SDO HMI 2014-09-27 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 |
| 57.46 | 222.38 | 57.16 | 215.19 | 12.41 | 169.37 | -59.92 | 79.61 | 0.8602 | -123.4 | -12.2 | |
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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 | 1.76 | 0.00 | 1.55 | 11.25 | 173.12 | -56.16 | 81.04 | 0.8269 | -410.0 | -302.0 | |
| 5.12 | 23.92 | 4.61 | 21.49 | 12.45 | 172.01 | -57.28 | 79.58 | 0.8374 | -787.9 | -423.0 | |
| 0.00 | 2.82 | 0.00 | 2.59 | 12.97 | 171.36 | -57.92 | 78.97 | 0.8434 | -495.0 | -392.5 | |
| 4.06 | 28.68 | 3.73 | 26.58 | 12.50 | 171.24 | -58.05 | 79.53 | 0.8445 | -543.8 | 42.4 | |
| 18.18 | 64.07 | 16.67 | 58.66 | 11.87 | 171.34 | -57.95 | 80.28 | 0.8436 | -671.4 | -282.6 | |
| 0.00 | 1.32 | 0.00 | 1.20 | 10.21 | 171.79 | -57.49 | 82.27 | 0.8397 | -604.0 | -499.7 | |
| 3.09 | -4.00 | 2.86 | -4.00 | 12.47 | 170.95 | -58.33 | 79.56 | 0.8471 | -373.3 | 999999 | |
| 0.00 | 1.32 | 0.00 | 1.21 | 9.73 | 171.64 | -57.65 | 82.82 | 0.8413 | -300.0 | -322.6 | |
| 0.00 | 0.62 | 0.00 | 0.59 | 13.65 | 169.59 | -59.69 | 78.17 | 0.8592 | -332.0 | -323.6 | |
| 0.35 | 10.15 | 0.34 | 9.73 | 12.91 | 169.83 | -59.46 | 79.04 | 0.8571 | -332.5 | -145.6 | |
| 0.00 | 1.76 | 0.00 | 1.75 | 13.56 | 168.63 | -60.65 | 78.28 | 0.8674 | 92.0 | 173.9 | |
| 8.12 | 34.42 | 8.09 | 34.04 | 12.98 | 168.36 | -60.92 | 78.95 | 0.8697 | 701.9 | 496.0 | |
| 11.21 | 39.45 | 11.53 | 40.55 | 12.56 | 167.30 | -61.98 | 79.41 | 0.8786 | 554.1 | 263.1 | |
| 2.56 | 5.38 | 3.05 | 6.41 | 12.99 | 162.96 | -66.33 | 78.82 | 0.9114 | -455.1 | -286.9 | |
| 4.77 | 6.71 | 6.28 | 8.84 | 12.10 | 160.41 | -68.87 | 79.69 | 0.9286 | 289.9 | 163.1 | |
| 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. | |