SDO HMI 2014-07-08 06:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.63 | 17.61 | 0.95 | 10.63 | -21.40 | 200.73 | -24.05 | 138.43 | 0.5694 | -235.1 | -39.0 | |
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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 |
| 1.18 | 5.63 | 0.68 | 3.26 | -21.13 | 205.56 | -19.22 | 143.54 | 0.5187 | 896.4 | 682.7 | |
| 0.00 | 1.54 | 0.00 | 0.91 | -22.90 | 204.89 | -19.89 | 144.73 | 0.5450 | -864.0 | -678.3 | |
| 0.45 | 1.36 | 0.27 | 0.80 | -22.90 | 204.71 | -20.07 | 144.50 | 0.5466 | -749.6 | -654.9 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -21.57 | 203.69 | -21.10 | 141.58 | 0.5407 | 785.0 | 671.5 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -22.05 | 203.58 | -21.21 | 142.02 | 0.5469 | 477.0 | 498.0 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -21.81 | 203.58 | -21.20 | 141.73 | 0.5443 | 724.0 | 599.0 | |
| 0.00 | 0.82 | 0.00 | 0.51 | -20.79 | 195.58 | -29.20 | 131.67 | 0.6128 | -655.0 | -538.6 | |
| 0.00 | 2.18 | 0.00 | 1.38 | -21.01 | 194.85 | -29.93 | 131.30 | 0.6222 | -636.0 | -558.9 | |
| 0.00 | 1.27 | 0.00 | 0.81 | -20.89 | 193.47 | -31.31 | 129.94 | 0.6354 | -631.0 | -559.3 | |
| 0.00 | 1.18 | 0.00 | 0.77 | -21.78 | 192.99 | -31.79 | 130.67 | 0.6473 | -721.0 | -605.9 | |
| 0.00 | 0.73 | 0.00 | 0.48 | -18.82 | 190.05 | -34.73 | 124.55 | 0.6570 | -711.0 | -563.2 | |
| 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. | |