SDO HMI 2014-09-20 04:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.09 | 0.00 | 9.56 | 8.63 | 331.91 | 4.21 | 237.43 | 0.1169 | 140.5 | 228.5 | |
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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 | 1.24 | 0.00 | 0.64 | 6.81 | 345.20 | 17.50 | 270.05 | 0.2999 | -683.0 | -518.3 | |
| 0.00 | 2.31 | 0.00 | 1.19 | 7.83 | 344.42 | 16.72 | 273.54 | 0.2868 | -627.0 | -526.1 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 9.92 | 339.44 | 11.74 | 284.38 | 0.2078 | -893.0 | -712.0 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 10.04 | 337.98 | 10.28 | 286.78 | 0.1843 | -720.0 | -504.9 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 9.84 | 334.26 | 6.56 | 293.22 | 0.1231 | -893.0 | -731.6 | |
| 0.00 | 0.89 | 0.00 | 0.44 | 13.55 | 332.86 | 5.16 | 322.12 | 0.1431 | -574.0 | -405.4 | |
| 0.00 | 3.02 | 0.00 | 1.49 | 7.66 | 329.14 | 1.43 | 291.02 | 0.0267 | 769.0 | 739.3 | |
| 0.00 | 0.89 | 0.00 | 0.44 | 7.87 | 329.11 | 1.41 | 298.54 | 0.0278 | 935.0 | 812.6 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 7.76 | 328.56 | 0.86 | 306.86 | 0.0186 | 945.0 | 699.7 | |
| 0.00 | 1.86 | 0.00 | 0.92 | 7.73 | 328.13 | 0.43 | 324.82 | 0.0130 | 1106.0 | 877.0 | |
| 0.00 | 2.93 | 0.00 | 1.45 | 7.61 | 326.71 | -1.00 | 63.64 | 0.0193 | 780.0 | 673.0 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 10.05 | 318.13 | -9.57 | 72.11 | 0.1729 | 854.0 | 555.5 | |
| 0.00 | 0.62 | 0.00 | 0.32 | 14.54 | 317.02 | -10.68 | 53.83 | 0.2233 | 828.0 | 733.0 | |
| 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. | |