SDO HMI 2011-11-20 07:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.24 | 233.06 | 37.40 | 202.16 | 14.12 | 252.21 | -54.60 | 74.34 | 0.8232 | -515.1 | -211.6 | |
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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 | 2.06 | 0.00 | 1.73 | 15.73 | 253.82 | -52.99 | 72.11 | 0.8099 | 416.0 | 250.1 | |
| 0.00 | 0.86 | 0.00 | 0.74 | 15.38 | 252.49 | -54.32 | 72.77 | 0.8222 | -347.0 | -337.1 | |
| 37.67 | 217.01 | 32.50 | 187.71 | 14.22 | 252.44 | -54.37 | 74.18 | 0.8211 | -818.2 | -243.9 | |
| 2.40 | -3.00 | 2.10 | -3.00 | 13.44 | 251.76 | -55.05 | 75.22 | 0.8267 | -404.6 | 999999 | |
| 1.37 | -3.00 | 1.21 | -3.00 | 13.92 | 251.54 | -55.27 | 74.68 | 0.8294 | 273.5 | 999999 | |
| 0.94 | -3.00 | 0.83 | -3.00 | 14.01 | 251.45 | -55.36 | 74.58 | 0.8303 | -113.7 | 999999 | |
| 0.86 | -3.00 | 0.76 | -3.00 | 14.03 | 251.22 | -55.59 | 74.59 | 0.8324 | 277.0 | 999999 | |
| 0.00 | 2.83 | 0.00 | 2.55 | 14.66 | 250.77 | -56.04 | 73.91 | 0.8374 | -463.0 | -302.3 | |
| 0.00 | 1.03 | 0.00 | 0.93 | 14.23 | 250.77 | -56.04 | 74.41 | 0.8369 | -286.0 | -209.8 | |
| 0.00 | 2.15 | 0.00 | 1.94 | 14.44 | 250.63 | -56.18 | 74.18 | 0.8384 | -215.0 | -102.3 | |
| 0.00 | 1.72 | 0.00 | 1.54 | 13.68 | 250.70 | -56.11 | 75.08 | 0.8369 | 380.0 | 400.0 | |
| 0.00 | 0.77 | 0.00 | 0.70 | 13.15 | 250.39 | -56.42 | 75.74 | 0.8392 | 595.0 | 467.7 | |
| 0.00 | 1.03 | 0.00 | 0.96 | 14.53 | 249.59 | -57.22 | 74.22 | 0.8479 | 666.0 | 552.2 | |
| 0.00 | 1.03 | 0.00 | 0.96 | 11.18 | 249.25 | -57.56 | 78.19 | 0.8479 | 468.0 | 416.2 | |
| 0.00 | 1.54 | 0.00 | 1.43 | 9.67 | 249.18 | -57.63 | 79.98 | 0.8476 | 336.0 | 343.2 | |
| 0.00 | 1.03 | 0.00 | 0.97 | 10.38 | 248.76 | -58.05 | 79.18 | 0.8519 | 514.0 | 436.2 | |
| 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. | |