SDO HMI 2014-07-07 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.15 | 159.33 | 20.68 | 97.12 | 6.65 | 203.48 | -35.64 | 83.49 | 0.5845 | -637.7 | -336.9 | |
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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 |
| 2.45 | 12.26 | 1.47 | 7.36 | 6.99 | 204.90 | -34.21 | 82.74 | 0.5648 | -1088.6 | -664.2 | |
| 4.36 | -1.00 | 2.62 | -1.00 | 7.14 | 204.81 | -34.30 | 82.49 | 0.5662 | -975.6 | 999999 | |
| 26.16 | 126.64 | 15.86 | 76.75 | 6.50 | 203.89 | -35.22 | 83.71 | 0.5787 | -1230.5 | -414.8 | |
| 0.00 | 1.27 | 0.00 | 0.78 | 8.56 | 203.28 | -35.83 | 80.26 | 0.5895 | -586.0 | -429.9 | |
| 1.18 | 6.36 | 0.73 | 3.90 | 7.48 | 202.90 | -36.22 | 82.16 | 0.5936 | -632.3 | -528.2 | |
| 0.00 | 0.73 | 0.00 | 0.45 | 8.09 | 202.80 | -36.32 | 81.14 | 0.5956 | -621.0 | -522.9 | |
| 0.00 | 1.27 | 0.00 | 0.79 | 7.51 | 202.01 | -37.10 | 82.21 | 0.6059 | 747.0 | 589.6 | |
| 0.00 | 1.18 | 0.00 | 0.76 | 5.59 | 199.71 | -39.40 | 85.48 | 0.6360 | 650.0 | 585.0 | |
| 0.00 | 2.54 | 0.00 | 1.64 | 6.74 | 199.45 | -39.66 | 83.69 | 0.6400 | 581.0 | 482.1 | |
| 0.00 | 1.36 | 0.00 | 0.88 | 6.35 | 198.85 | -40.27 | 84.33 | 0.6478 | 581.0 | 462.0 | |
| 0.00 | 1.45 | 0.00 | 0.96 | 8.01 | 197.40 | -41.71 | 81.92 | 0.6678 | 673.0 | 581.8 | |
| 0.00 | 0.64 | 0.00 | 0.42 | 9.38 | 197.13 | -41.98 | 79.90 | 0.6726 | 456.0 | 523.4 | |
| 0.00 | 1.09 | 0.00 | 0.73 | 8.21 | 197.00 | -42.11 | 81.66 | 0.6731 | 527.0 | 482.8 | |
| 0.00 | 1.45 | 0.00 | 0.97 | 6.48 | 196.87 | -42.25 | 84.23 | 0.6737 | 383.0 | 386.4 | |
| 0.00 | 1.09 | 0.00 | 0.73 | 6.67 | 196.81 | -42.31 | 83.96 | 0.6746 | 541.0 | 418.8 | |
| 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. | |