SDO HMI 2014-09-26 21:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.71 | 19.33 | 0.63 | 17.93 | -14.43 | 185.16 | -54.01 | 111.96 | 0.8467 | -118.0 | -60.7 | |
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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 | 1.02 | -14.27 | 186.74 | -52.43 | 112.36 | 0.8327 | 523.0 | 441.9 | |
| 0.71 | 1.85 | 0.63 | 1.65 | -14.09 | 186.65 | -52.52 | 112.11 | 0.8329 | 563.4 | 446.1 | |
| 0.00 | 0.88 | 0.00 | 0.78 | -13.40 | 186.87 | -52.30 | 111.41 | 0.8288 | 583.0 | 468.8 | |
| 0.00 | 5.12 | 0.00 | 4.59 | -13.16 | 186.07 | -53.09 | 110.85 | 0.8353 | 484.0 | 379.3 | |
| 0.00 | 3.35 | 0.00 | 3.22 | -15.74 | 184.30 | -54.87 | 113.11 | 0.8579 | -555.0 | -451.3 | |
| 0.00 | 1.50 | 0.00 | 1.40 | -14.04 | 184.89 | -54.28 | 111.43 | 0.8482 | -518.0 | -476.9 | |
| 0.00 | 0.71 | 0.00 | 0.67 | -15.09 | 184.34 | -54.83 | 112.41 | 0.8558 | -488.0 | -532.4 | |
| 0.00 | 1.68 | 0.00 | 1.62 | -15.55 | 183.94 | -55.23 | 112.77 | 0.8603 | -359.0 | -278.6 | |
| 0.00 | 1.06 | 0.00 | 1.02 | -15.25 | 184.00 | -55.17 | 112.47 | 0.8590 | -506.0 | -495.7 | |
| 0.00 | 1.06 | 0.00 | 1.02 | -14.94 | 183.90 | -55.26 | 112.09 | 0.8589 | -485.0 | -394.0 | |
| 0.00 | 0.97 | 0.00 | 0.94 | -14.52 | 183.62 | -55.54 | 111.53 | 0.8601 | -288.0 | -244.5 | |
| 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. | |