SDO HMI 2014-11-19 10:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.99 | 0.00 | 8.55 | 14.37 | 265.23 | 12.21 | 255.45 | 0.3551 | 374.5 | 309.2 | |
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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 | 1.55 | 0.00 | 0.93 | 9.12 | 287.41 | 34.39 | 282.64 | 0.5738 | 610.0 | 490.0 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 13.02 | 283.45 | 30.44 | 291.14 | 0.5313 | 401.0 | 365.2 | |
| 0.00 | 1.97 | 0.00 | 1.12 | 13.79 | 279.94 | 26.92 | 294.75 | 0.4862 | 889.0 | 621.2 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 3.43 | 267.65 | 14.63 | 274.62 | 0.2541 | 900.0 | 751.5 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 22.17 | 265.28 | 12.27 | 329.95 | 0.3946 | -810.0 | -631.2 | |
| 0.00 | 1.29 | 0.00 | 0.66 | 14.72 | 262.53 | 9.51 | 323.36 | 0.2691 | 847.0 | 720.1 | |
| 0.00 | 1.03 | 0.00 | 0.52 | 13.28 | 259.70 | 6.68 | 329.21 | 0.2223 | 709.0 | 551.9 | |
| 0.00 | 1.12 | 0.00 | 0.56 | 1.64 | 259.45 | 6.43 | 263.88 | 0.1132 | 699.0 | 487.2 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 23.19 | 258.75 | 5.73 | 345.55 | 0.3694 | -806.0 | -588.8 | |
| 0.00 | 1.29 | 0.00 | 0.66 | 15.81 | 257.49 | 4.48 | 342.15 | 0.2460 | -711.0 | -565.2 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 19.26 | 247.18 | -5.84 | 18.24 | 0.3080 | 804.0 | 602.2 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 18.14 | 246.22 | -6.80 | 22.43 | 0.2963 | 962.0 | 790.2 | |
| 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. | |