SDO HMI 2014-06-05 21:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.73 | 263.72 | 25.52 | 132.60 | -4.38 | 302.06 | 8.76 | 243.30 | 0.1716 | 821.9 | 446.0 | |
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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 | 1.27 | 0.00 | 0.64 | -4.91 | 304.07 | 10.77 | 245.81 | 0.2050 | 924.0 | 727.2 | |
| 0.00 | 2.98 | 0.00 | 1.51 | -6.62 | 303.45 | 10.15 | 237.07 | 0.2094 | 859.0 | 622.6 | |
| 0.00 | 2.26 | 0.00 | 1.14 | -5.34 | 303.30 | 10.00 | 242.23 | 0.1963 | 1160.0 | 933.1 | |
| 37.26 | 216.78 | 18.74 | 109.01 | -4.06 | 302.36 | 9.06 | 246.35 | 0.1722 | 1436.7 | 485.8 | |
| 11.12 | 19.44 | 5.60 | 9.79 | -5.73 | 301.85 | 8.55 | 236.50 | 0.1782 | 1105.5 | 621.8 | |
| 0.00 | 1.36 | 0.00 | 0.68 | -4.60 | 301.50 | 8.20 | 241.16 | 0.1630 | 398.0 | 338.2 | |
| 2.35 | 8.77 | 1.18 | 4.41 | -5.89 | 301.36 | 8.06 | 234.21 | 0.1727 | 1083.9 | 696.9 | |
| 0.00 | 1.81 | 0.00 | 0.91 | -9.32 | 298.16 | 4.86 | 207.62 | 0.1813 | -881.0 | -705.0 | |
| 0.00 | 1.09 | 0.00 | 0.55 | -8.46 | 297.78 | 4.48 | 208.06 | 0.1651 | -968.0 | -796.0 | |
| 0.00 | 1.27 | 0.00 | 0.63 | -3.66 | 297.41 | 4.11 | 229.22 | 0.0950 | -782.0 | -637.4 | |
| 0.00 | 2.17 | 0.00 | 1.08 | -6.37 | 297.30 | 4.00 | 212.50 | 0.1298 | -981.0 | -729.3 | |
| 0.00 | 1.36 | 0.00 | 0.67 | -3.87 | 296.99 | 3.69 | 224.43 | 0.0921 | -835.0 | -629.0 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -6.77 | 296.72 | 3.42 | 207.11 | 0.1307 | -766.0 | -603.5 | |
| 0.00 | 0.90 | 0.00 | 0.45 | -5.51 | 291.62 | -1.68 | 162.70 | 0.0989 | -857.0 | -694.7 | |
| 0.00 | 1.27 | 0.00 | 0.63 | -5.26 | 291.16 | -2.14 | 157.47 | 0.0976 | -828.0 | -538.5 | |
| 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. | |