SDO HMI 2014-10-04 09:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.85 | 0.00 | 8.54 | -18.00 | 106.27 | -33.94 | 127.17 | 0.6657 | 262.4 | 136.2 | |
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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 | 1.06 | 0.00 | 0.68 | -22.74 | 112.99 | -27.22 | 138.55 | 0.6395 | 548.0 | 488.9 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -16.70 | 112.93 | -27.27 | 131.08 | 0.5845 | 683.0 | 576.3 | |
| 0.00 | 0.53 | 0.00 | 0.35 | -23.30 | 109.88 | -30.33 | 136.18 | 0.6722 | 503.0 | 516.7 | |
| 0.00 | 1.32 | 0.00 | 0.81 | -15.95 | 111.31 | -28.89 | 128.46 | 0.5955 | 503.0 | 352.4 | |
| 0.00 | 0.53 | 0.00 | 0.33 | -17.52 | 109.56 | -30.65 | 128.92 | 0.6271 | 255.0 | 256.5 | |
| 0.00 | 0.97 | 0.00 | 0.62 | -17.22 | 108.58 | -31.62 | 127.68 | 0.6351 | 606.0 | 491.3 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -16.95 | 108.64 | -31.57 | 127.38 | 0.6325 | 717.0 | 570.4 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -16.08 | 108.58 | -31.63 | 126.18 | 0.6265 | 561.0 | 450.0 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -16.18 | 108.52 | -31.68 | 126.26 | 0.6279 | 462.0 | 383.6 | |
| 0.00 | 1.85 | 0.00 | 1.23 | -19.35 | 106.62 | -33.58 | 128.75 | 0.6715 | 244.0 | 169.1 | |
| 0.00 | 1.06 | 0.00 | 0.77 | -17.30 | 98.96 | -41.24 | 120.95 | 0.7362 | -666.0 | -543.8 | |
| 0.00 | 0.88 | 0.00 | 0.64 | -17.39 | 98.69 | -41.52 | 120.89 | 0.7395 | -570.0 | -520.4 | |
| 0.00 | 1.58 | 0.00 | 1.17 | -17.53 | 98.18 | -42.02 | 120.77 | 0.7452 | -435.0 | -382.4 | |
| 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. | |