SDO HMI 2014-08-05 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.89 | 0.00 | 13.48 | -19.00 | 237.68 | 26.63 | 225.56 | 0.5950 | -178.5 | -192.6 | |
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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 | 1.72 | 0.00 | 1.09 | -16.13 | 243.21 | 32.16 | 234.67 | 0.6289 | 650.0 | 549.2 | |
| 0.00 | 0.63 | 0.00 | 0.41 | -17.94 | 242.58 | 31.53 | 231.76 | 0.6356 | 605.0 | 488.1 | |
| 0.00 | 1.54 | 0.00 | 0.97 | -17.39 | 241.69 | 30.64 | 231.70 | 0.6219 | 708.0 | 578.4 | |
| 0.00 | 1.81 | 0.00 | 1.15 | -19.70 | 240.62 | 29.56 | 227.76 | 0.6296 | 616.0 | 400.9 | |
| 0.00 | 1.27 | 0.00 | 0.80 | -19.88 | 240.21 | 29.15 | 227.15 | 0.6271 | 699.0 | 505.6 | |
| 0.00 | 1.90 | 0.00 | 1.17 | -19.17 | 237.73 | 26.68 | 225.56 | 0.5961 | -763.0 | -591.7 | |
| 0.00 | 0.72 | 0.00 | 0.45 | -19.53 | 237.54 | 26.49 | 224.91 | 0.5976 | -70.0 | -148.6 | |
| 0.00 | 2.26 | 0.00 | 1.40 | -20.05 | 237.17 | 26.11 | 223.86 | 0.5988 | -827.0 | -630.5 | |
| 0.00 | 0.54 | 0.00 | 0.33 | -18.36 | 236.81 | 25.75 | 225.62 | 0.5792 | -660.0 | -612.8 | |
| 0.00 | 1.54 | 0.00 | 0.95 | -20.07 | 236.92 | 25.86 | 223.57 | 0.5966 | -540.0 | -452.1 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -19.73 | 234.79 | 23.74 | 221.59 | 0.5729 | -536.0 | -443.6 | |
| 0.00 | 1.63 | 0.00 | 0.97 | -19.01 | 234.47 | 23.41 | 222.10 | 0.5625 | -649.0 | -462.8 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -21.30 | 234.84 | 23.78 | 219.77 | 0.5894 | -453.0 | -436.4 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -18.57 | 234.37 | 23.31 | 222.54 | 0.5570 | -707.0 | -621.6 | |
| 0.00 | 3.26 | 0.00 | 1.94 | -18.63 | 234.13 | 23.08 | 222.18 | 0.5553 | -750.0 | -613.6 | |
| 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. | |