SDO HMI 2014-07-30 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.05 | 48.29 | 13.02 | 44.96 | -18.63 | 237.20 | -53.21 | 116.23 | 0.8477 | -150.3 | -171.6 | |
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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 | 1.18 | 0.00 | 0.97 | -18.72 | 242.71 | -47.70 | 118.61 | 0.8002 | 119.0 | 206.2 | |
| 1.45 | 3.35 | 1.25 | 2.89 | -17.99 | 240.19 | -50.22 | 116.68 | 0.8201 | 654.4 | 515.8 | |
| 2.81 | 5.34 | 2.46 | 4.68 | -18.24 | 239.58 | -50.82 | 116.71 | 0.8263 | 543.1 | 395.4 | |
| 0.45 | 1.54 | 0.40 | 1.36 | -18.47 | 239.07 | -51.33 | 116.77 | 0.8316 | 399.4 | 370.3 | |
| 0.00 | 1.00 | 0.00 | 0.88 | -17.84 | 239.18 | -51.22 | 116.10 | 0.8285 | 339.0 | 287.6 | |
| 0.00 | 1.45 | 0.00 | 1.30 | -18.01 | 238.34 | -52.07 | 115.96 | 0.8364 | -121.0 | -101.3 | |
| 0.00 | 3.99 | 0.00 | 3.73 | -18.68 | 236.92 | -53.49 | 116.17 | 0.8504 | -566.0 | -595.2 | |
| 4.17 | 21.65 | 3.97 | 20.77 | -18.90 | 236.32 | -54.08 | 116.19 | 0.8559 | -703.0 | -217.3 | |
| 1.09 | 8.79 | 1.03 | 8.38 | -18.50 | 236.29 | -54.12 | 115.74 | 0.8550 | -745.9 | -469.0 | |
| 1.63 | -8.00 | 1.57 | -8.00 | -19.13 | 235.88 | -54.53 | 116.29 | 0.8602 | -213.1 | 999999 | |
| 2.45 | -9.00 | 2.34 | -9.00 | -18.36 | 236.03 | -54.38 | 115.49 | 0.8568 | -555.0 | 999999 | |
| 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. | |