SDO HMI 2011-11-20 04:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.11 | 232.64 | 39.84 | 210.81 | 14.12 | 252.15 | -56.30 | 74.59 | 0.8391 | -494.4 | -167.5 | |
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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 |
| 35.96 | 216.43 | 32.32 | 195.23 | 14.19 | 252.42 | -56.03 | 74.48 | 0.8367 | -809.2 | -204.8 | |
| 0.94 | -1.00 | 0.86 | -1.00 | 14.60 | 251.87 | -56.58 | 74.06 | 0.8421 | -456.9 | 999999 | |
| 1.89 | -1.00 | 1.73 | -1.00 | 13.74 | 251.70 | -56.75 | 75.10 | 0.8428 | 505.0 | 999999 | |
| 1.89 | -1.00 | 1.72 | -1.00 | 13.47 | 251.74 | -56.71 | 75.42 | 0.8421 | -341.0 | 999999 | |
| 0.77 | -1.00 | 0.71 | -1.00 | 14.06 | 251.35 | -57.10 | 74.77 | 0.8463 | -87.8 | 999999 | |
| 2.15 | 2.75 | 2.01 | 2.58 | 14.65 | 250.82 | -57.63 | 74.14 | 0.8516 | -348.4 | -256.2 | |
| 0.00 | 1.03 | 0.00 | 0.97 | 14.28 | 250.69 | -57.76 | 74.59 | 0.8524 | -232.0 | -166.3 | |
| 0.51 | 2.40 | 0.49 | 2.27 | 14.49 | 250.54 | -57.91 | 74.36 | 0.8539 | -137.5 | -41.9 | |
| 0.00 | 0.77 | 0.00 | 0.73 | 14.04 | 250.73 | -57.72 | 74.87 | 0.8518 | 370.0 | 390.8 | |
| 0.00 | 1.80 | 0.00 | 1.70 | 13.15 | 250.55 | -57.90 | 75.93 | 0.8525 | 682.0 | 536.9 | |
| 0.00 | 1.63 | 0.00 | 1.56 | 13.81 | 250.06 | -58.38 | 75.22 | 0.8574 | 342.0 | 357.1 | |
| 0.00 | 2.23 | 0.00 | 2.16 | 14.49 | 249.66 | -58.79 | 74.47 | 0.8615 | 475.0 | 413.6 | |
| 0.00 | 1.46 | 0.00 | 1.50 | 15.68 | 247.75 | -60.70 | 73.33 | 0.8784 | 496.0 | 382.2 | |
| 0.00 | 0.94 | 0.00 | 0.92 | 10.00 | 249.16 | -59.29 | 79.73 | 0.8626 | 556.0 | 457.2 | |
| 0.00 | 1.20 | 0.00 | 1.19 | 11.30 | 248.50 | -59.95 | 78.27 | 0.8690 | 391.0 | 370.3 | |
| 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. | |