SDO HMI 2011-10-21 19:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 117.83 | 474.10 | 65.10 | 262.77 | -21.14 | 334.29 | -1.49 | 177.03 | 0.4498 | -89.0 | -124.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.22 | 0.00 | 0.68 | -21.40 | 338.02 | 2.24 | 184.62 | 0.4538 | 825.0 | 624.8 | |
| 9.40 | 37.93 | 5.16 | 20.82 | -20.13 | 337.55 | 1.78 | 183.87 | 0.4334 | 1098.8 | 524.9 | |
| 1.74 | 29.67 | 0.95 | 16.19 | -19.27 | 337.51 | 1.74 | 183.92 | 0.4198 | 995.1 | 787.1 | |
| 2.44 | -3.00 | 1.33 | -3.00 | -19.50 | 337.45 | 1.67 | 183.75 | 0.4234 | 816.0 | 999999 | |
| 1.74 | -3.00 | 0.95 | -3.00 | -19.37 | 337.26 | 1.48 | 183.34 | 0.4211 | 1081.2 | 999999 | |
| 1.39 | -2.00 | 0.76 | -2.00 | -19.97 | 337.20 | 1.43 | 183.13 | 0.4305 | 892.2 | 999999 | |
| 1.83 | -3.00 | 1.00 | -3.00 | -19.50 | 337.13 | 1.36 | 183.04 | 0.4231 | 1159.5 | 999999 | |
| 1.31 | -3.00 | 0.71 | -3.00 | -19.24 | 337.13 | 1.36 | 183.07 | 0.4189 | 1103.4 | 999999 | |
| 15.49 | 29.15 | 8.53 | 16.06 | -20.56 | 336.98 | 1.21 | 182.58 | 0.4397 | 832.8 | 428.2 | |
| 3.31 | -3.00 | 1.81 | -3.00 | -19.60 | 336.91 | 1.14 | 182.54 | 0.4245 | 883.9 | 999999 | |
| 6.26 | 14.18 | 3.41 | 7.73 | -19.21 | 336.82 | 1.04 | 182.36 | 0.4182 | 1127.9 | 733.8 | |
| 0.00 | 1.31 | 0.00 | 0.72 | -20.86 | 336.64 | 0.86 | 181.82 | 0.4442 | 601.0 | 416.5 | |
| 0.00 | 2.26 | 0.00 | 1.23 | -18.78 | 336.53 | 0.75 | 181.74 | 0.4112 | 1066.0 | 874.2 | |
| 0.00 | 0.96 | 0.00 | 0.53 | -20.13 | 336.35 | 0.57 | 181.24 | 0.4325 | 626.0 | 520.5 | |
| 3.13 | 18.01 | 1.70 | 9.78 | -18.78 | 336.25 | 0.47 | 181.09 | 0.4111 | 1107.9 | 898.3 | |
| 0.00 | 0.87 | 0.00 | 0.47 | -19.24 | 335.93 | 0.16 | 180.35 | 0.4183 | 630.0 | 401.6 | |
| 3.57 | 3.83 | 1.94 | 2.08 | -18.94 | 335.46 | -0.32 | 179.27 | 0.4136 | 909.7 | 741.7 | |
| 0.00 | 1.65 | 0.00 | 0.90 | -19.37 | 335.27 | -0.51 | 178.85 | 0.4205 | 785.0 | 621.7 | |
| 0.00 | 1.31 | 0.00 | 0.72 | -20.00 | 335.11 | -0.67 | 178.53 | 0.4305 | -403.0 | -389.3 | |
| 0.00 | 1.13 | 0.00 | 0.62 | -20.23 | 334.88 | -0.89 | 178.06 | 0.4343 | 817.0 | 590.3 | |
| 0.00 | 1.22 | 0.00 | 0.67 | -20.46 | 334.72 | -1.05 | 177.74 | 0.4380 | 691.0 | 582.1 | |
| 2.87 | 3.83 | 1.57 | 2.09 | -19.67 | 334.70 | -1.08 | 177.60 | 0.4255 | 862.4 | 683.7 | |
| 2.96 | 3.65 | 1.61 | 1.99 | -19.04 | 334.51 | -1.26 | 177.11 | 0.4157 | 877.2 | 565.8 | |
| 1.48 | 26.54 | 0.83 | 14.82 | -22.30 | 334.45 | -1.32 | 177.36 | 0.4669 | -614.2 | -439.1 | |
| 4.70 | -24.00 | 2.62 | -24.00 | -22.13 | 334.16 | -1.61 | 176.77 | 0.4645 | -1016.2 | 999999 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -21.03 | 333.86 | -1.92 | 175.98 | 0.4477 | -380.0 | -311.8 | |
| 0.00 | 1.39 | 0.00 | 0.76 | -19.28 | 333.81 | -1.96 | 175.57 | 0.4201 | 740.0 | 605.0 | |
| 0.00 | 0.87 | 0.00 | 0.47 | -19.34 | 333.62 | -2.15 | 175.15 | 0.4214 | 621.0 | 481.7 | |
| 0.00 | 3.22 | 0.00 | 1.76 | -19.64 | 333.52 | -2.25 | 175.00 | 0.4262 | 668.0 | 505.4 | |
| 1.13 | 278.07 | 0.63 | 155.16 | -22.27 | 333.42 | -2.36 | 175.31 | 0.4675 | -699.3 | -409.7 | |
| 1.22 | 6.96 | 0.67 | 3.84 | -20.80 | 333.38 | -2.40 | 174.94 | 0.4446 | -899.1 | -351.3 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -20.30 | 333.10 | -2.68 | 174.23 | 0.4373 | -758.0 | -586.2 | |
| 51.86 | -30.00 | 28.92 | -30.00 | -21.84 | 332.98 | -2.80 | 174.34 | 0.4614 | -1324.3 | 999999 | |
| 0.00 | 2.26 | 0.00 | 1.24 | -19.81 | 332.89 | -2.89 | 173.64 | 0.4299 | -792.0 | -629.8 | |
| 0.00 | 0.96 | 0.00 | 0.53 | -20.57 | 332.65 | -3.13 | 173.34 | 0.4422 | -752.0 | -630.1 | |
| 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. | |