SDO HMI 2014-12-06 05:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.36 | 315.08 | 29.12 | 182.09 | -3.66 | 0.94 | -30.75 | 97.54 | 0.5168 | 1055.4 | 356.5 | |
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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 | 1.02 | 0.00 | 0.56 | -4.36 | 7.89 | -23.80 | 101.21 | 0.4120 | 944.0 | 787.0 | |
| 0.00 | 1.11 | 0.00 | 0.62 | -4.60 | 4.06 | -27.63 | 100.28 | 0.4718 | 726.0 | 600.8 | |
| 0.00 | 1.02 | 0.00 | 0.58 | -6.26 | 3.77 | -27.92 | 103.61 | 0.4809 | 823.0 | 670.8 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -7.63 | 3.58 | -28.11 | 106.28 | 0.4885 | 652.0 | 503.4 | |
| 0.00 | 1.54 | 0.00 | 0.87 | -5.40 | 3.62 | -28.07 | 101.78 | 0.4806 | 622.0 | 516.6 | |
| 0.00 | 2.73 | 0.00 | 1.54 | -4.06 | 3.61 | -28.08 | 99.02 | 0.4774 | 314.0 | 417.2 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -6.77 | 2.83 | -28.87 | 104.22 | 0.4966 | -661.0 | -543.9 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -4.72 | 1.06 | -30.63 | 99.59 | 0.5170 | 50.0 | 41.1 | |
| 1.71 | 303.31 | 0.99 | 175.40 | -4.01 | 0.92 | -30.77 | 98.19 | 0.5177 | 901.4 | 358.0 | |
| 47.54 | -9.00 | 27.48 | -9.00 | -3.59 | 0.87 | -30.82 | 97.38 | 0.5177 | 1335.9 | 999999 | |
| 1.11 | -9.00 | 0.65 | -9.00 | -3.62 | 0.28 | -31.41 | 97.31 | 0.5265 | 677.8 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.50 | -4.39 | 359.30 | -32.39 | 98.53 | 0.5422 | 502.0 | 421.0 | |
| 0.00 | 0.85 | 0.00 | 0.51 | -5.88 | 358.47 | -33.22 | 101.00 | 0.5573 | -731.0 | -554.1 | |
| 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. | |