SDO HMI 2014-07-07 19:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 81.52 | 550.44 | 48.07 | 325.62 | -19.29 | 255.14 | 24.30 | 225.36 | 0.5480 | 768.3 | 337.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.91 | 0.00 | 0.61 | -20.34 | 266.48 | 35.63 | 234.17 | 0.6760 | 139.0 | 222.9 | |
| 0.00 | 1.00 | 0.00 | 0.67 | -20.37 | 266.20 | 35.36 | 233.94 | 0.6733 | 599.0 | 507.5 | |
| 0.00 | 1.09 | 0.00 | 0.72 | -20.22 | 265.73 | 34.88 | 233.80 | 0.6673 | 736.0 | 587.9 | |
| 0.00 | 1.63 | 0.00 | 1.08 | -21.04 | 264.71 | 33.87 | 231.98 | 0.6624 | 737.0 | 588.7 | |
| 0.00 | 1.63 | 0.00 | 1.08 | -21.47 | 264.51 | 33.66 | 231.28 | 0.6634 | 612.0 | 486.8 | |
| 0.00 | 1.00 | 0.00 | 0.66 | -21.46 | 264.27 | 33.42 | 231.11 | 0.6609 | 606.0 | 470.9 | |
| 0.00 | 1.36 | 0.00 | 0.89 | -22.15 | 262.85 | 32.00 | 229.10 | 0.6516 | 503.0 | 363.6 | |
| 0.00 | 0.82 | 0.00 | 0.52 | -20.85 | 262.07 | 31.22 | 230.11 | 0.6336 | 700.0 | 573.4 | |
| 0.00 | 1.00 | 0.00 | 0.64 | -23.87 | 259.62 | 28.77 | 224.12 | 0.6344 | -706.0 | -534.2 | |
| 0.00 | 1.00 | 0.00 | 0.64 | -24.38 | 259.33 | 28.48 | 223.24 | 0.6362 | -676.0 | -531.3 | |
| 0.00 | 1.18 | 0.00 | 0.77 | -27.04 | 258.71 | 27.86 | 219.62 | 0.6549 | -723.0 | -609.8 | |
| 0.00 | 0.27 | 0.00 | 0.17 | -21.98 | 255.69 | 24.84 | 222.44 | 0.5794 | -613.0 | -570.3 | |
| 0.00 | 0.91 | 0.00 | 0.56 | -23.45 | 255.94 | 25.09 | 220.91 | 0.5962 | -568.0 | -491.8 | |
| 80.07 | 499.60 | 47.20 | 294.49 | -18.97 | 255.10 | 24.26 | 225.78 | 0.5442 | 1409.5 | 402.6 | |
| 0.00 | 2.00 | 0.00 | 1.22 | -22.72 | 255.43 | 24.58 | 221.24 | 0.5842 | -892.0 | -774.0 | |
| 0.00 | 1.18 | 0.00 | 0.73 | -23.89 | 255.59 | 24.74 | 220.01 | 0.5973 | -609.0 | -469.3 | |
| 0.00 | 1.91 | 0.00 | 1.15 | -21.99 | 254.79 | 23.94 | 221.42 | 0.5709 | -805.0 | -639.0 | |
| 0.27 | -14.00 | 0.16 | -14.00 | -18.78 | 254.23 | 23.38 | 225.03 | 0.5332 | 1480.0 | 999999 | |
| 0.36 | 5.27 | 0.22 | 3.19 | -22.77 | 254.79 | 23.94 | 220.45 | 0.5788 | -902.0 | -287.4 | |
| 0.00 | 1.36 | 0.00 | 0.82 | -22.33 | 254.60 | 23.75 | 220.78 | 0.5724 | 497.0 | 421.4 | |
| 0.00 | 4.63 | 0.00 | 2.81 | -22.97 | 254.50 | 23.65 | 219.88 | 0.5781 | -849.0 | -863.6 | |
| 0.82 | 2.27 | 0.49 | 1.36 | -22.15 | 254.24 | 23.39 | 220.59 | 0.5673 | 762.1 | 604.3 | |
| 0.00 | 0.91 | 0.00 | 0.54 | -21.87 | 254.12 | 23.27 | 220.79 | 0.5633 | 637.0 | 531.7 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -19.89 | 253.80 | 22.95 | 222.98 | 0.5399 | 181.0 | 131.7 | |
| 0.00 | 1.72 | 0.00 | 1.04 | -22.72 | 254.13 | 23.28 | 219.76 | 0.5721 | -856.0 | -688.9 | |
| 0.00 | 1.54 | 0.00 | 0.92 | -21.83 | 253.83 | 22.98 | 220.50 | 0.5602 | 498.0 | 410.4 | |
| 0.00 | 1.27 | 0.00 | 0.77 | -23.33 | 254.09 | 23.24 | 218.98 | 0.5782 | -441.0 | -278.2 | |
| 0.00 | 1.63 | 0.00 | 0.96 | -20.69 | 252.55 | 21.70 | 220.38 | 0.5360 | 467.0 | 397.4 | |
| 0.00 | 0.91 | 0.00 | 0.53 | -21.08 | 252.05 | 21.20 | 219.24 | 0.5354 | -571.0 | -470.8 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -18.64 | 251.36 | 20.52 | 221.58 | 0.5023 | -742.0 | -619.8 | |
| 0.00 | 2.27 | 0.00 | 1.31 | -20.19 | 251.15 | 20.30 | 219.20 | 0.5173 | -457.0 | -384.2 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -20.12 | 250.90 | 20.05 | 218.96 | 0.5141 | -717.0 | -543.0 | |
| 0.00 | 0.91 | 0.00 | 0.53 | -25.36 | 246.67 | 15.82 | 207.09 | 0.5431 | -658.0 | -529.2 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -25.19 | 246.58 | 15.73 | 207.12 | 0.5402 | -673.0 | -552.4 | |
| 0.00 | 2.54 | 0.00 | 1.49 | -25.27 | 245.40 | 14.55 | 205.30 | 0.5336 | -580.0 | -523.0 | |
| 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. | |