SDO HMI 2014-03-06 11:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.39 | 327.06 | 27.18 | 192.29 | -25.41 | 88.60 | 27.93 | 231.89 | 0.5387 | -196.3 | -71.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.21 | 28.90 | 0.76 | 18.22 | -21.42 | 97.60 | 36.92 | 244.35 | 0.6227 | 670.8 | 659.8 | |
| 1.82 | -1.00 | 1.15 | -1.00 | -21.68 | 97.55 | 36.88 | 243.94 | 0.6231 | 785.8 | 999999 | |
| 1.30 | -1.00 | 0.82 | -1.00 | -21.35 | 97.41 | 36.74 | 244.39 | 0.6201 | 842.9 | 999999 | |
| 1.56 | -1.00 | 0.98 | -1.00 | -21.50 | 97.38 | 36.71 | 244.13 | 0.6203 | 1020.6 | 999999 | |
| 2.08 | -1.00 | 1.31 | -1.00 | -21.82 | 97.31 | 36.64 | 243.62 | 0.6207 | 833.9 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.38 | -24.58 | 96.65 | 35.98 | 239.08 | 0.6250 | -343.0 | -318.1 | |
| 0.00 | 1.64 | 0.00 | 1.04 | -24.93 | 96.73 | 36.05 | 238.61 | 0.6275 | -807.0 | -677.5 | |
| 0.00 | 1.12 | 0.00 | 0.71 | -23.77 | 96.23 | 35.55 | 240.10 | 0.6161 | 595.0 | 433.0 | |
| 0.00 | 1.56 | 0.00 | 0.97 | -23.45 | 95.37 | 34.70 | 240.15 | 0.6044 | 616.0 | 436.6 | |
| 0.00 | 1.47 | 0.00 | 0.90 | -23.02 | 94.78 | 34.10 | 240.51 | 0.5951 | 346.0 | 195.5 | |
| 0.00 | 2.42 | 0.00 | 1.49 | -23.21 | 94.79 | 34.12 | 240.22 | 0.5962 | 530.0 | 390.6 | |
| 0.00 | 2.16 | 0.00 | 1.32 | -22.48 | 94.43 | 33.76 | 241.18 | 0.5883 | 526.0 | 503.2 | |
| 0.00 | 2.34 | 0.00 | 1.42 | -22.27 | 94.30 | 33.62 | 241.44 | 0.5856 | 690.0 | 577.1 | |
| 0.00 | 2.86 | 0.00 | 1.75 | -22.92 | 94.40 | 33.72 | 240.46 | 0.5900 | 690.0 | 433.3 | |
| 1.04 | 1.90 | 0.64 | 1.18 | -24.30 | 94.76 | 34.09 | 238.49 | 0.6014 | 632.9 | 456.8 | |
| 0.35 | 2.25 | 0.21 | 1.39 | -24.09 | 94.62 | 33.95 | 238.73 | 0.5986 | 869.2 | 681.3 | |
| 0.43 | 3.37 | 0.27 | 2.07 | -23.33 | 94.36 | 33.68 | 239.79 | 0.5915 | 671.8 | 618.1 | |
| 0.00 | 1.04 | 0.00 | 0.63 | -23.05 | 94.24 | 33.57 | 240.16 | 0.5888 | 661.0 | 514.8 | |
| 0.43 | 13.76 | 0.26 | 8.38 | -22.86 | 93.92 | 33.24 | 240.29 | 0.5838 | 943.4 | 809.5 | |
| 0.00 | 1.30 | 0.00 | 0.79 | -23.26 | 93.91 | 33.24 | 239.64 | 0.5858 | 481.0 | 550.9 | |
| 0.00 | 1.56 | 0.00 | 0.94 | -22.13 | 93.57 | 32.89 | 241.27 | 0.5759 | 748.0 | 641.1 | |
| 1.12 | 2.77 | 0.68 | 1.69 | -23.21 | 93.74 | 33.07 | 239.62 | 0.5835 | 990.5 | 772.4 | |
| 0.00 | 1.82 | 0.00 | 1.11 | -23.62 | 93.78 | 33.10 | 239.00 | 0.5860 | 896.0 | 774.8 | |
| 0.00 | 1.56 | 0.00 | 0.94 | -22.18 | 93.35 | 32.67 | 241.07 | 0.5734 | 889.0 | 756.3 | |
| 0.00 | 1.21 | 0.00 | 0.74 | -23.41 | 93.64 | 32.97 | 239.26 | 0.5833 | 830.0 | 627.4 | |
| 0.61 | 19.12 | 0.37 | 11.69 | -24.22 | 93.60 | 32.93 | 237.94 | 0.5872 | 912.1 | 677.9 | |
| 0.00 | 1.04 | 0.00 | 0.63 | -23.40 | 93.25 | 32.58 | 239.04 | 0.5785 | 527.0 | 472.2 | |
| 0.00 | 1.82 | 0.00 | 1.11 | -24.46 | 93.40 | 32.72 | 237.44 | 0.5861 | 734.0 | 569.7 | |
| 0.00 | 0.26 | 0.00 | 0.16 | -27.80 | 94.27 | 33.60 | 232.93 | 0.6157 | 594.0 | 482.7 | |
