SDO HMI 2014-11-07 10:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.67 | 0.00 | 9.06 | -22.17 | 76.01 | 24.79 | 221.20 | 0.5993 | 337.7 | 276.7 | |
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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 | 0.86 | 0.00 | 0.55 | -15.70 | 85.83 | 34.61 | 239.55 | 0.6366 | 614.0 | 540.5 | |
| 0.00 | 1.21 | 0.00 | 0.78 | -20.45 | 83.24 | 32.03 | 231.15 | 0.6403 | 479.0 | 313.8 | |
| 0.00 | 1.21 | 0.00 | 0.77 | -20.31 | 82.84 | 31.62 | 231.00 | 0.6350 | 575.0 | 434.1 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -19.28 | 82.02 | 30.80 | 231.68 | 0.6184 | 700.0 | 646.1 | |
| 0.00 | 0.60 | 0.00 | 0.38 | -19.50 | 82.03 | 30.81 | 231.39 | 0.6202 | 711.0 | 527.6 | |
| 0.00 | 0.86 | 0.00 | 0.55 | -21.13 | 82.17 | 30.95 | 229.37 | 0.6344 | 457.0 | 339.4 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -21.49 | 79.46 | 28.24 | 226.43 | 0.6099 | 661.0 | 521.6 | |
| 0.00 | 1.99 | 0.00 | 1.22 | -20.68 | 78.50 | 27.28 | 226.55 | 0.5930 | 660.0 | 547.0 | |
| 0.00 | 0.52 | 0.00 | 0.31 | -20.70 | 77.01 | 25.79 | 224.98 | 0.5780 | 184.0 | 307.2 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -24.02 | 76.56 | 25.34 | 220.38 | 0.6057 | 656.0 | 547.4 | |
| 0.00 | 0.60 | 0.00 | 0.36 | -21.41 | 75.76 | 24.55 | 222.70 | 0.5725 | 765.0 | 609.7 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -23.03 | 73.46 | 22.24 | 218.02 | 0.5678 | 652.0 | 517.3 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -25.17 | 65.74 | 14.52 | 205.24 | 0.5341 | -734.0 | -570.0 | |
| 0.00 | 1.21 | 0.00 | 0.72 | -28.69 | 58.50 | 7.28 | 191.73 | 0.5491 | -764.0 | -619.8 | |
| 0.00 | 0.69 | 0.00 | 0.42 | -32.07 | 52.45 | 1.23 | 181.79 | 0.5873 | -551.0 | -542.1 | |
| 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. | |