SDO HMI 2014-09-26 15:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.06 | 0.00 | 22.32 | -14.46 | 185.25 | -57.23 | 110.90 | 0.8733 | 2.0 | -36.3 | |
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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 |
| 0.00 | 1.15 | 0.00 | 1.10 | -13.54 | 187.01 | -55.47 | 110.45 | 0.8569 | 591.0 | 516.0 | |
| 0.00 | 3.44 | 0.00 | 3.35 | -14.54 | 186.58 | -55.90 | 111.42 | 0.8630 | 490.0 | 340.7 | |
| 0.00 | 1.32 | 0.00 | 1.29 | -14.31 | 186.62 | -55.86 | 111.18 | 0.8622 | 474.0 | 403.4 | |
| 0.00 | 1.06 | 0.00 | 1.02 | -13.44 | 186.77 | -55.71 | 110.26 | 0.8586 | 522.0 | 459.9 | |
| 0.00 | 2.12 | 0.00 | 2.06 | -14.11 | 186.47 | -56.01 | 110.90 | 0.8628 | 306.0 | 254.9 | |
| 0.00 | 1.94 | 0.00 | 1.92 | -13.14 | 185.71 | -56.77 | 109.58 | 0.8666 | 241.0 | 102.5 | |
| 0.00 | 1.32 | 0.00 | 1.33 | -13.85 | 185.27 | -57.21 | 110.23 | 0.8719 | -198.0 | -194.5 | |
| 0.00 | 2.12 | 0.00 | 2.23 | -15.71 | 184.30 | -58.18 | 111.96 | 0.8838 | -473.0 | -426.5 | |
| 0.00 | 0.97 | 0.00 | 1.03 | -15.55 | 183.96 | -58.52 | 111.68 | 0.8861 | -308.0 | -251.2 | |
| 0.00 | 0.71 | 0.00 | 0.74 | -15.15 | 184.14 | -58.34 | 111.30 | 0.8838 | -550.0 | -536.8 | |
| 0.00 | 1.94 | 0.00 | 2.05 | -14.84 | 183.97 | -58.51 | 110.92 | 0.8843 | -585.0 | -467.6 | |
| 0.00 | 3.97 | 0.00 | 4.20 | -14.64 | 183.76 | -58.72 | 110.63 | 0.8855 | -486.0 | -333.9 | |
| 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. | |