SDO HMI 2014-11-09 21:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.37 | 0.00 | 9.08 | -10.03 | 337.76 | -41.04 | 108.69 | 0.6843 | -88.0 | -88.4 | |
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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 | 1.03 | 0.00 | 0.65 | -9.88 | 343.26 | -35.54 | 111.00 | 0.6156 | -582.0 | -420.3 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -4.86 | 342.40 | -36.39 | 102.70 | 0.6082 | 533.0 | 445.5 | |
| 0.00 | 0.78 | 0.00 | 0.51 | -10.14 | 340.35 | -38.45 | 109.97 | 0.6536 | 354.0 | 329.0 | |
| 0.00 | 0.34 | 0.00 | 0.23 | -10.33 | 340.16 | -38.63 | 110.16 | 0.6566 | 523.0 | 450.5 | |
| 0.00 | 0.86 | 0.00 | 0.57 | -11.84 | 339.77 | -39.03 | 112.15 | 0.6678 | 536.0 | 392.5 | |
| 0.00 | 1.21 | 0.00 | 0.80 | -11.23 | 339.67 | -39.12 | 111.24 | 0.6663 | 542.0 | 463.6 | |
| 0.00 | 1.21 | 0.00 | 0.78 | -7.06 | 339.80 | -38.99 | 105.19 | 0.6494 | 631.0 | 500.2 | |
| 0.00 | 0.78 | 0.00 | 0.54 | -10.98 | 336.06 | -42.73 | 109.34 | 0.7084 | -624.0 | -524.8 | |
| 0.00 | 1.38 | 0.00 | 0.98 | -12.04 | 335.65 | -43.15 | 110.60 | 0.7169 | -602.0 | -484.8 | |
| 0.00 | 0.69 | 0.00 | 0.49 | -11.85 | 335.64 | -43.15 | 110.35 | 0.7163 | -621.0 | -557.2 | |
| 0.00 | 0.95 | 0.00 | 0.65 | -6.09 | 336.26 | -42.54 | 102.60 | 0.6912 | -278.0 | -332.2 | |
| 0.00 | 0.69 | 0.00 | 0.49 | -11.53 | 335.37 | -43.42 | 109.81 | 0.7182 | -332.0 | -351.0 | |
| 0.00 | 0.95 | 0.00 | 0.68 | -12.37 | 335.08 | -43.72 | 110.81 | 0.7245 | -591.0 | -466.3 | |
| 0.00 | 0.43 | 0.00 | 0.30 | -9.97 | 335.37 | -43.43 | 107.71 | 0.7131 | -572.0 | -514.6 | |
| 0.00 | 1.12 | 0.00 | 0.82 | -10.31 | 333.18 | -45.61 | 107.40 | 0.7391 | -237.0 | -193.2 | |
| 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. | |