SDO HMI 2014-10-09 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.68 | 0.00 | 8.48 | -17.03 | 106.93 | 28.31 | 229.38 | 0.6003 | 314.5 | 304.2 | |
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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 | 0.70 | 0.00 | 0.44 | -13.75 | 110.81 | 32.19 | 237.75 | 0.6142 | 496.0 | 454.6 | |
| 0.00 | 0.96 | 0.00 | 0.61 | -15.69 | 110.69 | 32.07 | 234.97 | 0.6266 | 459.0 | 408.6 | |
| 0.00 | 1.40 | 0.00 | 0.87 | -13.49 | 110.26 | 31.65 | 237.68 | 0.6060 | 658.0 | 671.2 | |
| 0.00 | 1.32 | 0.00 | 0.81 | -13.41 | 109.96 | 31.34 | 237.55 | 0.6019 | 710.0 | 642.4 | |
| 0.00 | 1.23 | 0.00 | 0.78 | -15.89 | 110.21 | 31.60 | 234.30 | 0.6227 | 665.0 | 580.7 | |
| 0.00 | 1.49 | 0.00 | 0.92 | -13.24 | 109.76 | 31.14 | 237.63 | 0.5983 | 767.0 | 610.1 | |
| 0.00 | 0.88 | 0.00 | 0.59 | -22.79 | 110.02 | 31.40 | 225.54 | 0.6753 | 550.0 | 380.1 | |
| 0.00 | 0.88 | 0.00 | 0.58 | -22.82 | 108.29 | 29.67 | 223.94 | 0.6598 | 397.0 | 367.2 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -15.60 | 105.87 | 27.25 | 230.67 | 0.5724 | 596.0 | 437.2 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -23.41 | 107.27 | 28.65 | 222.31 | 0.6559 | 649.0 | 507.2 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -16.55 | 100.88 | 22.26 | 223.65 | 0.5281 | -632.0 | -514.9 | |
| 0.00 | 0.96 | 0.00 | 0.57 | -19.24 | 100.07 | 21.45 | 219.16 | 0.5489 | -589.0 | -510.5 | |
| 0.00 | 1.40 | 0.00 | 0.80 | -19.44 | 94.23 | 15.61 | 210.51 | 0.5018 | -638.0 | -493.7 | |
| 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. | |