SDO HMI 2014-11-12 10:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.50 | 0.00 | 8.95 | -9.44 | 338.56 | -6.74 | 153.27 | 0.2522 | 152.8 | 42.2 | |
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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 | 1.21 | 0.00 | 0.60 | -4.98 | 343.67 | -1.63 | 168.69 | 0.1450 | 978.0 | 819.3 | |
| 0.00 | 1.03 | 0.00 | 0.52 | -5.58 | 342.47 | -2.82 | 162.11 | 0.1603 | 757.0 | 543.2 | |
| 0.00 | 1.12 | 0.00 | 0.57 | -9.87 | 342.08 | -3.22 | 166.21 | 0.2332 | 809.0 | 672.7 | |
| 0.00 | 1.98 | 0.00 | 1.01 | -11.09 | 341.58 | -3.72 | 165.50 | 0.2554 | 839.0 | 716.0 | |
| 0.00 | 1.64 | 0.00 | 0.84 | -10.97 | 341.31 | -3.99 | 164.37 | 0.2546 | 773.0 | 532.3 | |
| 0.00 | 1.81 | 0.00 | 0.91 | -6.76 | 339.71 | -5.59 | 150.66 | 0.1982 | 778.0 | 629.2 | |
| 0.00 | 2.93 | 0.00 | 1.52 | -12.25 | 336.86 | -8.44 | 151.60 | 0.3028 | -665.0 | -513.2 | |
| 0.00 | 2.07 | 0.00 | 1.06 | -9.77 | 336.75 | -8.55 | 146.73 | 0.2682 | -644.0 | -566.8 | |
| 0.00 | 1.64 | 0.00 | 0.85 | -10.43 | 334.80 | -10.49 | 142.58 | 0.2961 | -569.0 | -482.0 | |
| 0.00 | 1.64 | 0.00 | 0.85 | -8.11 | 333.23 | -12.07 | 133.17 | 0.2851 | -864.0 | -728.3 | |
| 0.00 | 0.43 | 0.00 | 0.22 | -7.72 | 332.69 | -12.61 | 130.91 | 0.2875 | -511.0 | -547.8 | |
| 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. | |