SDO HMI 2014-08-27 11:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.53 | 333.83 | 76.85 | 358.67 | 7.81 | 344.05 | 63.24 | 275.16 | 0.8899 | -381.4 | -312.5 | |
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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 | 2.15 | 0.00 | 2.73 | 7.89 | 348.43 | 67.62 | 275.59 | 0.9219 | -213.0 | -177.1 | |
| 0.00 | 1.62 | 0.00 | 2.04 | 8.11 | 348.34 | 67.53 | 275.83 | 0.9213 | -173.0 | -133.3 | |
| 6.28 | 11.31 | 7.80 | 14.02 | 8.37 | 347.95 | 67.14 | 276.08 | 0.9185 | -504.8 | -367.2 | |
| 1.44 | 2.96 | 1.73 | 3.58 | 9.73 | 347.36 | 66.55 | 277.52 | 0.9138 | 287.2 | 225.6 | |
| 0.90 | 3.59 | 1.04 | 4.17 | 7.46 | 346.20 | 65.39 | 274.94 | 0.9066 | 285.6 | 171.7 | |
| 16.51 | 305.01 | 18.08 | 324.84 | 7.11 | 344.45 | 63.64 | 274.40 | 0.8936 | 623.8 | -335.2 | |
| 2.51 | -6.00 | 2.70 | -6.00 | 7.38 | 343.90 | 63.09 | 274.66 | 0.8892 | -598.4 | 999999 | |
| 0.00 | 2.06 | 0.00 | 2.19 | 6.63 | 343.52 | 62.71 | 273.78 | 0.8865 | 52.0 | -41.2 | |
| 42.89 | -6.00 | 45.50 | -6.00 | 8.01 | 343.53 | 62.72 | 275.34 | 0.8858 | -854.4 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.99 | 10.32 | 342.06 | 61.25 | 277.88 | 0.8727 | 512.0 | 453.3 | |
| 0.00 | 1.62 | 0.00 | 1.63 | 10.92 | 342.14 | 61.33 | 278.58 | 0.8732 | 501.0 | 385.7 | |
| 0.00 | 1.53 | 0.00 | 1.51 | 9.76 | 341.50 | 60.69 | 277.21 | 0.8682 | -147.0 | -54.4 | |
| 0.00 | 0.99 | 0.00 | 0.97 | 8.96 | 341.26 | 60.45 | 276.27 | 0.8665 | -160.0 | -220.9 | |
| 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. | |