SDO HMI 2014-10-13 23:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.34 | 515.32 | 38.58 | 286.89 | -20.88 | 17.37 | 3.61 | 187.43 | 0.4575 | 969.2 | 362.8 | |
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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 | 1.57 | 0.00 | 0.86 | -18.12 | 20.92 | 7.17 | 196.22 | 0.4262 | 977.0 | 810.2 | |
| 0.00 | 3.93 | 0.00 | 2.22 | -21.87 | 19.99 | 6.23 | 192.19 | 0.4792 | -879.0 | -706.4 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -18.16 | 19.31 | 5.55 | 192.68 | 0.4205 | 926.0 | 672.5 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -18.92 | 19.14 | 5.39 | 191.92 | 0.4316 | 869.0 | 774.8 | |
| 0.26 | 497.60 | 0.15 | 277.02 | -21.34 | 18.00 | 4.24 | 188.55 | 0.4657 | 830.3 | 392.6 | |
| 18.45 | -5.00 | 10.28 | -5.00 | -20.93 | 17.83 | 4.07 | 188.34 | 0.4591 | 1344.5 | 999999 | |
| 0.00 | 1.22 | 0.00 | 0.69 | -22.72 | 17.78 | 4.02 | 187.68 | 0.4863 | -195.0 | -119.6 | |
| 50.28 | -5.00 | 27.96 | -5.00 | -20.86 | 17.22 | 3.46 | 187.12 | 0.4567 | 1400.1 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.47 | -17.90 | 16.18 | 2.43 | 185.68 | 0.4085 | -847.0 | -763.7 | |
| 0.35 | 1.31 | 0.19 | 0.71 | -18.03 | 15.87 | 2.11 | 184.92 | 0.4101 | -851.2 | -814.4 | |
| 0.00 | 1.57 | 0.00 | 0.85 | -18.03 | 15.65 | 1.89 | 184.41 | 0.4098 | -858.0 | -750.2 | |
| 0.00 | 3.06 | 0.00 | 1.70 | -21.04 | 12.83 | -0.93 | 178.10 | 0.4565 | -1001.0 | -803.4 | |
| 0.00 | 0.87 | 0.00 | 0.50 | -24.04 | 12.12 | -1.64 | 177.01 | 0.5030 | -585.0 | -566.2 | |
| 0.00 | 0.61 | 0.00 | 0.36 | -25.48 | 11.10 | -2.65 | 175.42 | 0.5255 | -738.0 | -556.1 | |
| 0.00 | 0.70 | 0.00 | 0.41 | -25.87 | 9.89 | -3.86 | 173.44 | 0.5330 | -589.0 | -415.4 | |
| 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. | |