SDO HMI 2014-11-10 22:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.93 | 0.00 | 11.98 | -9.04 | 337.78 | -27.28 | 114.69 | 0.4995 | -232.3 | -125.6 | |
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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 |
| 0.00 | 2.15 | 0.00 | 1.14 | -5.51 | 346.09 | -18.96 | 115.03 | 0.3586 | 700.0 | 546.3 | |
| 0.00 | 1.81 | 0.00 | 1.00 | -6.77 | 340.50 | -24.55 | 112.46 | 0.4484 | 755.0 | 631.1 | |
| 0.00 | 1.55 | 0.00 | 0.88 | -11.20 | 339.77 | -25.29 | 120.39 | 0.4878 | 757.0 | 611.6 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -6.79 | 340.01 | -25.05 | 112.09 | 0.4556 | 723.0 | 528.9 | |
| 0.00 | 2.50 | 0.00 | 1.41 | -6.97 | 338.50 | -26.56 | 111.32 | 0.4783 | 713.0 | 514.3 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -9.95 | 336.98 | -28.08 | 115.73 | 0.5167 | -728.0 | -607.4 | |
| 0.00 | 1.64 | 0.00 | 0.95 | -10.03 | 336.29 | -28.77 | 115.34 | 0.5265 | -879.0 | -787.8 | |
| 0.00 | 1.29 | 0.00 | 0.76 | -12.06 | 336.06 | -28.99 | 118.62 | 0.5421 | -714.0 | -609.9 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -10.41 | 336.04 | -29.02 | 115.81 | 0.5320 | -640.0 | -514.7 | |
| 0.00 | 1.64 | 0.00 | 0.96 | -10.86 | 335.30 | -29.76 | 116.02 | 0.5446 | -809.0 | -717.4 | |
| 0.00 | 1.03 | 0.00 | 0.61 | -10.18 | 335.37 | -29.69 | 114.93 | 0.5396 | -622.0 | -553.0 | |
| 0.00 | 1.21 | 0.00 | 0.71 | -10.31 | 335.18 | -29.87 | 115.01 | 0.5429 | -729.0 | -640.9 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -9.41 | 334.75 | -30.30 | 113.17 | 0.5436 | -668.0 | -562.3 | |
| 0.00 | 1.29 | 0.00 | 0.77 | -10.79 | 334.32 | -30.73 | 115.22 | 0.5570 | -699.0 | -547.5 | |
| 0.00 | 1.03 | 0.00 | 0.61 | -7.61 | 334.04 | -31.01 | 109.61 | 0.5443 | -644.0 | -504.6 | |
| 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. | |