SDO HMI 2014-09-15 04:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.64 | 38.41 | 4.89 | 24.32 | -15.69 | 64.94 | 31.23 | 233.26 | 0.6250 | 201.2 | 367.2 | |
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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 | 1.51 | 0.00 | 0.99 | -17.23 | 67.21 | 33.50 | 233.23 | 0.6603 | 523.0 | 441.1 | |
| 2.13 | 23.74 | 1.37 | 15.19 | -15.22 | 66.52 | 32.81 | 235.29 | 0.6384 | 634.2 | 710.5 | |
| 2.49 | -2.00 | 1.59 | -2.00 | -15.30 | 66.28 | 32.57 | 234.98 | 0.6363 | 828.5 | 999999 | |
| 3.02 | -2.00 | 1.93 | -2.00 | -15.28 | 65.98 | 32.27 | 234.76 | 0.6328 | 890.1 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.50 | -14.82 | 65.05 | 31.34 | 234.59 | 0.6192 | 744.0 | 622.4 | |
| 0.00 | 2.49 | 0.00 | 1.55 | -15.23 | 63.88 | 30.17 | 233.01 | 0.6094 | -480.0 | -435.4 | |
| 0.00 | 0.98 | 0.00 | 0.62 | -17.84 | 64.11 | 30.40 | 229.81 | 0.6329 | 552.0 | 466.1 | |
| 0.00 | 3.91 | 0.00 | 2.40 | -14.69 | 62.54 | 28.83 | 232.50 | 0.5902 | 682.0 | 366.9 | |
| 0.00 | 1.24 | 0.00 | 0.78 | -19.05 | 61.35 | 27.64 | 225.63 | 0.6157 | -399.0 | -331.6 | |
| 0.00 | 0.80 | 0.00 | 0.50 | -18.76 | 60.87 | 27.16 | 225.50 | 0.6082 | -519.0 | -443.7 | |
| 0.00 | 1.16 | 0.00 | 0.70 | -16.14 | 60.31 | 26.60 | 228.27 | 0.5785 | -691.0 | -498.6 | |
| 0.00 | 0.98 | 0.00 | 0.60 | -17.19 | 60.18 | 26.47 | 226.76 | 0.5868 | -749.0 | -609.8 | |
| 0.00 | 0.80 | 0.00 | 0.49 | -18.96 | 58.70 | 24.99 | 222.90 | 0.5891 | -571.0 | -472.2 | |
| 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. | |