SDO HMI 2014-10-12 00:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.13 | 481.60 | 39.02 | 289.05 | -20.62 | 17.66 | -21.93 | 141.73 | 0.5662 | 1000.6 | 339.5 | |
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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 | 2.10 | 0.00 | 1.22 | -18.64 | 20.01 | -19.58 | 142.45 | 0.5230 | 276.0 | 307.4 | |
| 0.00 | 1.84 | 0.00 | 1.06 | -18.12 | 20.04 | -19.55 | 141.84 | 0.5166 | 929.0 | 706.9 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -18.22 | 19.90 | -19.69 | 141.76 | 0.5192 | 663.0 | 624.2 | |
| 0.00 | 0.44 | 0.00 | 0.25 | -18.46 | 19.57 | -20.02 | 141.60 | 0.5250 | 695.0 | 679.2 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -19.63 | 19.25 | -20.34 | 142.59 | 0.5411 | 387.0 | 414.0 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -19.03 | 19.29 | -20.30 | 141.93 | 0.5339 | 692.0 | 607.9 | |
| 65.13 | 460.48 | 39.02 | 275.95 | -20.62 | 17.84 | -21.75 | 141.93 | 0.5646 | 1370.3 | 365.6 | |
| 0.00 | 1.58 | 0.00 | 0.97 | -20.81 | 14.25 | -25.34 | 137.93 | 0.5994 | 283.0 | 238.1 | |
| 0.00 | 0.61 | 0.00 | 0.36 | -13.22 | 14.59 | -25.00 | 128.00 | 0.5241 | -740.0 | -610.1 | |
| 0.00 | 1.93 | 0.00 | 1.12 | -13.11 | 14.37 | -25.22 | 127.58 | 0.5257 | -756.0 | -673.3 | |
| 0.00 | 2.19 | 0.00 | 1.40 | -22.25 | 11.83 | -27.76 | 137.09 | 0.6353 | -460.0 | -339.4 | |
| 0.00 | 2.19 | 0.00 | 1.48 | -25.98 | 10.36 | -29.23 | 139.78 | 0.6822 | -595.0 | -479.2 | |
| 0.00 | 2.89 | 0.00 | 1.97 | -26.39 | 9.89 | -29.70 | 139.79 | 0.6897 | -686.0 | -555.1 | |
| 0.00 | 1.93 | 0.00 | 1.20 | -18.24 | 10.72 | -28.87 | 131.08 | 0.6107 | -675.0 | -562.0 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -20.66 | 2.93 | -36.66 | 127.63 | 0.7078 | -429.0 | -424.8 | |
| 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. | |