SDO HMI 2011-02-14 09:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.67 | 134.96 | 33.13 | 91.11 | 20.05 | 64.42 | 33.90 | 309.63 | 0.6821 | 118.7 | 284.9 | |
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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 |
| 18.25 | 38.30 | 12.87 | 26.99 | 19.51 | 68.07 | 37.54 | 306.17 | 0.7139 | -842.6 | -364.5 | |
| 0.00 | 1.54 | 0.00 | 1.07 | 19.03 | 67.35 | 36.82 | 306.10 | 0.7036 | -443.0 | -528.6 | |
| 0.00 | 0.26 | 0.00 | 0.18 | 20.77 | 67.31 | 36.78 | 308.20 | 0.7148 | -529.0 | -488.0 | |
| 0.00 | 0.60 | 0.00 | 0.41 | 19.26 | 66.43 | 35.91 | 307.04 | 0.6960 | -602.0 | -532.7 | |
| 0.00 | 1.11 | 0.00 | 0.74 | 19.00 | 64.23 | 33.70 | 308.43 | 0.6720 | 452.0 | 382.9 | |
| 3.34 | 7.88 | 2.22 | 5.24 | 19.21 | 63.90 | 33.37 | 308.95 | 0.6703 | 810.5 | 587.3 | |
| 0.00 | 2.83 | 0.00 | 1.87 | 18.90 | 63.64 | 33.11 | 308.78 | 0.6653 | 701.0 | 675.7 | |
| 4.28 | 5.31 | 2.91 | 3.61 | 21.73 | 63.57 | 33.05 | 312.22 | 0.6864 | -670.1 | -584.6 | |
| 4.54 | 67.10 | 2.99 | 44.32 | 19.75 | 62.71 | 32.19 | 310.60 | 0.6626 | 1176.0 | 552.8 | |
| 13.03 | -9.00 | 8.63 | -9.00 | 20.21 | 62.74 | 32.22 | 311.13 | 0.6666 | 894.9 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.91 | 20.62 | 62.84 | 32.31 | 311.53 | 0.6707 | 316.0 | 231.1 | |
| 0.60 | -9.00 | 0.40 | -9.00 | 20.06 | 62.37 | 31.85 | 311.26 | 0.6617 | 932.9 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.79 | 21.04 | 61.71 | 31.18 | 313.02 | 0.6633 | 633.0 | 544.3 | |
| 0.00 | 1.03 | 0.00 | 0.67 | 20.59 | 61.38 | 30.86 | 312.77 | 0.6564 | 725.0 | 639.9 | |
| 4.63 | 6.43 | 3.11 | 4.31 | 23.23 | 61.28 | 30.75 | 315.91 | 0.6776 | 706.7 | 585.9 | |
| 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. | |