SDO HMI 2013-08-23 05:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.35 | 283.61 | 27.98 | 160.71 | -7.12 | 139.44 | 25.48 | 241.49 | 0.4880 | 857.3 | 363.4 | |
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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 | 1.17 | 0.00 | 0.67 | -5.76 | 140.94 | 26.97 | 245.30 | 0.4987 | -659.0 | -470.1 | |
| 48.54 | 265.52 | 27.52 | 150.45 | -6.93 | 139.57 | 25.61 | 241.94 | 0.4881 | 1320.8 | 406.8 | |
| 0.00 | 2.16 | 0.00 | 1.24 | -9.31 | 139.53 | 25.56 | 237.72 | 0.5056 | 603.0 | 526.4 | |
| 0.81 | -2.00 | 0.46 | -2.00 | -7.42 | 139.30 | 25.33 | 240.79 | 0.4880 | 774.7 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -9.39 | 139.16 | 25.19 | 237.21 | 0.5016 | 693.0 | 491.4 | |
| 0.00 | 1.35 | 0.00 | 0.77 | -9.52 | 138.76 | 24.80 | 236.56 | 0.4977 | 759.0 | 634.2 | |
| 0.00 | 2.34 | 0.00 | 1.39 | -15.92 | 138.60 | 24.63 | 226.64 | 0.5534 | -398.0 | -414.5 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -13.31 | 137.95 | 23.98 | 229.60 | 0.5215 | -747.0 | -569.3 | |
| 0.00 | 1.98 | 0.00 | 1.14 | -13.48 | 137.53 | 23.56 | 228.84 | 0.5183 | -519.0 | -499.7 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -7.26 | 136.94 | 22.97 | 238.57 | 0.4556 | 832.0 | 678.1 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -7.06 | 136.04 | 22.07 | 237.90 | 0.4420 | -753.0 | -660.1 | |
| 0.00 | 1.35 | 0.00 | 0.76 | -10.29 | 135.87 | 21.90 | 231.84 | 0.4687 | -545.0 | -447.3 | |
| 0.00 | 1.89 | 0.00 | 1.03 | -5.57 | 135.45 | 21.48 | 240.16 | 0.4219 | -757.0 | -595.3 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -3.65 | 134.83 | 20.86 | 243.57 | 0.3986 | -855.0 | -716.0 | |
| 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. | |