SDO HMI 2014-02-26 10:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 93.41 | 378.36 | 88.08 | 353.83 | -13.09 | 108.11 | -58.49 | 101.02 | 0.8457 | 277.3 | -62.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.50 | 0.00 | 1.59 | -12.66 | 127.52 | -39.09 | 101.31 | 0.6296 | 284.0 | 398.6 | |
| 0.00 | 1.38 | 0.00 | 0.89 | -16.42 | 126.50 | -40.10 | 107.00 | 0.6484 | 601.0 | 515.8 | |
| 4.48 | 8.70 | 2.87 | 5.58 | -11.21 | 126.91 | -39.70 | 98.95 | 0.6366 | 836.2 | 615.2 | |
| 0.00 | 3.71 | 0.00 | 2.38 | -11.56 | 126.85 | -39.76 | 99.50 | 0.6376 | 715.0 | 645.8 | |
| 0.00 | 2.59 | 0.00 | 1.73 | -18.82 | 124.88 | -41.72 | 110.21 | 0.6736 | 542.0 | 345.5 | |
| 0.00 | 1.55 | 0.00 | 0.99 | -7.10 | 127.15 | -39.46 | 92.46 | 0.6335 | 640.0 | 512.8 | |
| 0.60 | 2.50 | 0.39 | 1.61 | -11.00 | 126.55 | -40.06 | 98.60 | 0.6412 | 672.1 | 535.0 | |
| 0.00 | 1.21 | 0.00 | 0.79 | -14.78 | 125.76 | -40.85 | 104.36 | 0.6551 | 686.0 | 580.9 | |
| 0.00 | 0.69 | 0.00 | 0.46 | -16.18 | 124.67 | -41.93 | 106.27 | 0.6709 | 613.0 | 508.6 | |
| 0.00 | 0.86 | 0.00 | 0.57 | -14.83 | 124.85 | -41.76 | 104.29 | 0.6667 | 420.0 | 429.3 | |
| 0.00 | 0.69 | 0.00 | 0.46 | -14.58 | 124.03 | -42.57 | 103.80 | 0.6765 | 599.0 | 510.2 | |
| 0.00 | 1.21 | 0.00 | 0.81 | -14.66 | 123.85 | -42.76 | 103.89 | 0.6789 | 454.0 | 396.3 | |
| 0.00 | 0.78 | 0.00 | 0.53 | -10.02 | 122.72 | -43.89 | 97.02 | 0.6902 | 344.0 | 269.7 | |
| 0.00 | 0.60 | 0.00 | 0.41 | -11.39 | 122.25 | -44.35 | 98.99 | 0.6962 | 518.0 | 459.0 | |
| 0.00 | 2.41 | 0.00 | 1.69 | -10.84 | 121.16 | -45.45 | 98.18 | 0.7094 | 535.0 | 423.8 | |
| 0.00 | 0.69 | 0.00 | 0.49 | -10.79 | 120.21 | -46.40 | 98.09 | 0.7208 | 591.0 | 459.4 | |
| 0.00 | 0.69 | 0.00 | 0.49 | -8.63 | 120.21 | -46.40 | 95.09 | 0.7211 | 398.0 | 368.5 | |
| 0.00 | 1.29 | 0.00 | 1.07 | -13.60 | 112.75 | -53.86 | 101.65 | 0.8036 | -516.0 | -367.3 | |
| 0.00 | 0.78 | 0.00 | 0.69 | -18.54 | 110.14 | -56.47 | 107.56 | 0.8311 | -531.0 | -430.9 | |
| 0.00 | 0.69 | 0.00 | 0.58 | -12.70 | 111.89 | -54.72 | 100.52 | 0.8122 | -602.0 | -556.1 | |
| 0.00 | 1.38 | 0.00 | 1.16 | -12.20 | 112.00 | -54.61 | 99.89 | 0.8111 | 434.0 | 296.9 | |
| 0.00 | 0.60 | 0.00 | 0.52 | -12.67 | 111.26 | -55.35 | 100.47 | 0.8184 | -459.0 | -441.7 | |
| 0.00 | 1.03 | 0.00 | 0.89 | -10.11 | 110.99 | -55.61 | 97.35 | 0.8213 | 597.0 | 469.4 | |
| 0.00 | 0.69 | 0.00 | 0.61 | -11.60 | 110.29 | -56.31 | 99.18 | 0.8278 | 546.0 | 507.2 | |
| 0.00 | 0.78 | 0.00 | 0.69 | -11.27 | 110.01 | -56.60 | 98.79 | 0.8306 | 524.0 | 457.4 | |
| 0.00 | 1.03 | 0.00 | 0.95 | -12.53 | 108.51 | -58.09 | 100.32 | 0.8445 | -131.0 | -158.9 | |
| 1.38 | 333.88 | 1.29 | 321.75 | -13.42 | 107.76 | -58.84 | 101.38 | 0.8512 | -801.6 | -108.0 | |
| 23.18 | -27.00 | 22.01 | -27.00 | -13.71 | 107.29 | -59.32 | 101.71 | 0.8554 | -784.1 | 999999 | |
| 0.00 | 1.55 | 0.00 | 1.52 | -15.28 | 106.08 | -60.53 | 103.55 | 0.8659 | -335.0 | -363.9 | |
| 5.86 | -27.00 | 5.72 | -27.00 | -14.28 | 106.36 | -60.24 | 102.38 | 0.8634 | -397.6 | 999999 | |
| 1.03 | -27.00 | 1.00 | -27.00 | -13.84 | 106.56 | -60.05 | 101.87 | 0.8617 | 294.8 | 999999 | |
| 56.88 | -27.00 | 54.80 | -27.00 | -12.75 | 106.82 | -59.78 | 100.60 | 0.8595 | 748.3 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.44 | -15.37 | 104.88 | -61.73 | 103.63 | 0.8758 | 336.0 | 293.4 | |
| 0.00 | 0.95 | 0.00 | 0.96 | -14.15 | 104.89 | -61.71 | 102.24 | 0.8757 | 275.0 | 162.2 | |
| 0.00 | 0.52 | 0.00 | 0.53 | -14.03 | 104.89 | -61.72 | 102.10 | 0.8758 | 316.0 | 259.7 | |
| 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. | |