SDO HMI 2014-07-08 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.36 | 19.88 | 0.21 | 11.91 | -23.47 | 200.62 | -20.87 | 144.36 | 0.5615 | -116.0 | 10.7 | |
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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 |
| 0.36 | 1.54 | 0.21 | 0.87 | -20.88 | 205.87 | -15.62 | 148.64 | 0.4855 | 881.2 | 726.0 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -22.82 | 204.78 | -16.71 | 149.13 | 0.5185 | -579.0 | -606.9 | |
| 0.00 | 2.00 | 0.00 | 1.16 | -22.57 | 203.50 | -17.99 | 146.99 | 0.5256 | 486.0 | 419.4 | |
| 0.00 | 2.27 | 0.00 | 1.32 | -22.41 | 203.31 | -18.18 | 146.54 | 0.5251 | 515.0 | 492.0 | |
| 0.00 | 2.63 | 0.00 | 1.52 | -21.80 | 203.36 | -18.13 | 145.90 | 0.5174 | 856.0 | 746.1 | |
| 0.00 | 1.36 | 0.00 | 0.84 | -27.11 | 200.50 | -20.99 | 147.87 | 0.6018 | -726.0 | -613.3 | |
| 0.00 | 0.91 | 0.00 | 0.56 | -27.12 | 200.28 | -21.21 | 147.61 | 0.6035 | -574.0 | -497.6 | |
| 0.00 | 1.09 | 0.00 | 0.68 | -26.94 | 200.16 | -21.33 | 147.30 | 0.6024 | -695.0 | -565.3 | |
| 0.00 | 1.91 | 0.00 | 1.20 | -28.45 | 199.81 | -21.68 | 148.38 | 0.6217 | -292.0 | -226.8 | |
| 0.00 | 1.09 | 0.00 | 0.65 | -22.73 | 199.64 | -21.85 | 142.05 | 0.5602 | 646.0 | 529.8 | |
| 0.00 | 0.27 | 0.00 | 0.17 | -21.47 | 195.80 | -25.69 | 136.07 | 0.5836 | -598.0 | -528.7 | |
| 0.00 | 2.09 | 0.00 | 1.28 | -20.92 | 195.03 | -26.46 | 134.55 | 0.5861 | -684.0 | -435.9 | |
| 0.00 | 1.09 | 0.00 | 0.69 | -23.14 | 193.08 | -28.41 | 135.40 | 0.6254 | -534.0 | -456.5 | |
| 0.00 | 0.45 | 0.00 | 0.29 | -18.36 | 190.10 | -31.39 | 126.51 | 0.6173 | -535.0 | -532.0 | |
| 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. | |