SDO HMI 2014-09-08 02:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.50 | 0.00 | 10.39 | -17.27 | 156.76 | 29.53 | 229.63 | 0.6193 | -99.8 | -31.3 | |
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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 | 1.25 | 0.00 | 0.83 | -18.76 | 160.85 | 33.61 | 231.39 | 0.6732 | 602.0 | 584.1 | |
| 0.00 | 1.52 | 0.00 | 1.00 | -18.65 | 160.25 | 33.02 | 231.03 | 0.6663 | 607.0 | 537.8 | |
| 0.00 | 2.32 | 0.00 | 1.46 | -16.34 | 157.17 | 29.93 | 231.25 | 0.6161 | 712.0 | 634.2 | |
| 0.00 | 1.78 | 0.00 | 1.14 | -18.44 | 157.36 | 30.12 | 228.75 | 0.6355 | -587.0 | -512.5 | |
| 0.00 | 1.34 | 0.00 | 0.83 | -16.30 | 156.62 | 29.38 | 230.78 | 0.6099 | 814.0 | 655.8 | |
| 0.00 | 0.80 | 0.00 | 0.50 | -16.18 | 156.27 | 29.03 | 230.62 | 0.6052 | 728.0 | 662.4 | |
| 0.00 | 0.89 | 0.00 | 0.57 | -18.68 | 156.42 | 29.18 | 227.57 | 0.6280 | -689.0 | -576.7 | |
| 0.00 | 0.62 | 0.00 | 0.40 | -19.21 | 156.37 | 29.13 | 226.87 | 0.6322 | -564.0 | -500.9 | |
| 0.00 | 0.54 | 0.00 | 0.34 | -19.06 | 156.16 | 28.92 | 226.85 | 0.6288 | -706.0 | -644.0 | |
| 0.00 | 1.61 | 0.00 | 0.98 | -16.07 | 155.00 | 27.76 | 229.52 | 0.5907 | -668.0 | -493.6 | |
| 0.00 | 1.78 | 0.00 | 1.09 | -16.41 | 154.62 | 27.39 | 228.69 | 0.5897 | -654.0 | -521.5 | |
| 0.00 | 2.05 | 0.00 | 1.25 | -16.22 | 154.24 | 27.00 | 228.54 | 0.5840 | -792.0 | -614.4 | |
| 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. | |