SDO HMI 2014-08-26 04:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.12 | 0.00 | 9.40 | -10.15 | 330.60 | 32.74 | 241.86 | 0.6047 | -97.2 | -50.4 | |
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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 | 0.99 | 0.00 | 0.70 | -7.77 | 341.44 | 43.58 | 251.96 | 0.7207 | 415.0 | 333.6 | |
| 0.00 | 1.89 | 0.00 | 1.29 | -7.45 | 339.28 | 41.42 | 251.44 | 0.6943 | 283.0 | 296.9 | |
| 0.00 | 1.17 | 0.00 | 0.77 | -12.03 | 334.70 | 36.84 | 242.66 | 0.6625 | -269.0 | -329.1 | |
| 0.00 | 0.90 | 0.00 | 0.57 | -10.75 | 332.42 | 34.56 | 242.94 | 0.6280 | -619.0 | -523.6 | |
| 0.00 | 1.17 | 0.00 | 0.71 | -4.43 | 331.08 | 33.22 | 251.83 | 0.5771 | 767.0 | 625.9 | |
| 0.00 | 0.54 | 0.00 | 0.33 | -7.61 | 331.30 | 33.44 | 246.87 | 0.5961 | 568.0 | 534.8 | |
| 0.00 | 0.81 | 0.00 | 0.50 | -9.66 | 331.39 | 33.53 | 243.82 | 0.6090 | 606.0 | 544.2 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -9.77 | 331.11 | 33.25 | 243.46 | 0.6062 | 700.0 | 620.6 | |
| 0.00 | 0.27 | 0.00 | 0.17 | -14.07 | 331.41 | 33.55 | 237.56 | 0.6375 | -609.0 | -593.0 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -10.15 | 325.85 | 27.99 | 238.61 | 0.5432 | -553.0 | -408.5 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -13.03 | 325.00 | 27.14 | 233.36 | 0.5560 | -630.0 | -461.2 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -10.76 | 324.45 | 26.58 | 236.28 | 0.5307 | -559.0 | -392.5 | |
| 0.00 | 1.44 | 0.00 | 0.87 | -17.77 | 323.32 | 25.46 | 225.04 | 0.5807 | -721.0 | -549.9 | |
| 0.00 | 1.35 | 0.00 | 0.76 | -8.93 | 321.68 | 23.82 | 236.37 | 0.4810 | -740.0 | -526.1 | |
| 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. | |