SDO HMI 2014-10-08 04:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.03 | 0.00 | 8.58 | 11.10 | 97.37 | 7.21 | 283.26 | 0.1678 | -559.4 | -518.4 | |
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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 | 1.93 | 0.00 | 0.98 | 8.56 | 102.53 | 12.36 | 280.97 | 0.2167 | -714.0 | -547.4 | |
| 0.00 | 0.70 | 0.00 | 0.36 | 10.09 | 102.43 | 12.27 | 287.94 | 0.2208 | -828.0 | -649.6 | |
| 0.00 | 2.63 | 0.00 | 1.33 | 9.96 | 100.01 | 9.84 | 290.99 | 0.1812 | -843.0 | -744.6 | |
| 0.00 | 2.11 | 0.00 | 1.06 | 13.04 | 99.68 | 9.52 | 306.20 | 0.2006 | -768.0 | -467.9 | |
| 0.00 | 1.67 | 0.00 | 0.84 | 10.51 | 99.41 | 9.24 | 295.12 | 0.1752 | -947.0 | -708.1 | |
| 0.00 | 1.58 | 0.00 | 0.79 | 10.58 | 99.10 | 8.94 | 296.18 | 0.1709 | -995.0 | -756.9 | |
| 0.00 | 1.67 | 0.00 | 0.84 | 11.79 | 96.67 | 6.51 | 310.74 | 0.1470 | -1004.0 | -758.4 | |
| 0.00 | 0.70 | 0.00 | 0.35 | 10.92 | 93.56 | 3.39 | 323.98 | 0.0992 | -474.0 | -460.4 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 16.91 | 93.40 | 3.24 | 343.58 | 0.1921 | 821.0 | 552.8 | |
| 0.00 | 0.53 | 0.00 | 0.27 | 17.43 | 92.41 | 2.24 | 349.02 | 0.1968 | 824.0 | 602.7 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 8.23 | 92.13 | 1.97 | 314.06 | 0.0475 | -908.0 | -676.2 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 9.22 | 86.10 | -4.07 | 54.32 | 0.0866 | -877.0 | -580.8 | |
| 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. | |