| 0.00 | 0.43 | 0.00 | 0.26 | -22.20 | 92.52 | 31.84 | 240.56 | 0.5631 | 156.0 | 220.4 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -21.44 | 91.84 | 31.17 | 241.44 | 0.5506 | 641.0 | 458.8 | |
| 0.00 | 1.30 | 0.00 | 0.78 | -24.02 | 91.78 | 31.10 | 237.09 | 0.5642 | 744.0 | 555.8 | |
| 0.00 | 1.21 | 0.00 | 0.73 | -25.14 | 91.43 | 30.76 | 235.06 | 0.5670 | 857.0 | 785.6 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -25.41 | 90.63 | 29.96 | 234.05 | 0.5593 | 685.0 | 511.4 | |
| 0.00 | 3.29 | 0.00 | 1.95 | -26.17 | 89.47 | 28.80 | 231.94 | 0.5512 | -617.0 | -505.0 | |
| 0.00 | 1.47 | 0.00 | 0.87 | -26.52 | 89.53 | 28.85 | 231.44 | 0.5543 | -569.0 | -450.5 | |
| 0.00 | 3.89 | 0.00 | 2.30 | -26.49 | 88.91 | 28.24 | 230.98 | 0.5472 | -609.0 | -639.8 | |
| 0.00 | 1.99 | 0.00 | 1.18 | -26.95 | 88.62 | 27.95 | 230.01 | 0.5474 | -712.0 | -504.3 | |
| 0.00 | 0.69 | 0.00 | 0.41 | -26.99 | 88.44 | 27.77 | 229.79 | 0.5457 | -705.0 | -599.1 | |
| 0.00 | 2.60 | 0.00 | 1.53 | -27.28 | 88.48 | 27.81 | 229.38 | 0.5484 | -875.0 | -689.8 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -26.47 | 88.19 | 27.52 | 230.41 | 0.5388 | -697.0 | -548.9 | |
| 0.00 | 0.87 | 0.00 | 0.51 | -27.51 | 88.35 | 27.68 | 228.92 | 0.5488 | -529.0 | -421.6 | |
| 0.87 | 1.64 | 0.51 | 0.97 | -27.91 | 88.05 | 27.37 | 228.03 | 0.5486 | 610.5 | 537.7 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -30.49 | 88.22 | 27.54 | 224.39 | 0.5718 | -674.0 | -708.1 | |
| 0.00 | 2.51 | 0.00 | 1.51 | -30.73 | 88.02 | 27.34 | 223.88 | 0.5719 | -763.0 | -660.8 | |
| 0.00 | 5.10 | 0.00 | 3.01 | -28.43 | 87.35 | 26.68 | 226.61 | 0.5455 | 646.0 | 462.1 | |
| 1.30 | 4.07 | 0.76 | 2.37 | -27.50 | 86.73 | 26.06 | 227.46 | 0.5310 | -847.8 | -667.2 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -28.40 | 86.67 | 25.99 | 226.01 | 0.5379 | -629.0 | -504.8 | |
| 0.00 | 2.42 | 0.00 | 1.41 | -27.83 | 85.74 | 25.06 | 225.96 | 0.5232 | -809.0 | -673.2 | |
| 0.00 | 1.04 | 0.00 | 0.60 | -27.41 | 85.34 | 24.66 | 226.22 | 0.5151 | -445.0 | -383.7 | |
| 0.00 | 1.64 | 0.00 | 0.95 | -27.32 | 85.21 | 24.53 | 226.23 | 0.5129 | -685.0 | -484.2 | |
| 32.27 | 179.35 | 18.46 | 102.51 | -26.41 | 84.96 | 24.29 | 227.43 | 0.5022 | -1266.2 | -430.6 | |
| 0.00 | 0.52 | 0.00 | 0.30 | -28.19 | 85.12 | 24.44 | 224.79 | 0.5198 | -657.0 | -551.5 | |
| 0.00 | 0.61 | 0.00 | 0.35 | -29.83 | 85.04 | 24.37 | 222.26 | 0.5344 | -497.0 | -502.1 | |
| 0.00 | 2.08 | 0.00 | 1.20 | -28.43 | 84.62 | 23.95 | 223.89 | 0.5169 | -737.0 | -652.9 | |
| 0.00 | 1.38 | 0.00 | 0.78 | -25.56 | 83.55 | 22.88 | 227.33 | 0.4789 | -912.0 | -743.4 | |
| 0.00 | 1.38 | 0.00 | 0.78 | -25.20 | 83.23 | 22.55 | 227.59 | 0.4720 | -712.0 | -498.3 | |
| 0.00 | 1.04 | 0.00 | 0.60 | -29.04 | 83.39 | 22.72 | 221.64 | 0.5103 | -771.0 | -635.9 | |
| 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. | |