SDO HMI 2011-11-13 09:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.66 | 151.69 | 28.13 | 173.35 | -18.89 | 336.58 | -61.41 | 112.75 | 0.8984 | 391.8 | 183.5 | |
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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 | 1.20 | 0.00 | 1.08 | -18.49 | 344.93 | -53.06 | 114.61 | 0.8359 | 486.0 | 476.1 | |
| 0.00 | 0.86 | 0.00 | 0.80 | -20.02 | 344.15 | -53.84 | 116.10 | 0.8469 | 516.0 | 454.9 | |
| 0.00 | 0.69 | 0.00 | 0.68 | -20.76 | 342.16 | -55.84 | 116.28 | 0.8650 | 496.0 | 480.9 | |
| 19.36 | 123.74 | 20.20 | 129.16 | -17.78 | 339.10 | -58.90 | 112.11 | 0.8821 | 660.7 | 204.0 | |
| 0.00 | 3.01 | 0.00 | 3.38 | -18.02 | 336.82 | -61.18 | 111.81 | 0.8992 | 420.0 | 320.6 | |
| 0.00 | 3.61 | 0.00 | 4.07 | -17.43 | 336.65 | -61.35 | 111.13 | 0.8995 | 468.0 | 315.0 | |
| 0.00 | 0.77 | 0.00 | 0.94 | -19.41 | 334.83 | -63.17 | 112.86 | 0.9150 | 287.0 | 311.4 | |
| 0.00 | 1.03 | 0.00 | 1.55 | -22.22 | 330.22 | -67.77 | 114.82 | 0.9456 | -300.0 | -309.9 | |
| 0.00 | 1.29 | 0.00 | 1.98 | -22.50 | 329.85 | -68.15 | 115.04 | 0.9479 | -330.0 | -256.7 | |
| 1.89 | 2.75 | 3.76 | 5.45 | -24.50 | 325.42 | -72.57 | 116.28 | 0.9694 | 197.9 | -4.6 | |
| 0.43 | -10.00 | 0.84 | -10.00 | -24.43 | 325.53 | -72.47 | 116.23 | 0.9689 | -54.0 | 999999 | |
| 1.98 | 3.79 | 3.33 | 6.41 | -21.92 | 327.83 | -70.17 | 114.06 | 0.9570 | -443.6 | -277.4 | |
| 0.00 | 7.57 | 0.00 | 15.10 | -23.89 | 325.21 | -72.78 | 115.62 | 0.9697 | 176.0 | 131.1 | |
| 0.00 | 1.38 | 0.00 | 2.75 | -23.53 | 325.17 | -72.82 | 115.25 | 0.9696 | 153.0 | 155.9 | |
| 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. | |