SDO HMI 2014-06-06 01:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.42 | 259.38 | 22.50 | 131.37 | -4.18 | 302.28 | 11.19 | 249.57 | 0.2077 | 853.7 | 455.5 | |
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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 |
| 0.00 | 1.18 | 0.00 | 0.60 | -4.98 | 304.26 | 13.18 | 249.41 | 0.2437 | 855.0 | 621.2 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -5.34 | 303.39 | 12.31 | 246.64 | 0.2322 | 964.0 | 801.4 | |
| 36.19 | 218.12 | 18.33 | 110.50 | -4.00 | 302.50 | 11.41 | 250.92 | 0.2098 | 1368.9 | 465.3 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 0.78 | 302.32 | 11.24 | 274.42 | 0.1963 | 790.0 | 568.6 | |
| 8.23 | 16.92 | 4.17 | 8.58 | -5.56 | 301.99 | 10.91 | 243.15 | 0.2120 | 1113.0 | 689.2 | |
| 0.00 | 5.16 | 0.00 | 2.61 | -5.80 | 301.50 | 10.41 | 241.03 | 0.2065 | 1107.0 | 879.7 | |
| 0.00 | 6.15 | 0.00 | 3.11 | -4.55 | 301.32 | 10.24 | 246.30 | 0.1944 | 19.0 | 483.8 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -4.73 | 301.02 | 9.93 | 244.77 | 0.1909 | 535.0 | 426.0 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -5.19 | 300.40 | 9.32 | 241.13 | 0.1850 | -653.0 | -483.5 | |
| 0.00 | 1.18 | 0.00 | 0.59 | -5.58 | 299.51 | 8.43 | 236.70 | 0.1753 | -740.0 | -514.0 | |
| 0.00 | 1.45 | 0.00 | 0.73 | -3.81 | 298.85 | 7.76 | 244.25 | 0.1503 | 960.0 | 727.8 | |
| 0.00 | 1.18 | 0.00 | 0.59 | -7.54 | 297.59 | 6.51 | 220.90 | 0.1724 | -971.0 | -839.9 | |
| 0.00 | 1.90 | 0.00 | 0.95 | -3.48 | 297.40 | 6.32 | 241.70 | 0.1253 | -874.0 | -683.7 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -6.68 | 296.72 | 5.64 | 220.34 | 0.1514 | -779.0 | -641.1 | |
| 0.00 | 0.90 | 0.00 | 0.45 | -4.66 | 293.34 | 2.25 | 206.18 | 0.0893 | -641.0 | -532.3 | |
| 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. | |