SDO HMI 2014-07-03 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.08 | 0.00 | 10.76 | -13.08 | 254.51 | -39.19 | 113.45 | 0.6721 | 360.6 | 281.7 | |
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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 | 1.00 | 0.00 | 0.64 | -12.59 | 257.71 | -36.00 | 114.39 | 0.6320 | 819.0 | 729.4 | |
| 0.00 | 1.09 | 0.00 | 0.70 | -12.85 | 257.67 | -36.04 | 114.74 | 0.6338 | 724.0 | 612.4 | |
| 0.00 | 1.91 | 0.00 | 1.22 | -12.47 | 257.50 | -36.21 | 114.09 | 0.6341 | 715.0 | 505.0 | |
| 0.00 | 1.18 | 0.00 | 0.75 | -12.28 | 257.45 | -36.25 | 113.79 | 0.6337 | 625.0 | 551.5 | |
| 0.00 | 1.00 | 0.00 | 0.65 | -12.50 | 255.81 | -37.90 | 113.23 | 0.6549 | 355.0 | 312.3 | |
| 0.00 | 1.36 | 0.00 | 0.90 | -13.23 | 255.59 | -38.11 | 114.17 | 0.6608 | 618.0 | 541.4 | |
| 0.00 | 1.27 | 0.00 | 0.84 | -13.01 | 255.43 | -38.27 | 113.78 | 0.6617 | 671.0 | 577.9 | |
| 0.00 | 0.73 | 0.00 | 0.48 | -12.49 | 255.17 | -38.53 | 112.89 | 0.6625 | 555.0 | 512.8 | |
| 0.00 | 1.09 | 0.00 | 0.72 | -11.91 | 255.27 | -38.43 | 112.12 | 0.6588 | 576.0 | 471.4 | |
| 0.00 | 1.09 | 0.00 | 0.72 | -11.57 | 254.33 | -39.38 | 111.18 | 0.6689 | 653.0 | 532.0 | |
| 0.00 | 0.82 | 0.00 | 0.56 | -13.77 | 252.79 | -40.91 | 113.54 | 0.6961 | 606.0 | 488.2 | |
| 0.00 | 1.09 | 0.00 | 0.79 | -14.20 | 249.88 | -43.82 | 112.81 | 0.7306 | -606.0 | -581.7 | |
| 0.00 | 1.63 | 0.00 | 1.19 | -14.88 | 249.62 | -44.08 | 113.59 | 0.7360 | -564.0 | -416.8 | |
| 0.00 | 0.82 | 0.00 | 0.60 | -14.66 | 249.50 | -44.20 | 113.25 | 0.7364 | -698.0 | -595.0 | |
| 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. | |