SDO HMI 2014-11-06 14:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.27 | 32.97 | 5.22 | 16.58 | 5.68 | 71.16 | 8.95 | 286.27 | 0.1602 | -192.3 | 92.6 | |
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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 |
| 2.93 | 13.12 | 1.49 | 6.67 | 5.75 | 75.30 | 13.09 | 278.92 | 0.2292 | -976.4 | -789.7 | |
| 6.13 | -1.00 | 3.12 | -1.00 | 5.60 | 75.27 | 13.06 | 278.30 | 0.2283 | -1130.6 | 999999 | |
| 1.21 | 2.59 | 0.61 | 1.31 | 5.40 | 74.47 | 12.26 | 277.86 | 0.2143 | -1135.0 | -896.8 | |
| 0.00 | 1.47 | 0.00 | 0.74 | 5.19 | 74.40 | 12.19 | 276.93 | 0.2128 | -908.0 | -713.8 | |
| 0.00 | 1.38 | 0.00 | 0.69 | 5.34 | 70.13 | 7.92 | 281.21 | 0.1405 | -828.0 | -644.9 | |
| 0.00 | 1.38 | 0.00 | 0.69 | 6.20 | 69.76 | 7.54 | 287.94 | 0.1378 | -785.0 | -572.8 | |
| 0.00 | 3.54 | 0.00 | 1.76 | 5.57 | 67.10 | 4.89 | 290.00 | 0.0907 | 882.0 | 745.4 | |
| 0.00 | 1.12 | 0.00 | 0.56 | 5.52 | 66.57 | 4.35 | 291.57 | 0.0816 | 959.0 | 746.8 | |
| 0.00 | 3.11 | 0.00 | 1.54 | 6.23 | 66.51 | 4.30 | 299.59 | 0.0861 | 1044.0 | 789.4 | |
| 0.00 | 1.38 | 0.00 | 0.69 | 6.50 | 65.98 | 3.76 | 305.78 | 0.0807 | 991.0 | 802.9 | |
| 0.00 | 1.12 | 0.00 | 0.56 | 6.68 | 65.83 | 3.61 | 308.67 | 0.0806 | 797.0 | 670.8 | |
| 0.00 | 2.76 | 0.00 | 1.37 | 5.02 | 64.50 | 2.29 | 297.95 | 0.0452 | 788.0 | 590.2 | |
| 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. | |