| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.40 | 196.88 | 23.41 | 113.53 | -18.71 | 338.29 | 22.13 | 224.55 | 0.5141 | 349.4 | 262.0 | |
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back to the solar disc SDO HMI 2011-11-19 14:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.67 | -17.45 | 345.01 | 28.85 | 234.04 | 0.5710 | 619.0 | 491.2 | |
| 0.00 | 4.72 | 0.00 | 2.79 | -16.61 | 343.82 | 27.66 | 234.22 | 0.5504 | 763.0 | 597.3 | |
| 0.00 | 1.63 | 0.00 | 0.96 | -16.73 | 343.56 | 27.40 | 233.79 | 0.5483 | 718.0 | 656.6 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -17.96 | 343.62 | 27.46 | 231.99 | 0.5588 | 519.0 | 492.2 | |
| 0.00 | 1.54 | 0.00 | 0.92 | -17.74 | 343.51 | 27.35 | 232.22 | 0.5558 | 875.0 | 662.1 | |
| 0.00 | 2.66 | 0.00 | 1.57 | -17.16 | 342.93 | 26.77 | 232.53 | 0.5443 | 825.0 | 640.9 | |
| 0.00 | 1.03 | 0.00 | 0.61 | -17.82 | 342.96 | 26.80 | 231.56 | 0.5502 | 728.0 | 600.2 | |
| 0.00 | 2.23 | 0.00 | 1.31 | -16.91 | 342.78 | 26.62 | 232.78 | 0.5406 | 657.0 | 449.9 | |
| 1.46 | 1.72 | 0.85 | 1.01 | -16.84 | 342.50 | 26.34 | 232.60 | 0.5366 | 767.2 | 624.7 | |
| 0.00 | 1.72 | 0.00 | 1.04 | -21.01 | 343.15 | 26.99 | 227.19 | 0.5797 | 535.0 | 503.2 | |
| 4.72 | 9.86 | 2.77 | 5.79 | -17.37 | 342.37 | 26.21 | 231.65 | 0.5396 | 809.8 | 644.6 | |
| 0.00 | 2.92 | 0.00 | 1.77 | -21.17 | 342.82 | 26.66 | 226.65 | 0.5777 | 815.0 | 669.7 | |
| 0.00 | 3.26 | 0.00 | 1.91 | -17.62 | 342.20 | 26.04 | 231.10 | 0.5398 | 830.0 | 656.1 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -15.83 | 341.80 | 25.64 | 233.50 | 0.5200 | -699.0 | -483.7 | |
| 0.00 | 1.46 | 0.00 | 0.87 | -19.30 | 342.34 | 26.18 | 228.76 | 0.5559 | 750.0 | 531.3 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -17.39 | 341.82 | 25.66 | 231.06 | 0.5334 | 708.0 | 632.1 | |
| 0.00 | 1.37 | 0.00 | 0.80 | -17.20 | 341.72 | 25.56 | 231.25 | 0.5307 | 940.0 | 844.7 | |
| 4.37 | 5.58 | 2.64 | 3.37 | -21.35 | 342.33 | 26.17 | 225.89 | 0.5742 | 751.6 | 488.7 | |
| 0.00 | 2.32 | 0.00 | 1.38 | -19.61 | 342.01 | 25.85 | 227.97 | 0.5551 | 625.0 | 553.9 | |
| 0.00 | 1.89 | 0.00 | 1.10 | -16.73 | 341.52 | 25.36 | 231.77 | 0.5242 | 686.0 | 454.1 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -18.53 | 341.72 | 25.56 | 229.25 | 0.5422 | 784.0 | 590.3 | |
| 0.00 | 2.23 | 0.00 | 1.29 | -16.53 | 341.28 | 25.12 | 231.83 | 0.5198 | 804.0 | 615.3 | |
| 6.43 | 96.67 | 3.72 | 55.57 | -17.33 | 340.37 | 24.21 | 229.58 | 0.5163 | 803.7 | 508.9 | |
