SDO HMI 2011-10-22 17:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.68 | 428.97 | 104.17 | 790.31 | 7.78 | 249.02 | -74.68 | 83.41 | 0.9592 | -259.5 | -49.8 | |
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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 | 0.87 | 0.00 | 1.13 | 10.92 | 255.58 | -68.11 | 80.35 | 0.9258 | -328.0 | -219.7 | |
| 25.91 | 266.70 | 34.79 | 368.39 | 6.25 | 254.98 | -68.72 | 85.37 | 0.9309 | -809.2 | -162.2 | |
| 14.52 | -2.00 | 20.33 | -2.00 | 6.14 | 254.07 | -69.63 | 85.43 | 0.9366 | -356.2 | 999999 | |
| 0.78 | -2.00 | 1.10 | -2.00 | 5.62 | 253.95 | -69.74 | 85.97 | 0.9375 | -243.9 | 999999 | |
| 0.00 | 0.70 | 0.00 | 1.10 | 11.14 | 251.37 | -72.33 | 80.00 | 0.9507 | -85.0 | -30.4 | |
| 1.74 | -2.00 | 2.52 | -2.00 | 5.96 | 253.32 | -70.37 | 85.58 | 0.9411 | 202.2 | 999999 | |
| 0.00 | 0.70 | 0.00 | 1.51 | 10.32 | 246.25 | -77.44 | 80.62 | 0.9743 | 369.0 | 385.0 | |
| 1.83 | 5.30 | 3.57 | 10.35 | 6.66 | 247.92 | -75.77 | 84.49 | 0.9684 | 363.5 | 399.4 | |
| 0.00 | 0.96 | 0.00 | 1.89 | 6.79 | 247.73 | -75.96 | 84.34 | 0.9692 | 620.0 | 485.5 | |
| 4.43 | 142.70 | 10.89 | 380.81 | 10.27 | 244.62 | -79.07 | 80.58 | 0.9803 | 407.5 | 11.4 | |
| 2.87 | -10.00 | 7.02 | -10.00 | 9.82 | 244.71 | -78.98 | 81.04 | 0.9800 | 369.6 | 999999 | |
| 2.43 | -10.00 | 6.29 | -10.00 | 9.51 | 243.99 | -79.70 | 81.31 | 0.9825 | 316.3 | 999999 | |
| 0.00 | 11.04 | 0.00 | 25.13 | 6.50 | 245.85 | -77.84 | 84.51 | 0.9768 | 487.0 | 328.8 | |
| 1.65 | -10.00 | 4.48 | -10.00 | 8.93 | 243.64 | -80.05 | 81.88 | 0.9837 | 157.7 | 999999 | |
| 4.52 | -10.00 | 13.18 | -10.00 | 8.59 | 242.84 | -80.85 | 82.17 | 0.9862 | -399.8 | 999999 | |
| 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. | |