SDO HMI 2014-07-10 03:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.90 | 0.00 | 9.38 | -21.64 | 225.21 | 25.25 | 220.07 | 0.6058 | -297.5 | -267.2 | |
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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 | 0.91 | 0.00 | 0.74 | -24.53 | 245.13 | 45.18 | 234.68 | 0.7930 | -487.0 | -477.8 | |
| 0.00 | 1.00 | 0.00 | 0.80 | -25.11 | 244.26 | 44.30 | 233.57 | 0.7882 | -72.0 | -173.0 | |
| 0.00 | 0.91 | 0.00 | 0.63 | -18.28 | 239.26 | 39.30 | 238.95 | 0.7043 | 425.0 | 333.2 | |
| 0.00 | 0.91 | 0.00 | 0.60 | -14.24 | 237.71 | 37.75 | 243.45 | 0.6657 | 577.0 | 493.6 | |
| 0.00 | 1.18 | 0.00 | 0.76 | -15.97 | 234.64 | 34.68 | 239.10 | 0.6397 | 620.0 | 511.2 | |
| 0.00 | 1.09 | 0.00 | 0.69 | -16.91 | 232.90 | 32.95 | 236.55 | 0.6259 | -426.0 | -354.0 | |
| 0.00 | 0.82 | 0.00 | 0.51 | -17.28 | 230.79 | 30.83 | 234.34 | 0.6046 | -580.0 | -493.9 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -17.98 | 216.82 | 16.86 | 216.79 | 0.4625 | -167.0 | -135.5 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -22.01 | 216.37 | 16.41 | 211.16 | 0.5083 | -691.0 | -528.5 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -22.07 | 216.24 | 16.28 | 210.89 | 0.5081 | -763.0 | -642.0 | |
| 0.00 | 2.18 | 0.00 | 1.25 | -22.67 | 215.52 | 15.57 | 209.15 | 0.5103 | -598.0 | -511.7 | |
| 0.00 | 0.73 | 0.00 | 0.42 | -25.77 | 210.93 | 10.98 | 199.19 | 0.5238 | -461.0 | -481.2 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -28.62 | 205.11 | 5.15 | 188.36 | 0.5442 | -790.0 | -714.5 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -28.50 | 204.13 | 4.17 | 186.82 | 0.5406 | -752.0 | -598.1 | |
| 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. | |