SDO HMI 2014-09-08 06:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.99 | 0.00 | 13.27 | -17.78 | 158.82 | 33.78 | 232.65 | 0.6670 | 188.8 | 208.7 | |
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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 |
| 0.00 | 0.98 | 0.00 | 0.69 | -19.12 | 162.70 | 37.66 | 234.00 | 0.7158 | 627.0 | 468.9 | |
| 0.00 | 1.25 | 0.00 | 0.85 | -17.13 | 161.45 | 36.40 | 235.54 | 0.6902 | 703.0 | 590.9 | |
| 0.00 | 0.98 | 0.00 | 0.68 | -19.20 | 161.24 | 36.19 | 232.85 | 0.7020 | 554.0 | 359.7 | |
| 0.00 | 1.16 | 0.00 | 0.80 | -18.74 | 160.84 | 35.80 | 233.12 | 0.6949 | 621.0 | 571.3 | |
| 0.00 | 1.61 | 0.00 | 1.10 | -18.46 | 160.74 | 35.69 | 233.37 | 0.6919 | 720.0 | 575.9 | |
| 0.00 | 1.25 | 0.00 | 0.84 | -17.40 | 160.30 | 35.25 | 234.35 | 0.6801 | 635.0 | 571.2 | |
| 0.00 | 0.98 | 0.00 | 0.67 | -18.41 | 160.49 | 35.45 | 233.25 | 0.6890 | 669.0 | 593.6 | |
| 0.00 | 2.59 | 0.00 | 1.76 | -18.55 | 160.21 | 35.17 | 232.86 | 0.6872 | 537.0 | 488.2 | |
| 0.00 | 1.07 | 0.00 | 0.72 | -18.21 | 160.09 | 35.05 | 233.19 | 0.6836 | 521.0 | 414.1 | |
| 0.00 | 0.98 | 0.00 | 0.64 | -18.50 | 157.28 | 32.24 | 230.56 | 0.6572 | -525.0 | -474.2 | |
| 0.00 | 1.87 | 0.00 | 1.20 | -16.39 | 156.87 | 31.82 | 232.89 | 0.6366 | 694.0 | 614.5 | |
| 0.00 | 0.98 | 0.00 | 0.64 | -19.01 | 156.52 | 31.48 | 229.28 | 0.6537 | -733.0 | -612.3 | |
| 0.00 | 1.70 | 0.00 | 1.06 | -15.89 | 154.94 | 29.90 | 231.83 | 0.6121 | -791.0 | -620.9 | |
| 0.00 | 1.52 | 0.00 | 0.95 | -16.43 | 154.67 | 29.63 | 230.86 | 0.6135 | -656.0 | -434.2 | |
| 0.00 | 1.07 | 0.00 | 0.67 | -16.36 | 154.12 | 29.07 | 230.43 | 0.6071 | -744.0 | -598.2 | |
| 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. | |