SDO HMI 2014-08-26 00:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.39 | 0.00 | 8.55 | -9.13 | 329.45 | 29.39 | 241.36 | 0.5544 | 44.2 | -80.9 | |
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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 | 0.90 | 0.00 | 0.58 | -8.83 | 337.11 | 37.06 | 247.28 | 0.6478 | 610.0 | 472.9 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -9.85 | 333.02 | 32.96 | 243.15 | 0.6031 | 689.0 | 597.6 | |
| 0.00 | 1.44 | 0.00 | 0.89 | -10.63 | 332.45 | 32.39 | 241.56 | 0.6010 | -718.0 | -663.8 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -9.63 | 332.16 | 32.10 | 242.84 | 0.5910 | 620.0 | 453.1 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -4.38 | 331.15 | 31.10 | 250.64 | 0.5479 | 465.0 | 384.3 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -4.40 | 330.94 | 30.88 | 250.48 | 0.5451 | 778.0 | 629.8 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -14.43 | 331.25 | 31.20 | 235.16 | 0.6134 | -531.0 | -423.0 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -4.26 | 329.67 | 29.61 | 249.90 | 0.5267 | 678.0 | 536.1 | |
| 0.00 | 0.72 | 0.00 | 0.45 | -16.55 | 330.25 | 30.19 | 231.41 | 0.6189 | -468.0 | -455.6 | |
| 0.00 | 1.44 | 0.00 | 0.81 | -7.69 | 325.24 | 25.18 | 240.03 | 0.4888 | -138.0 | -144.2 | |
| 0.00 | 1.71 | 0.00 | 0.98 | -9.98 | 325.14 | 25.08 | 235.98 | 0.5057 | -710.0 | -561.5 | |
| 0.00 | 2.15 | 0.00 | 1.21 | -8.74 | 323.73 | 23.67 | 236.55 | 0.4775 | -744.0 | -607.4 | |
| 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. | |