SDO HMI 2014-07-09 09:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.44 | 0.00 | 10.86 | -18.19 | 230.75 | 20.85 | 221.05 | 0.5372 | -35.2 | 51.7 | |
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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 | 1.36 | 0.00 | 0.98 | -25.30 | 247.35 | 37.44 | 229.26 | 0.7277 | -629.0 | -492.1 | |
| 0.00 | 0.82 | 0.00 | 0.50 | -15.51 | 239.95 | 30.05 | 236.33 | 0.5818 | 797.0 | 686.7 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -14.05 | 236.76 | 26.86 | 235.70 | 0.5325 | 752.0 | 606.5 | |
| 0.00 | 2.27 | 0.00 | 1.34 | -16.17 | 236.62 | 26.72 | 232.28 | 0.5480 | 676.0 | 579.6 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -14.23 | 236.36 | 26.46 | 235.03 | 0.5291 | 719.0 | 506.1 | |
| 0.00 | 3.18 | 0.00 | 1.87 | -16.03 | 236.39 | 26.49 | 232.25 | 0.5442 | 755.0 | 619.6 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -14.99 | 235.02 | 25.12 | 232.43 | 0.5193 | 705.0 | 568.1 | |
| 0.00 | 1.73 | 0.00 | 0.96 | -14.11 | 230.88 | 20.98 | 228.94 | 0.4623 | -825.0 | -663.6 | |
| 0.00 | 0.64 | 0.00 | 0.35 | -14.26 | 230.42 | 20.52 | 228.07 | 0.4585 | -736.0 | -566.3 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -17.65 | 227.63 | 17.73 | 218.72 | 0.4658 | -599.0 | -519.6 | |
| 0.00 | 0.82 | 0.00 | 0.44 | -13.59 | 226.46 | 16.55 | 223.15 | 0.4066 | -750.0 | -592.7 | |
| 0.00 | 1.45 | 0.00 | 0.85 | -28.00 | 206.03 | -3.87 | 173.53 | 0.5315 | -635.0 | -570.6 | |
| 0.00 | 1.54 | 0.00 | 0.90 | -27.16 | 202.69 | -7.22 | 167.71 | 0.5273 | -688.0 | -549.7 | |
| 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. | |