SDO HMI 2014-11-09 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 | 15.69 | 0.00 | 10.52 | -10.41 | 338.07 | -40.17 | 109.67 | 0.6751 | -103.7 | -57.2 | |
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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 | 0.95 | 0.00 | 0.59 | -9.92 | 343.22 | -35.02 | 111.34 | 0.6091 | -599.0 | -401.3 | |
| 0.00 | 2.41 | 0.00 | 1.52 | -9.68 | 342.17 | -36.07 | 110.43 | 0.6216 | 686.0 | 465.7 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -9.99 | 342.14 | -36.11 | 110.87 | 0.6234 | 588.0 | 465.5 | |
| 0.00 | 0.69 | 0.00 | 0.43 | -6.02 | 342.40 | -35.84 | 104.76 | 0.6044 | 574.0 | 503.9 | |
| 0.00 | 1.12 | 0.00 | 0.73 | -11.23 | 339.94 | -38.30 | 111.63 | 0.6563 | 605.0 | 532.1 | |
| 0.00 | 1.72 | 0.00 | 1.13 | -11.82 | 339.80 | -38.44 | 112.41 | 0.6605 | 564.0 | 477.5 | |
| 0.00 | 0.78 | 0.00 | 0.54 | -10.99 | 336.08 | -42.16 | 109.57 | 0.7016 | -573.0 | -488.2 | |
| 0.00 | 0.78 | 0.00 | 0.54 | -12.05 | 335.68 | -42.56 | 110.85 | 0.7102 | -376.0 | -418.4 | |
| 0.00 | 0.95 | 0.00 | 0.66 | -11.86 | 335.67 | -42.57 | 110.60 | 0.7096 | -575.0 | -554.7 | |
| 0.00 | 1.03 | 0.00 | 0.73 | -11.51 | 335.37 | -42.87 | 109.99 | 0.7118 | -346.0 | -311.2 | |
| 0.00 | 1.21 | 0.00 | 0.86 | -12.35 | 335.12 | -43.12 | 111.02 | 0.7177 | -451.0 | -397.7 | |
| 0.00 | 0.78 | 0.00 | 0.55 | -9.40 | 334.58 | -43.66 | 106.84 | 0.7140 | -576.0 | -475.7 | |
| 0.00 | 1.46 | 0.00 | 1.03 | -8.53 | 334.42 | -43.82 | 105.60 | 0.7133 | -507.0 | -466.6 | |
| 0.00 | 0.95 | 0.00 | 0.67 | -9.26 | 334.26 | -43.98 | 106.55 | 0.7173 | -466.0 | -460.1 | |
| 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. | |