SDO HMI 2014-07-29 13:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.86 | 0.00 | 9.39 | 12.27 | 260.51 | -42.57 | 77.44 | 0.6771 | 85.6 | 144.9 | |
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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 | 1.18 | 0.00 | 0.71 | 16.32 | 269.47 | -33.61 | 69.17 | 0.5706 | -489.0 | -452.7 | |
| 0.00 | 1.36 | 0.00 | 0.82 | 16.16 | 269.31 | -33.77 | 69.51 | 0.5721 | -696.0 | -541.8 | |
| 0.00 | 0.91 | 0.00 | 0.55 | 15.80 | 269.00 | -34.09 | 70.25 | 0.5751 | -649.0 | -515.6 | |
| 0.00 | 0.72 | 0.00 | 0.44 | 14.55 | 268.12 | -34.96 | 72.68 | 0.5832 | -545.0 | -433.5 | |
| 0.00 | 1.00 | 0.00 | 0.62 | 12.98 | 266.10 | -36.98 | 75.83 | 0.6067 | -664.0 | -536.9 | |
| 0.00 | 0.91 | 0.00 | 0.63 | 10.25 | 258.68 | -44.40 | 81.02 | 0.6993 | 647.0 | 467.0 | |
| 0.00 | 0.72 | 0.00 | 0.50 | 10.49 | 258.64 | -44.44 | 80.67 | 0.7000 | 621.0 | 540.2 | |
| 0.00 | 2.45 | 0.00 | 1.74 | 9.80 | 257.04 | -46.04 | 81.74 | 0.7190 | 723.0 | 504.9 | |
| 0.00 | 1.72 | 0.00 | 1.23 | 9.42 | 256.89 | -46.20 | 82.27 | 0.7208 | 621.0 | 464.6 | |
| 0.00 | 1.81 | 0.00 | 1.29 | 9.63 | 256.72 | -46.37 | 81.99 | 0.7229 | 611.0 | 468.9 | |
| 0.00 | 0.45 | 0.00 | 0.33 | 12.97 | 255.13 | -47.96 | 77.54 | 0.7434 | 508.0 | 437.0 | |
| 0.00 | 0.63 | 0.00 | 0.53 | 19.17 | 249.56 | -53.52 | 70.27 | 0.8090 | 339.0 | 318.0 | |
| 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. | |