SDO HMI 2014-03-14 08:11:44 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 57.51 | 0.00 | 29.98 | -10.73 | 300.32 | -16.47 | 101.18 | 0.2949 | 178.4 | 89.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.65 | 0.00 | 0.82 | -1.46 | 314.57 | -2.23 | 21.32 | 0.1074 | 731.0 | 592.2 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -11.79 | 309.86 | -6.93 | 124.55 | 0.1441 | 744.0 | 589.0 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -7.81 | 309.13 | -7.66 | 95.26 | 0.1332 | 738.0 | 515.6 | |
| 0.00 | 1.22 | 0.00 | 0.61 | -7.39 | 308.75 | -8.05 | 92.01 | 0.1396 | 718.0 | 570.9 | |
| 0.00 | 1.30 | 0.00 | 0.66 | -16.17 | 306.33 | -10.46 | 132.22 | 0.2366 | 765.0 | 575.6 | |
| 0.00 | 2.26 | 0.00 | 1.14 | -11.16 | 305.35 | -11.44 | 110.28 | 0.2084 | 835.0 | 615.1 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -10.82 | 305.03 | -11.77 | 108.28 | 0.2119 | 688.0 | 464.7 | |
| 0.00 | 1.48 | 0.00 | 0.75 | -6.77 | 305.13 | -11.66 | 88.69 | 0.2017 | 801.0 | 645.4 | |
| 0.00 | 0.52 | 0.00 | 0.26 | -4.70 | 304.72 | -12.07 | 79.01 | 0.2133 | 350.0 | 299.2 | |
| 0.00 | 1.13 | 0.00 | 0.58 | -11.12 | 303.90 | -12.90 | 108.16 | 0.2316 | 740.0 | 618.3 | |
| 0.00 | 2.09 | 0.00 | 1.07 | -13.24 | 303.60 | -13.19 | 116.09 | 0.2485 | 661.0 | 528.2 | |
| 0.00 | 1.56 | 0.00 | 0.80 | -9.05 | 303.39 | -13.40 | 98.93 | 0.2327 | 859.0 | 780.1 | |
| 0.00 | 2.87 | 0.00 | 1.47 | -11.94 | 303.14 | -13.66 | 110.51 | 0.2478 | 631.0 | 573.4 | |
| 0.00 | 2.69 | 0.00 | 1.38 | -11.30 | 302.95 | -13.84 | 107.83 | 0.2476 | 887.0 | 766.8 | |
| 0.00 | 1.39 | 0.00 | 0.71 | -10.97 | 302.84 | -13.95 | 106.42 | 0.2479 | 837.0 | 792.4 | |
| 0.00 | 1.04 | 0.00 | 0.53 | -11.15 | 302.74 | -14.05 | 107.01 | 0.2503 | 648.0 | 575.1 | |
| 0.00 | 1.30 | 0.00 | 0.67 | -5.31 | 302.93 | -13.87 | 83.06 | 0.2415 | 627.0 | 462.4 | |
| 0.00 | 1.13 | 0.00 | 0.58 | -10.64 | 302.61 | -14.19 | 104.89 | 0.2504 | 620.0 | 521.6 | |
| 0.00 | 1.65 | 0.00 | 0.85 | -10.69 | 302.39 | -14.41 | 104.90 | 0.2542 | 514.0 | 425.4 | |
| 0.00 | 1.82 | 0.00 | 0.94 | -2.83 | 302.17 | -14.62 | 74.12 | 0.2633 | 832.0 | 697.1 | |
| 0.00 | 1.22 | 0.00 | 0.63 | -2.78 | 301.55 | -15.24 | 74.61 | 0.2735 | 738.0 | 545.4 | |
| 0.00 | 1.22 | 0.00 | 0.63 | -1.75 | 299.48 | -17.31 | 73.35 | 0.3118 | -869.0 | -643.1 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -11.16 | 298.08 | -18.71 | 103.56 | 0.3252 | -651.0 | -509.1 | |
| 0.00 | 1.22 | 0.00 | 0.64 | -1.64 | 298.26 | -18.53 | 74.18 | 0.3317 | 810.0 | 640.0 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -11.86 | 297.68 | -19.12 | 105.42 | 0.3339 | -579.0 | -544.4 | |
| 0.00 | 0.87 | 0.00 | 0.45 | -7.57 | 297.87 | -18.92 | 92.40 | 0.3232 | -775.0 | -604.4 | |
| 0.00 | 1.74 | 0.00 | 0.91 | -6.28 | 297.74 | -19.06 | 88.43 | 0.3261 | -456.0 | -357.6 | |
| 0.00 | 1.30 | 0.00 | 0.69 | -11.17 | 296.95 | -19.84 | 103.01 | 0.3433 | -667.0 | -494.0 | |
| 0.00 | 2.52 | 0.00 | 1.34 | -13.77 | 296.05 | -20.74 | 109.63 | 0.3668 | -772.0 | -649.1 | |
| 0.00 | 1.22 | 0.00 | 0.65 | -13.84 | 294.92 | -21.87 | 109.03 | 0.3842 | -611.0 | -520.9 | |
| 0.00 | 1.13 | 0.00 | 0.61 | -14.68 | 294.07 | -22.72 | 110.52 | 0.4007 | -584.0 | -545.4 | |
| 0.00 | 1.56 | 0.00 | 0.85 | -15.37 | 293.49 | -23.31 | 111.77 | 0.4125 | -679.0 | -521.6 | |
| 0.00 | 4.52 | 0.00 | 2.46 | -15.53 | 293.13 | -23.66 | 111.90 | 0.4186 | -615.0 | -628.2 | |
| 0.00 | 4.69 | 0.00 | 2.56 | -15.05 | 293.05 | -23.74 | 110.73 | 0.4175 | -817.0 | -624.8 | |
| 0.00 | 1.13 | 0.00 | 0.62 | -15.12 | 292.77 | -24.02 | 110.72 | 0.4219 | -647.0 | -484.4 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -15.72 | 292.63 | -24.16 | 111.99 | 0.4267 | -628.0 | -575.2 | |
| 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. | |