SDO HMI 2014-10-07 12:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.37 | 0.00 | 10.68 | -13.57 | 58.83 | -40.15 | 116.76 | 0.7034 | 109.5 | 159.3 | |
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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 | 1.93 | 0.00 | 1.27 | -12.75 | 62.05 | -36.93 | 117.57 | 0.6633 | 753.0 | 690.2 | |
| 0.00 | 1.40 | 0.00 | 0.94 | -13.18 | 61.40 | -37.58 | 117.74 | 0.6732 | 673.0 | 515.2 | |
| 0.00 | 1.76 | 0.00 | 1.17 | -12.99 | 61.35 | -37.63 | 117.46 | 0.6727 | 708.0 | 553.5 | |
| 0.00 | 1.05 | 0.00 | 0.70 | -13.10 | 61.22 | -37.76 | 117.51 | 0.6748 | 594.0 | 540.4 | |
| 0.00 | 1.40 | 0.00 | 0.96 | -13.25 | 59.49 | -39.49 | 116.69 | 0.6952 | 416.0 | 416.8 | |
| 0.00 | 0.97 | 0.00 | 0.68 | -13.32 | 58.06 | -40.92 | 115.99 | 0.7114 | -558.0 | -484.4 | |
| 0.00 | 1.23 | 0.00 | 0.87 | -13.35 | 57.68 | -41.29 | 115.82 | 0.7156 | -776.0 | -653.6 | |
| 0.00 | 0.88 | 0.00 | 0.62 | -12.99 | 57.47 | -41.51 | 115.24 | 0.7162 | -572.0 | -475.7 | |
| 0.00 | 1.23 | 0.00 | 0.87 | -13.35 | 57.36 | -41.62 | 115.64 | 0.7192 | -564.0 | -415.5 | |
| 0.00 | 0.97 | 0.00 | 0.68 | -12.20 | 57.10 | -41.88 | 114.02 | 0.7167 | -523.0 | -464.2 | |
| 0.00 | 0.97 | 0.00 | 0.72 | -15.47 | 55.80 | -43.18 | 117.49 | 0.7458 | 414.0 | 459.2 | |
| 0.00 | 1.32 | 0.00 | 0.98 | -15.68 | 55.61 | -43.37 | 117.65 | 0.7486 | 431.0 | 359.5 | |
| 0.00 | 0.26 | 0.00 | 0.22 | -18.69 | 51.70 | -47.28 | 119.26 | 0.7999 | 427.0 | 460.0 | |
| 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. | |