SDO HMI 2011-11-10 13:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.08 | 334.77 | 25.77 | 211.00 | 27.80 | 44.61 | -30.75 | 47.06 | 0.6198 | -723.2 | -334.4 | |
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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 | 1.81 | 0.00 | 1.15 | 31.96 | 47.67 | -27.69 | 39.18 | 0.6264 | -528.0 | -395.2 | |
| 0.00 | 0.52 | 0.00 | 0.33 | 32.07 | 45.67 | -29.69 | 40.79 | 0.6448 | -670.0 | -524.8 | |
| 0.00 | 0.86 | 0.00 | 0.56 | 32.31 | 45.46 | -29.89 | 40.68 | 0.6485 | -487.0 | -470.2 | |
| 0.52 | 317.97 | 0.32 | 199.61 | 28.15 | 45.16 | -30.20 | 46.17 | 0.6170 | -942.8 | -370.6 | |
| 38.58 | -4.00 | 24.20 | -4.00 | 27.72 | 44.95 | -30.41 | 46.92 | 0.6158 | -1173.2 | 999999 | |
| 1.98 | -4.00 | 1.25 | -4.00 | 28.13 | 44.54 | -30.82 | 46.70 | 0.6231 | -706.5 | 999999 | |
| 0.00 | 1.55 | 0.00 | 1.00 | 27.57 | 42.15 | -33.21 | 49.27 | 0.6430 | -538.0 | -475.0 | |
| 0.00 | 0.86 | 0.00 | 0.58 | 26.47 | 38.38 | -36.98 | 53.22 | 0.6746 | 685.0 | 580.8 | |
| 0.00 | 1.72 | 0.00 | 1.13 | 24.87 | 38.79 | -36.56 | 55.13 | 0.6611 | 732.0 | 500.7 | |
| 0.00 | 1.81 | 0.00 | 1.21 | 26.10 | 37.98 | -37.38 | 53.95 | 0.6766 | 627.0 | 543.8 | |
| 0.00 | 1.21 | 0.00 | 0.81 | 26.41 | 37.73 | -37.62 | 53.67 | 0.6810 | 521.0 | 422.1 | |
| 0.00 | 1.98 | 0.00 | 1.33 | 26.22 | 37.68 | -37.67 | 53.96 | 0.6804 | 566.0 | 419.9 | |
| 0.00 | 0.86 | 0.00 | 0.62 | 30.32 | 35.20 | -40.16 | 50.14 | 0.7276 | 532.0 | 421.9 | |
| 0.00 | 1.29 | 0.00 | 0.95 | 30.71 | 33.90 | -41.46 | 50.36 | 0.7415 | 501.0 | 343.8 | |
| 0.00 | 2.33 | 0.00 | 1.72 | 30.36 | 33.40 | -41.96 | 51.05 | 0.7443 | 542.0 | 459.4 | |
| 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. | |