SDO HMI 2014-12-01 11:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.79 | 187.83 | 51.60 | 254.78 | 3.26 | 162.79 | 68.48 | 273.19 | 0.9313 | -245.7 | -97.2 | |
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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 | 1.45 | 0.00 | 2.10 | 3.24 | 164.30 | 69.99 | 273.14 | 0.9411 | 274.0 | 255.6 | |
| 12.39 | 157.75 | 17.63 | 220.31 | 2.50 | 163.94 | 69.62 | 272.35 | 0.9389 | -406.4 | -101.7 | |
| 20.08 | -2.00 | 27.47 | -2.00 | 3.34 | 163.12 | 68.81 | 273.26 | 0.9339 | -476.9 | 999999 | |
| 0.00 | 0.77 | 0.00 | 1.02 | 4.36 | 162.32 | 68.01 | 274.37 | 0.9289 | -277.0 | -228.7 | |
| 0.00 | 4.27 | 0.00 | 5.58 | 3.86 | 161.99 | 67.68 | 273.83 | 0.9267 | -666.0 | -552.1 | |
| 0.00 | 1.11 | 0.00 | 1.43 | 3.04 | 161.63 | 67.32 | 272.94 | 0.9243 | -546.0 | -528.3 | |
| 0.00 | 4.36 | 0.00 | 5.22 | 3.83 | 159.87 | 65.56 | 273.83 | 0.9122 | -616.0 | -460.3 | |
| 0.00 | 0.85 | 0.00 | 1.02 | 4.34 | 159.81 | 65.50 | 274.38 | 0.9118 | 39.0 | 20.1 | |
| 0.00 | 1.54 | 0.00 | 1.81 | 4.46 | 159.47 | 65.16 | 274.53 | 0.9093 | 374.0 | 217.1 | |
| 0.00 | 1.37 | 0.00 | 1.49 | 3.36 | 157.32 | 63.01 | 273.34 | 0.8930 | 477.0 | 393.5 | |
| 0.00 | 0.26 | 0.00 | 0.27 | 3.79 | 156.40 | 62.09 | 273.84 | 0.8857 | 480.0 | 482.7 | |
| 0.00 | 0.77 | 0.00 | 0.81 | 5.76 | 156.14 | 61.83 | 276.08 | 0.8840 | 346.0 | 302.3 | |
| 0.00 | 1.97 | 0.00 | 2.05 | 6.24 | 155.86 | 61.55 | 276.63 | 0.8819 | 306.0 | 252.4 | |
| 0.00 | 0.51 | 0.00 | 0.53 | 5.82 | 155.65 | 61.34 | 276.17 | 0.8800 | 404.0 | 386.0 | |
| 6.32 | 10.85 | 6.50 | 11.14 | 6.45 | 155.40 | 61.09 | 276.90 | 0.8782 | 621.6 | 409.5 | |
| 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. | |