SDO HMI 2013-08-21 10:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.44 | 342.49 | 26.25 | 174.83 | -6.92 | 139.27 | 1.61 | 186.67 | 0.2418 | 837.2 | 370.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.36 | 2.16 | 0.19 | 1.12 | -9.04 | 143.12 | 5.46 | 198.92 | 0.2912 | 949.5 | 820.5 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -9.05 | 141.09 | 3.43 | 192.13 | 0.2823 | 892.0 | 730.1 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -5.42 | 140.97 | 3.31 | 195.09 | 0.2220 | 765.0 | 546.2 | |
| 0.00 | 4.14 | 0.00 | 2.14 | -10.03 | 140.35 | 2.70 | 189.04 | 0.2961 | -807.0 | -719.2 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -4.80 | 140.33 | 2.67 | 192.90 | 0.2090 | -865.0 | -613.3 | |
| 50.18 | 317.20 | 25.60 | 161.80 | -6.75 | 139.33 | 1.67 | 186.99 | 0.2389 | 1431.5 | 421.4 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -14.87 | 138.64 | 0.98 | 182.56 | 0.3731 | -938.0 | -844.5 | |
| 0.00 | 2.16 | 0.00 | 1.14 | -13.96 | 137.58 | -0.08 | 179.78 | 0.3578 | -791.0 | -710.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -9.10 | 137.49 | -0.17 | 179.41 | 0.2770 | -834.0 | -665.6 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -14.61 | 137.42 | -0.24 | 179.37 | 0.3684 | -914.0 | -733.2 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -13.54 | 137.33 | -0.33 | 179.08 | 0.3509 | -1036.0 | -874.9 | |
| 0.90 | 5.76 | 0.46 | 2.94 | -7.40 | 136.85 | -0.80 | 176.77 | 0.2487 | 995.6 | 701.6 | |
| 0.00 | 2.07 | 0.00 | 1.05 | -5.41 | 135.12 | -2.54 | 168.33 | 0.2187 | -905.0 | -731.7 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -4.60 | 134.85 | -2.81 | 166.25 | 0.2063 | -937.0 | -667.6 | |
| 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. | |