SDO HMI 2014-09-06 20:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.24 | 0.00 | 10.12 | -20.57 | 168.90 | 25.15 | 221.25 | 0.6070 | 632.2 | 498.8 | |
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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 | 1.43 | 0.00 | 0.91 | -21.52 | 171.11 | 27.36 | 222.40 | 0.6363 | 678.0 | 597.0 | |
| 0.00 | 0.98 | 0.00 | 0.63 | -21.42 | 170.65 | 26.90 | 222.04 | 0.6312 | 737.0 | 630.1 | |
| 0.00 | 1.52 | 0.00 | 0.93 | -17.82 | 169.62 | 25.87 | 225.26 | 0.5870 | 473.0 | 368.4 | |
| 0.00 | 0.45 | 0.00 | 0.28 | -21.88 | 170.27 | 26.52 | 221.13 | 0.6322 | 465.0 | 496.6 | |
| 0.00 | 0.89 | 0.00 | 0.57 | -22.01 | 170.12 | 26.36 | 220.82 | 0.6320 | 612.0 | 536.0 | |
| 0.00 | 1.70 | 0.00 | 1.08 | -21.96 | 169.96 | 26.21 | 220.71 | 0.6302 | 752.0 | 631.1 | |
| 0.00 | 0.80 | 0.00 | 0.49 | -18.13 | 169.28 | 25.53 | 224.50 | 0.5866 | 683.0 | 483.4 | |
| 0.00 | 1.96 | 0.00 | 1.20 | -19.69 | 167.87 | 24.12 | 221.00 | 0.5887 | 560.0 | 525.0 | |
| 0.00 | 1.78 | 0.00 | 1.09 | -19.85 | 167.72 | 23.97 | 220.63 | 0.5890 | 663.0 | 519.2 | |
| 0.00 | 3.84 | 0.00 | 2.43 | -23.06 | 168.00 | 24.25 | 217.39 | 0.6246 | 669.0 | 389.9 | |
| 0.00 | 0.89 | 0.00 | 0.51 | -11.57 | 166.05 | 22.29 | 229.86 | 0.4881 | 662.0 | 506.9 | |
| 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. | |