| 21.19 | -23.00 | 12.18 | -23.00 | -17.26 | 339.85 | 23.69 | 229.10 | 0.5097 | 1166.5 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -15.81 | 339.33 | 23.17 | 230.81 | 0.4904 | 728.0 | 615.9 | |
| 0.00 | 0.51 | 0.00 | 0.29 | -16.02 | 338.62 | 22.46 | 229.63 | 0.4840 | -611.0 | -480.2 | |
| 0.00 | 2.66 | 0.00 | 1.49 | -16.77 | 336.91 | 20.75 | 226.22 | 0.4718 | -875.0 | -674.4 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -16.17 | 336.58 | 20.42 | 226.75 | 0.4620 | 834.0 | 631.5 | |
| 0.00 | 1.63 | 0.00 | 0.96 | -22.76 | 337.37 | 21.21 | 218.34 | 0.5400 | 670.0 | 480.1 | |
| 0.00 | 1.37 | 0.00 | 0.78 | -19.59 | 335.13 | 18.97 | 219.48 | 0.4835 | 666.0 | 594.3 | |
| 0.00 | 2.14 | 0.00 | 1.21 | -19.47 | 335.04 | 18.88 | 219.54 | 0.4813 | 799.0 | 579.4 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -22.80 | 330.82 | 14.66 | 208.83 | 0.4858 | -678.0 | -489.2 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -22.80 | 330.59 | 14.43 | 208.45 | 0.4841 | -603.0 | -512.4 | |
| 0.00 | 2.57 | 0.00 | 1.43 | -21.48 | 328.94 | 12.78 | 207.05 | 0.4546 | -575.0 | -650.1 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -21.22 | 328.85 | 12.69 | 207.17 | 0.4504 | -935.0 | -702.3 | |
| 0.00 | 1.20 | 0.00 | 0.67 | -23.07 | 328.20 | 12.04 | 204.13 | 0.4715 | -701.0 | -596.4 | |
| 0.00 | 4.12 | 0.00 | 2.32 | -23.96 | 327.92 | 11.76 | 202.83 | 0.4821 | -411.0 | -571.5 | |
| 0.00 | 4.55 | 0.00 | 2.56 | -23.60 | 327.85 | 11.69 | 203.04 | 0.4766 | -777.0 | -730.4 | |
| 0.00 | 1.54 | 0.00 | 0.87 | -23.82 | 327.64 | 11.48 | 202.46 | 0.4785 | -769.0 | -700.3 | |
| 0.00 | 1.37 | 0.00 | 0.77 | -23.99 | 327.49 | 11.33 | 202.06 | 0.4800 | -768.0 | -642.8 | |
| 0.00 | 1.20 | 0.00 | 0.67 | -23.56 | 327.36 | 11.19 | 202.19 | 0.4731 | -843.0 | -781.9 | |
| 2.23 | 3.60 | 1.25 | 2.02 | -23.65 | 327.03 | 10.87 | 201.54 | 0.4726 | -968.2 | -794.9 | |
| 0.00 | 0.94 | 0.00 | 0.55 | -26.97 | 327.31 | 11.15 | 199.41 | 0.5206 | -614.0 | -568.7 | |
| 0.00 | 1.46 | 0.00 | 0.84 | -26.87 | 327.13 | 10.97 | 199.19 | 0.5183 | -849.0 | -756.8 | |
| 0.00 | 1.80 | 0.00 | 1.01 | -23.65 | 326.84 | 10.68 | 201.19 | 0.4715 | -972.0 | -793.6 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -24.38 | 326.57 | 10.41 | 200.12 | 0.4804 | -784.0 | -669.3 | |
| 0.00 | 4.29 | 0.00 | 2.40 | -23.64 | 325.55 | 9.39 | 198.86 | 0.4646 | -634.0 | -652.9 | |
| 0.00 | 1.89 | 0.00 | 1.06 | -24.54 | 325.39 | 9.23 | 197.90 | 0.4767 | -741.0 | -573.4 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -25.23 | 324.71 | 8.55 | 196.22 | 0.4838 | -700.0 | -477.9 | |
| 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. | |