SDO HMI 2014-09-02 20:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.10 | 58.54 | 14.70 | 41.49 | -17.97 | 158.12 | -38.47 | 124.04 | 0.7162 | 315.8 | -212.1 | |
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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 | 0.80 | 0.00 | 0.57 | -22.06 | 161.14 | -35.44 | 131.02 | 0.7146 | 513.0 | 409.3 | |
| 12.87 | 28.87 | 8.91 | 20.01 | -17.64 | 159.41 | -37.18 | 124.52 | 0.7012 | 785.4 | 309.0 | |
| 4.92 | -2.00 | 3.40 | -2.00 | -17.36 | 159.24 | -37.35 | 124.05 | 0.7012 | 757.0 | 999999 | |
| 0.45 | -2.00 | 0.31 | -2.00 | -17.18 | 159.04 | -37.54 | 123.69 | 0.7020 | 457.6 | 999999 | |
| 0.00 | 2.50 | 0.00 | 1.72 | -16.30 | 158.97 | -37.62 | 122.54 | 0.6973 | 306.0 | 325.0 | |
| 0.00 | 0.63 | 0.00 | 0.47 | -21.98 | 157.09 | -39.50 | 128.02 | 0.7510 | 346.0 | 293.0 | |
| 0.00 | 1.61 | 0.00 | 1.14 | -17.53 | 157.53 | -39.05 | 123.12 | 0.7195 | 631.0 | 419.5 | |
| 0.00 | 0.80 | 0.00 | 0.59 | -19.03 | 156.75 | -39.83 | 124.40 | 0.7362 | -598.0 | -525.4 | |
| 1.34 | 15.55 | 0.97 | 11.32 | -18.25 | 156.85 | -39.74 | 123.54 | 0.7307 | -892.1 | -631.0 | |
| 0.89 | -9.00 | 0.65 | -9.00 | -18.67 | 156.60 | -39.98 | 123.88 | 0.7355 | -761.8 | 999999 | |
| 0.00 | 1.97 | 0.00 | 1.44 | -18.92 | 156.36 | -40.22 | 124.03 | 0.7394 | -477.0 | -385.6 | |
| 0.00 | 1.07 | 0.00 | 0.78 | -18.08 | 156.52 | -40.06 | 123.13 | 0.7329 | -817.0 | -720.8 | |
| 0.63 | 4.74 | 0.46 | 3.45 | -18.17 | 156.24 | -40.34 | 123.06 | 0.7362 | -843.1 | -609.0 | |
| 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. | |