SDO HMI 2014-11-30 11:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.09 | 0.00 | 13.55 | -23.14 | 92.86 | -14.63 | 150.39 | 0.4730 | -387.5 | -363.5 | |
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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 | 1.45 | 0.00 | 0.81 | -25.42 | 100.97 | -6.52 | 167.00 | 0.4581 | 708.0 | 483.1 | |
| 0.00 | 1.11 | 0.00 | 0.61 | -22.49 | 97.50 | -9.99 | 158.05 | 0.4308 | 814.0 | 584.5 | |
| 0.00 | 1.62 | 0.00 | 0.89 | -20.54 | 94.41 | -13.08 | 149.96 | 0.4250 | -783.0 | -624.7 | |
| 0.00 | 1.11 | 0.00 | 0.63 | -24.16 | 93.39 | -14.10 | 152.34 | 0.4809 | -633.0 | -670.0 | |
| 0.00 | 2.56 | 0.00 | 1.45 | -24.03 | 93.00 | -14.49 | 151.57 | 0.4820 | -635.0 | -598.2 | |
| 0.00 | 1.11 | 0.00 | 0.63 | -23.77 | 92.66 | -14.83 | 150.74 | 0.4811 | -893.0 | -821.1 | |
| 0.00 | 6.41 | 0.00 | 3.61 | -23.48 | 92.43 | -15.06 | 150.03 | 0.4791 | -830.0 | -569.3 | |
| 0.00 | 1.37 | 0.00 | 0.76 | -20.78 | 91.94 | -15.55 | 145.88 | 0.4487 | -790.0 | -597.5 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -20.59 | 91.70 | -15.79 | 145.22 | 0.4485 | -714.0 | -530.9 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -25.68 | 90.92 | -16.57 | 150.16 | 0.5185 | -661.0 | -547.8 | |
| 0.00 | 0.68 | 0.00 | 0.39 | -24.10 | 90.54 | -16.96 | 147.83 | 0.5020 | -617.0 | -581.6 | |
| 0.00 | 2.48 | 0.00 | 1.37 | -20.14 | 90.86 | -16.63 | 143.24 | 0.4508 | 798.0 | 571.3 | |
| 0.00 | 2.22 | 0.00 | 1.29 | -25.16 | 90.11 | -17.38 | 148.41 | 0.5182 | -801.0 | -591.2 | |
| 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. | |