SDO HMI 2014-06-08 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.33 | 0.00 | 8.21 | 3.32 | 256.98 | -5.44 | 97.44 | 0.1634 | 562.8 | 475.2 | |
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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 | 1.00 | 0.00 | 0.50 | 4.49 | 273.75 | 11.34 | 290.96 | 0.2109 | -881.0 | -688.6 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 5.19 | 272.99 | 10.57 | 295.54 | 0.2035 | -797.0 | -661.9 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 4.69 | 260.80 | -1.61 | 19.64 | 0.0838 | 752.0 | 521.6 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 5.34 | 258.78 | -3.63 | 35.09 | 0.1102 | 843.0 | 708.1 | |
| 0.00 | 4.35 | 0.00 | 2.16 | 0.46 | 257.18 | -5.24 | 86.97 | 0.0918 | 1039.0 | 694.7 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 10.53 | 257.07 | -5.35 | 27.04 | 0.2025 | 815.0 | 623.7 | |
| 0.00 | 1.18 | 0.00 | 0.59 | -1.76 | 256.68 | -5.73 | 108.76 | 0.1059 | 953.0 | 701.6 | |
| 0.00 | 1.09 | 0.00 | 0.55 | -0.69 | 252.85 | -9.57 | 95.24 | 0.1676 | 819.0 | 617.8 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 8.44 | 251.57 | -10.85 | 52.37 | 0.2361 | 790.0 | 556.8 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 5.43 | 250.67 | -11.75 | 65.70 | 0.2234 | 832.0 | 652.5 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 4.88 | 250.58 | -11.83 | 68.14 | 0.2211 | 744.0 | 510.9 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 1.53 | 246.10 | -16.32 | 85.19 | 0.2831 | 845.0 | 631.2 | |
| 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. | |