SDO HMI 2014-10-14 12:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.63 | 364.12 | 52.49 | 274.37 | -8.92 | 319.94 | -46.69 | 107.36 | 0.7544 | 506.6 | 250.6 | |
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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 |
| 30.25 | 331.70 | 22.39 | 244.95 | -9.15 | 320.93 | -45.70 | 107.98 | 0.7452 | 842.3 | 303.2 | |
| 27.01 | -1.00 | 19.92 | -1.00 | -8.63 | 320.97 | -45.66 | 107.31 | 0.7430 | 921.3 | 999999 | |
| 0.87 | -1.00 | 0.64 | -1.00 | -8.29 | 320.98 | -45.65 | 106.87 | 0.7418 | 756.1 | 999999 | |
| 1.40 | -1.00 | 1.04 | -1.00 | -8.73 | 320.39 | -46.24 | 107.23 | 0.7498 | 198.5 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.53 | -7.91 | 319.50 | -47.13 | 105.86 | 0.7570 | -191.0 | -125.2 | |
| 0.00 | 1.31 | 0.00 | 1.00 | -6.42 | 318.49 | -48.14 | 103.64 | 0.7638 | 464.0 | 354.2 | |
| 0.00 | 0.61 | 0.00 | 0.49 | -8.30 | 316.45 | -50.18 | 105.37 | 0.7905 | 529.0 | 432.4 | |
| 0.00 | 2.27 | 0.00 | 2.00 | -9.92 | 312.95 | -53.68 | 106.25 | 0.8289 | -706.0 | -587.4 | |
| 0.00 | 1.57 | 0.00 | 1.36 | -8.29 | 313.20 | -53.43 | 104.41 | 0.8227 | -585.0 | -427.9 | |
| 0.00 | 1.92 | 0.00 | 1.70 | -9.74 | 312.83 | -53.80 | 106.01 | 0.8296 | -513.0 | -495.2 | |
| 0.00 | 1.05 | 0.00 | 0.93 | -9.91 | 312.64 | -53.99 | 106.16 | 0.8318 | -515.0 | -447.2 | |
| 0.00 | 1.57 | 0.00 | 1.40 | -9.99 | 312.46 | -54.17 | 106.20 | 0.8336 | -395.0 | -326.6 | |
| 0.00 | 0.79 | 0.00 | 0.73 | -11.22 | 311.06 | -55.57 | 107.22 | 0.8491 | -327.0 | -243.1 | |
| 6.91 | 16.70 | 6.42 | 15.54 | -8.98 | 310.57 | -56.06 | 104.51 | 0.8485 | -579.4 | -181.3 | |
| 2.19 | 3.93 | 2.08 | 3.74 | -9.95 | 310.05 | -56.58 | 105.48 | 0.8551 | -380.8 | -304.8 | |
| 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. | |