SDO HMI 2011-10-22 09:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 104.79 | 473.51 | 58.22 | 263.79 | -21.12 | 333.83 | 5.74 | 191.94 | 0.4576 | -142.3 | -163.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.62 | 33.60 | 4.79 | 18.72 | -20.02 | 337.69 | 9.60 | 200.16 | 0.4564 | 1033.9 | 297.6 | |
| 4.35 | 29.33 | 2.40 | 16.22 | -19.26 | 337.54 | 9.46 | 200.51 | 0.4445 | 1158.2 | 798.4 | |
| 7.31 | -2.00 | 4.05 | -2.00 | -19.53 | 337.50 | 9.41 | 200.20 | 0.4481 | 939.1 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -19.89 | 337.39 | 9.30 | 199.70 | 0.4528 | 974.0 | 904.8 | |
| 5.31 | 14.19 | 2.95 | 7.88 | -20.15 | 337.21 | 9.12 | 199.15 | 0.4557 | 952.7 | 642.2 | |
| 0.00 | 3.13 | 0.00 | 1.75 | -20.54 | 337.07 | 8.98 | 198.58 | 0.4608 | 588.0 | 580.4 | |
| 0.00 | 3.05 | 0.00 | 1.68 | -19.35 | 336.81 | 8.72 | 198.98 | 0.4419 | 732.0 | 527.0 | |
| 0.96 | 3.83 | 0.52 | 2.10 | -18.53 | 336.74 | 8.65 | 199.48 | 0.4294 | 791.6 | 700.1 | |
| 0.00 | 1.57 | 0.00 | 0.87 | -20.44 | 336.84 | 8.75 | 198.21 | 0.4581 | 453.0 | 469.2 | |
| 0.00 | 1.31 | 0.00 | 0.73 | -20.24 | 336.80 | 8.71 | 198.27 | 0.4550 | 564.0 | 491.5 | |
| 0.00 | 1.31 | 0.00 | 0.72 | -19.61 | 336.67 | 8.58 | 198.48 | 0.4451 | 796.0 | 612.2 | |
| 0.00 | 1.57 | 0.00 | 0.88 | -21.00 | 336.71 | 8.62 | 197.56 | 0.4658 | 681.0 | 521.2 | |
| 1.22 | 1.91 | 0.67 | 1.05 | -18.59 | 336.52 | 8.43 | 198.97 | 0.4292 | 1032.7 | 820.0 | |
| 0.00 | 3.22 | 0.00 | 1.78 | -19.87 | 336.52 | 8.43 | 198.00 | 0.4482 | 557.0 | 567.0 | |
| 0.00 | 5.31 | 0.00 | 2.93 | -19.41 | 336.50 | 8.41 | 198.29 | 0.4413 | 936.0 | 678.4 | |
| 1.13 | 2.52 | 0.62 | 1.39 | -19.05 | 336.35 | 8.26 | 198.27 | 0.4351 | 853.9 | 788.7 | |
| 6.44 | 6.53 | 3.53 | 3.58 | -18.72 | 336.30 | 8.21 | 198.42 | 0.4300 | 981.1 | 973.0 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -20.77 | 336.34 | 8.26 | 197.02 | 0.4606 | 446.0 | 439.1 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -19.57 | 336.22 | 8.13 | 197.60 | 0.4423 | 475.0 | 342.9 | |
| 0.00 | 2.87 | 0.00 | 1.58 | -18.95 | 336.03 | 7.94 | 197.67 | 0.4320 | 603.0 | 615.4 | |
| 1.83 | 3.13 | 1.00 | 1.71 | -18.71 | 335.03 | 6.94 | 195.73 | 0.4239 | 895.0 | 455.3 | |
| 4.35 | 11.75 | 2.38 | 6.43 | -19.10 | 334.86 | 6.77 | 195.10 | 0.4291 | 879.2 | 801.9 | |
| 2.00 | 4.96 | 1.10 | 2.73 | -19.58 | 334.46 | 6.37 | 193.97 | 0.4350 | 767.6 | 524.7 | |
| 0.00 | 0.96 | 0.00 | 0.52 | -19.06 | 334.15 | 6.07 | 193.63 | 0.4257 | 667.0 | 585.3 | |
| 0.00 | 2.18 | 0.00 | 1.20 | -19.81 | 334.02 | 5.93 | 192.92 | 0.4368 | 772.0 | 421.1 | |
| 1.39 | 13.06 | 0.78 | 7.34 | -22.31 | 334.06 | 5.97 | 191.74 | 0.4749 | -798.4 | -620.4 | |
| 0.00 | 1.04 | 0.00 | 0.57 | -19.22 | 333.94 | 5.85 | 193.07 | 0.4274 | 747.0 | 589.6 | |
| 0.00 | 2.52 | 0.00 | 1.41 | -21.74 | 333.78 | 5.69 | 191.46 | 0.4654 | -829.0 | -648.2 | |
| 0.00 | 1.57 | 0.00 | 0.87 | -21.30 | 333.63 | 5.54 | 191.37 | 0.4583 | -232.0 | -213.3 | |
| 2.26 | 8.53 | 1.27 | 4.79 | -22.37 | 333.54 | 5.46 | 190.73 | 0.4743 | -810.4 | -754.8 | |
| 0.00 | 1.04 | 0.00 | 0.58 | -20.76 | 333.39 | 5.30 | 191.12 | 0.4494 | -684.0 | -514.3 | |
| 1.48 | 301.69 | 0.82 | 168.54 | -20.33 | 332.83 | 4.74 | 190.16 | 0.4411 | -858.3 | -410.1 | |
| 5.48 | -32.00 | 3.03 | -32.00 | -20.69 | 332.74 | 4.66 | 189.83 | 0.4464 | -1107.8 | 999999 | |
| 1.83 | -32.00 | 1.02 | -32.00 | -21.19 | 332.76 | 4.67 | 189.66 | 0.4542 | -930.0 | 999999 | |
| 0.52 | -32.00 | 0.29 | -32.00 | -20.62 | 332.49 | 4.40 | 189.33 | 0.4447 | -1021.0 | 999999 | |
| 0.00 | 1.13 | 0.00 | 0.62 | -20.26 | 332.44 | 4.36 | 189.38 | 0.4390 | -864.0 | -684.7 | |
| 48.31 | -32.00 | 27.00 | -32.00 | -21.96 | 332.43 | 4.34 | 188.72 | 0.4651 | -1245.9 | 999999 | |
| 0.00 | 1.39 | 0.00 | 0.77 | -20.26 | 332.22 | 4.13 | 188.91 | 0.4384 | 162.0 | 166.4 | |
| 0.00 | 0.87 | 0.00 | 0.50 | -24.40 | 332.02 | 3.93 | 187.18 | 0.5013 | -614.0 | -430.2 | |
| 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. | |