SDO HMI 2014-10-07 06:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.39 | 0.00 | 12.67 | -13.62 | 59.31 | -42.95 | 115.34 | 0.7343 | 267.5 | 263.4 | |
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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 |
| 0.00 | 0.88 | 0.00 | 0.61 | -12.66 | 61.95 | -40.31 | 115.47 | 0.7015 | 377.0 | 374.5 | |
| 0.00 | 3.51 | 0.00 | 2.45 | -12.84 | 61.71 | -40.55 | 115.58 | 0.7050 | 919.0 | 689.9 | |
| 0.00 | 2.72 | 0.00 | 1.92 | -12.83 | 61.02 | -41.24 | 115.19 | 0.7127 | 634.0 | 522.7 | |
| 0.00 | 1.76 | 0.00 | 1.24 | -13.02 | 60.94 | -41.32 | 115.40 | 0.7145 | 676.0 | 609.4 | |
| 0.00 | 1.49 | 0.00 | 1.09 | -15.42 | 59.93 | -42.33 | 117.90 | 0.7369 | 542.0 | 494.1 | |
| 0.00 | 0.53 | 0.00 | 0.39 | -13.46 | 58.19 | -44.07 | 114.56 | 0.7460 | -458.0 | -475.8 | |
| 0.00 | 2.72 | 0.00 | 2.04 | -13.32 | 57.58 | -44.68 | 114.09 | 0.7519 | -762.0 | -664.0 | |
| 0.00 | 0.97 | 0.00 | 0.72 | -12.25 | 57.08 | -45.18 | 112.54 | 0.7528 | -718.0 | -626.7 | |
| 0.00 | 0.61 | 0.00 | 0.48 | -15.82 | 55.84 | -46.42 | 116.32 | 0.7799 | 570.0 | 505.1 | |
| 0.00 | 0.88 | 0.00 | 0.69 | -15.53 | 55.88 | -46.38 | 115.99 | 0.7783 | 590.0 | 494.1 | |
| 0.00 | 1.32 | 0.00 | 1.04 | -15.61 | 55.58 | -46.68 | 115.96 | 0.7816 | 573.0 | 512.3 | |
| 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. | |