SDO HMI 2014-05-20 08:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.31 | 213.39 | 22.01 | 144.74 | -24.77 | 190.13 | 37.95 | 234.84 | 0.6853 | 540.9 | 261.4 | |
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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 |
| 30.96 | 197.82 | 21.09 | 134.70 | -24.62 | 190.54 | 38.36 | 235.31 | 0.6885 | 1133.9 | 332.6 | |
| 1.35 | -1.00 | 0.92 | -1.00 | -24.99 | 190.21 | 38.03 | 234.63 | 0.6871 | 836.3 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.98 | -24.67 | 185.77 | 33.58 | 232.20 | 0.6384 | -230.0 | -161.1 | |
| 0.00 | 0.72 | 0.00 | 0.47 | -26.06 | 185.88 | 33.70 | 230.41 | 0.6490 | -632.0 | -538.8 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -26.20 | 185.80 | 33.62 | 230.18 | 0.6491 | -504.0 | -473.3 | |
| 0.00 | 3.96 | 0.00 | 2.56 | -25.74 | 185.61 | 33.43 | 230.66 | 0.6440 | -793.0 | -633.7 | |
| 0.00 | 0.99 | 0.00 | 0.64 | -26.03 | 185.67 | 33.49 | 230.30 | 0.6466 | -730.0 | -645.3 | |
| 0.00 | 1.17 | 0.00 | 0.76 | -26.77 | 185.50 | 33.32 | 229.21 | 0.6501 | -672.0 | -549.2 | |
| 0.00 | 1.17 | 0.00 | 0.76 | -27.34 | 185.49 | 33.31 | 228.45 | 0.6540 | -594.0 | -456.8 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -28.48 | 184.65 | 32.47 | 226.38 | 0.6541 | -426.0 | -379.0 | |
| 0.00 | 0.81 | 0.00 | 0.52 | -26.76 | 184.01 | 31.82 | 228.08 | 0.6350 | -779.0 | -576.7 | |
| 0.00 | 1.89 | 0.00 | 1.23 | -28.48 | 184.20 | 32.02 | 226.02 | 0.6499 | -817.0 | -686.9 | |
| 0.00 | 1.53 | 0.00 | 0.95 | -27.32 | 180.62 | 28.44 | 224.50 | 0.6058 | -652.0 | -567.8 | |
| 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. | |