SDO HMI 2014-11-06 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.31 | 0.00 | 12.69 | -23.03 | 77.02 | 18.12 | 213.23 | 0.5534 | 422.2 | 335.2 | |
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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 | 2.24 | 0.00 | 1.44 | -27.07 | 84.38 | 25.48 | 217.05 | 0.6381 | -705.0 | -587.4 | |
| 0.00 | 1.55 | 0.00 | 0.92 | -19.77 | 82.65 | 23.75 | 223.83 | 0.5493 | 824.0 | 622.9 | |
| 0.00 | 1.21 | 0.00 | 0.72 | -20.16 | 82.57 | 23.67 | 223.23 | 0.5524 | 752.0 | 560.4 | |
| 0.00 | 1.47 | 0.00 | 0.87 | -20.38 | 82.50 | 23.60 | 222.85 | 0.5540 | 779.0 | 643.6 | |
| 0.00 | 1.47 | 0.00 | 0.87 | -19.76 | 82.34 | 23.43 | 223.48 | 0.5461 | 758.0 | 523.6 | |
| 0.00 | 4.14 | 0.00 | 2.43 | -21.04 | 80.27 | 21.36 | 219.27 | 0.5393 | 797.0 | 662.3 | |
| 0.00 | 1.29 | 0.00 | 0.75 | -20.72 | 78.05 | 19.15 | 216.70 | 0.5155 | 740.0 | 561.0 | |
| 0.00 | 1.04 | 0.00 | 0.59 | -21.27 | 76.31 | 17.41 | 213.51 | 0.5070 | 744.0 | 635.7 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -23.69 | 76.39 | 17.48 | 210.95 | 0.5371 | 764.0 | 616.1 | |
| 0.00 | 2.33 | 0.00 | 1.34 | -22.01 | 75.63 | 16.73 | 211.65 | 0.5106 | 516.0 | 402.9 | |
| 0.00 | 1.64 | 0.00 | 0.91 | -18.10 | 75.05 | 16.14 | 215.49 | 0.4571 | 736.0 | 566.3 | |
| 0.00 | 0.95 | 0.00 | 0.61 | -35.97 | 54.60 | -4.30 | 174.58 | 0.6449 | -575.0 | -454.8 | |
| 0.00 | 1.12 | 0.00 | 0.73 | -36.20 | 49.95 | -8.95 | 168.94 | 0.6567 | -641.0 | -522.9 | |
| 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. | |