SDO HMI 2014-05-14 12:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.06 | 256.61 | 33.67 | 166.66 | -23.78 | 193.91 | -35.45 | 124.68 | 0.6473 | 714.0 | 267.9 | |
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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 |
| 5.92 | 246.63 | 3.80 | 159.55 | -23.70 | 194.66 | -34.69 | 125.04 | 0.6388 | 1151.1 | 297.7 | |
| 12.48 | -1.00 | 8.03 | -1.00 | -23.59 | 194.45 | -34.90 | 124.76 | 0.6405 | 1099.3 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -22.62 | 194.58 | -34.77 | 123.46 | 0.6333 | 651.0 | 542.9 | |
| 16.07 | -1.00 | 10.42 | -1.00 | -23.94 | 193.94 | -35.42 | 124.91 | 0.6482 | 853.0 | 999999 | |
| 16.96 | -1.00 | 10.96 | -1.00 | -23.52 | 194.03 | -35.32 | 124.38 | 0.6447 | 997.6 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -23.17 | 193.12 | -36.23 | 123.34 | 0.6528 | 471.0 | 354.8 | |
| 0.00 | 0.81 | 0.00 | 0.53 | -23.26 | 192.01 | -37.34 | 122.84 | 0.6655 | 344.0 | 260.1 | |
| 0.00 | 0.63 | 0.00 | 0.45 | -25.74 | 188.06 | -41.29 | 124.03 | 0.7196 | -696.0 | -564.0 | |
| 0.00 | 1.62 | 0.00 | 1.18 | -26.30 | 186.72 | -42.63 | 124.09 | 0.7355 | -693.0 | -624.7 | |
| 0.63 | 1.79 | 0.46 | 1.31 | -26.06 | 186.41 | -42.94 | 123.65 | 0.7374 | -694.0 | -620.8 | |
| 0.00 | 0.81 | 0.00 | 0.59 | -26.25 | 186.23 | -43.12 | 123.81 | 0.7401 | -464.0 | -394.4 | |
| 0.00 | 1.53 | 0.00 | 1.13 | -26.43 | 185.68 | -43.67 | 123.78 | 0.7463 | -656.0 | -534.2 | |
| 0.00 | 0.90 | 0.00 | 0.70 | -29.24 | 183.86 | -45.49 | 126.40 | 0.7753 | -502.0 | -443.7 | |
| 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. | |