SDO HMI 2011-10-21 23:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 119.76 | 470.44 | 66.18 | 260.66 | -21.09 | 334.23 | 0.66 | 181.51 | 0.4486 | -97.6 | -165.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.65 | 0.00 | 0.92 | -21.43 | 338.06 | 4.49 | 189.18 | 0.4583 | 787.0 | 559.6 | |
| 11.84 | 29.33 | 6.51 | 16.14 | -20.13 | 337.60 | 4.04 | 188.73 | 0.4371 | 1039.2 | 404.7 | |
| 5.92 | 46.30 | 3.24 | 25.30 | -19.43 | 337.49 | 3.92 | 188.75 | 0.4260 | 949.1 | 702.0 | |
| 1.04 | -3.00 | 0.57 | -3.00 | -19.20 | 337.30 | 3.73 | 188.40 | 0.4219 | 1096.8 | 999999 | |
| 3.13 | 3.31 | 1.72 | 1.82 | -19.96 | 337.22 | 3.65 | 187.96 | 0.4336 | 847.2 | 764.5 | |
| 3.57 | -3.00 | 1.95 | -3.00 | -19.56 | 337.15 | 3.58 | 187.94 | 0.4272 | 944.3 | 999999 | |
| 5.57 | -3.00 | 3.04 | -3.00 | -19.27 | 337.08 | 3.51 | 187.89 | 0.4224 | 1161.7 | 999999 | |
| 15.06 | 23.94 | 8.30 | 13.20 | -20.49 | 337.04 | 3.47 | 187.41 | 0.4414 | 798.6 | 476.0 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -20.72 | 336.76 | 3.19 | 186.75 | 0.4445 | 168.0 | 220.2 | |
| 0.00 | 3.22 | 0.00 | 1.76 | -19.49 | 336.73 | 3.16 | 187.05 | 0.4253 | 675.0 | 603.3 | |
| 0.00 | 1.91 | 0.00 | 1.05 | -20.05 | 336.71 | 3.14 | 186.84 | 0.4341 | 736.0 | 556.2 | |
| 0.87 | 12.88 | 0.47 | 6.99 | -18.71 | 336.62 | 3.05 | 187.05 | 0.4126 | 898.8 | 946.8 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -20.82 | 336.60 | 3.03 | 186.39 | 0.4458 | 441.0 | 344.5 | |
| 0.00 | 1.83 | 0.00 | 1.00 | -20.12 | 336.55 | 2.98 | 186.48 | 0.4348 | 671.0 | 573.2 | |
| 0.00 | 1.22 | 0.00 | 0.66 | -18.93 | 336.44 | 2.87 | 186.56 | 0.4159 | 968.0 | 822.4 | |
| 0.96 | -12.00 | 0.52 | -12.00 | -18.74 | 336.37 | 2.80 | 186.47 | 0.4127 | 956.0 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.52 | -19.13 | 336.34 | 2.78 | 186.30 | 0.4188 | 914.0 | 693.5 | |
| 0.00 | 1.31 | 0.00 | 0.71 | -19.20 | 336.12 | 2.56 | 185.79 | 0.4195 | 772.0 | 644.6 | |
| 3.05 | 3.83 | 1.65 | 2.08 | -18.77 | 335.77 | 2.20 | 185.09 | 0.4122 | 891.3 | 845.4 | |
| 0.00 | 1.13 | 0.00 | 0.62 | -18.90 | 335.52 | 1.95 | 184.48 | 0.4139 | 792.0 | 575.4 | |
| 0.00 | 1.04 | 0.00 | 0.57 | -19.39 | 335.40 | 1.83 | 184.12 | 0.4216 | 558.0 | 327.7 | |
| 0.00 | 1.22 | 0.00 | 0.68 | -22.66 | 335.34 | 1.77 | 183.48 | 0.4726 | -781.0 | -538.5 | |
| 0.00 | 1.83 | 0.00 | 1.00 | -20.18 | 335.00 | 1.43 | 183.10 | 0.4337 | 955.0 | 718.9 | |
| 2.09 | 3.22 | 1.14 | 1.75 | -18.96 | 334.73 | 1.16 | 182.67 | 0.4142 | 983.1 | 816.5 | |
| 1.39 | 3.31 | 0.76 | 1.81 | -19.65 | 334.71 | 1.14 | 182.53 | 0.4251 | 650.6 | 553.2 | |
| 0.00 | 2.09 | 0.00 | 1.17 | -22.28 | 334.47 | 0.90 | 181.79 | 0.4662 | -588.0 | -463.7 | |
| 1.04 | 2.35 | 0.57 | 1.28 | -19.45 | 334.17 | 0.60 | 181.34 | 0.4217 | 670.7 | 677.0 | |
| 5.14 | 295.76 | 2.87 | 164.89 | -22.25 | 334.05 | 0.48 | 180.96 | 0.4655 | -950.8 | -440.5 | |
| 0.00 | 4.61 | 0.00 | 2.56 | -21.58 | 333.89 | 0.32 | 180.65 | 0.4550 | -878.0 | -643.3 | |
| 0.00 | 1.04 | 0.00 | 0.58 | -21.88 | 333.82 | 0.25 | 180.51 | 0.4597 | -762.0 | -616.9 | |
| 3.92 | 8.27 | 2.14 | 4.51 | -19.45 | 333.72 | 0.15 | 180.35 | 0.4216 | 780.6 | 747.6 | |
| 1.91 | -28.00 | 1.07 | -28.00 | -22.11 | 333.50 | -0.07 | 179.86 | 0.4634 | -793.9 | 999999 | |
| 0.00 | 3.22 | 0.00 | 1.77 | -20.64 | 333.37 | -0.19 | 179.58 | 0.4404 | -705.0 | -562.1 | |
| 0.52 | -28.00 | 0.29 | -28.00 | -20.84 | 333.15 | -0.42 | 179.11 | 0.4436 | -1004.0 | 999999 | |
| 5.48 | -28.00 | 3.03 | -28.00 | -21.04 | 333.12 | -0.45 | 179.05 | 0.4467 | -1069.4 | 999999 | |
| 0.00 | 6.79 | 0.00 | 3.73 | -20.18 | 332.96 | -0.61 | 178.68 | 0.4332 | -890.0 | -701.9 | |
| 47.26 | -28.00 | 26.34 | -28.00 | -21.88 | 332.83 | -0.74 | 178.49 | 0.4599 | -1273.1 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -19.78 | 332.84 | -0.73 | 178.38 | 0.4269 | -838.0 | -698.8 | |
| 0.00 | 0.96 | 0.00 | 0.53 | -20.51 | 332.64 | -0.93 | 178.01 | 0.4385 | -835.0 | -651.1 | |
| 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. | |