SDO HMI 2014-08-13 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.35 | 42.28 | 13.90 | 43.54 | -18.56 | 160.92 | 56.74 | 244.65 | 0.8791 | 353.1 | 293.3 | |
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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 |
| 3.34 | 8.75 | 3.56 | 9.31 | -16.17 | 162.81 | 58.63 | 247.86 | 0.8872 | 404.4 | 240.6 | |
| 2.89 | -1.00 | 3.07 | -1.00 | -16.36 | 162.71 | 58.53 | 247.63 | 0.8869 | 490.2 | 999999 | |
| 0.00 | 1.17 | 0.00 | 1.21 | -17.67 | 161.13 | 56.95 | 245.69 | 0.8783 | 317.0 | 291.7 | |
| 0.00 | 1.53 | 0.00 | 1.61 | -19.16 | 161.25 | 57.07 | 244.12 | 0.8831 | 272.0 | 178.4 | |
| 0.99 | 20.20 | 1.04 | 20.78 | -19.41 | 161.09 | 56.91 | 243.80 | 0.8826 | 342.2 | 323.5 | |
| 3.70 | -5.00 | 3.82 | -5.00 | -19.08 | 160.73 | 56.55 | 244.03 | 0.8791 | 684.8 | 999999 | |
| 0.00 | 2.16 | 0.00 | 2.19 | -18.63 | 160.21 | 56.03 | 244.33 | 0.8739 | 678.0 | 525.9 | |
| 0.00 | 1.35 | 0.00 | 1.36 | -18.31 | 159.99 | 55.81 | 244.60 | 0.8714 | 496.0 | 474.0 | |
| 0.00 | 1.98 | 0.00 | 2.01 | -18.99 | 160.16 | 55.98 | 243.92 | 0.8745 | 701.0 | 609.0 | |
| 0.00 | 0.72 | 0.00 | 0.70 | -18.65 | 158.74 | 54.57 | 243.77 | 0.8626 | -167.0 | -180.2 | |
| 2.43 | 4.42 | 2.41 | 4.37 | -20.47 | 158.65 | 54.47 | 241.76 | 0.8674 | -492.1 | -322.4 | |
| 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. | |