | 8.94 | 251.57 | 50.52 | 278.44 | 0.7730 | 596.0 | 471.3 | |
| 2.09 | 6.99 | 1.61 | 5.40 | 7.26 | 251.23 | 50.18 | 276.28 | 0.7687 | 673.1 | 469.8 | |
| 2.36 | 13.08 | 1.83 | 10.11 | 8.39 | 251.37 | 50.32 | 277.75 | 0.7706 | 547.0 | 384.8 | |
| 0.00 | 1.09 | 0.00 | 0.84 | 8.86 | 251.22 | 50.16 | 278.37 | 0.7691 | 513.0 | 505.0 | |
| 0.00 | 0.91 | 0.00 | 0.70 | 8.51 | 250.96 | 49.90 | 277.92 | 0.7661 | 564.0 | 526.2 | |
| 0.00 | 1.18 | 0.00 | 0.90 | 8.24 | 250.77 | 49.71 | 277.57 | 0.7638 | 422.0 | 384.2 | |
| 0.00 | 0.54 | 0.00 | 0.41 | 6.14 | 250.41 | 49.35 | 274.82 | 0.7593 | 594.0 | 514.8 | |
| 0.00 | 0.91 | 0.00 | 0.69 | 5.87 | 250.37 | 49.31 | 274.46 | 0.7589 | 557.0 | 511.2 | |
| 0.00 | 1.09 | 0.00 | 0.80 | 3.89 | 248.46 | 47.41 | 271.77 | 0.7371 | 467.0 | 423.2 | |
| 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. | |