SDO HMI 2014-05-18 18:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.34 | 42.47 | 1.40 | 25.25 | -17.99 | 143.09 | -30.04 | 120.45 | 0.5521 | 198.2 | 256.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.35 | 0.00 | 0.77 | -19.45 | 147.83 | -25.30 | 126.57 | 0.5037 | 560.0 | 409.5 | |
| 0.00 | 2.79 | 0.00 | 1.59 | -18.69 | 147.78 | -25.35 | 125.21 | 0.4984 | 793.0 | 678.5 | |
| 0.00 | 2.16 | 0.00 | 1.24 | -19.76 | 147.39 | -25.75 | 126.65 | 0.5116 | 837.0 | 669.5 | |
| 0.72 | 1.71 | 0.41 | 0.98 | -18.96 | 147.06 | -26.07 | 124.99 | 0.5094 | 860.8 | 666.8 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -18.89 | 146.54 | -26.60 | 124.38 | 0.5153 | 794.0 | 607.4 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -16.77 | 146.42 | -26.71 | 120.59 | 0.5020 | 880.0 | 805.0 | |
| 0.00 | 2.43 | 0.00 | 1.39 | -16.36 | 146.48 | -26.65 | 119.90 | 0.4985 | 807.0 | 583.9 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -19.16 | 145.91 | -27.22 | 124.29 | 0.5250 | 655.0 | 567.9 | |
| 0.00 | 2.16 | 0.00 | 1.24 | -17.17 | 146.14 | -26.99 | 121.07 | 0.5083 | 838.0 | 734.1 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -16.08 | 146.10 | -27.04 | 119.07 | 0.5017 | 595.0 | 532.7 | |
| 0.00 | 1.80 | 0.00 | 1.04 | -18.30 | 145.74 | -27.39 | 122.69 | 0.5211 | 586.0 | 402.2 | |
| 0.00 | 1.71 | 0.00 | 1.00 | -19.02 | 145.36 | -27.78 | 123.58 | 0.5309 | 766.0 | 660.2 | |
| 0.00 | 2.61 | 0.00 | 1.50 | -17.07 | 145.66 | -27.47 | 120.49 | 0.5138 | 760.0 | 530.7 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -19.15 | 145.19 | -27.94 | 123.65 | 0.5339 | 636.0 | 536.1 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -15.40 | 145.13 | -28.00 | 117.10 | 0.5105 | -593.0 | -491.3 | |
| 0.00 | 1.53 | 0.00 | 0.89 | -16.99 | 144.81 | -28.32 | 119.68 | 0.5243 | 601.0 | 471.3 | |
| 0.90 | 4.31 | 0.53 | 2.55 | -17.85 | 143.49 | -29.64 | 120.15 | 0.5465 | 977.0 | 701.4 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -12.81 | 142.70 | -30.43 | 110.86 | 0.5306 | 556.0 | 436.2 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -18.76 | 137.28 | -35.85 | 117.68 | 0.6285 | -688.0 | -562.7 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -18.41 | 137.33 | -35.80 | 117.18 | 0.6262 | -566.0 | -498.5 | |
| 0.00 | 1.53 | 0.00 | 0.97 | -18.02 | 136.83 | -36.30 | 116.34 | 0.6305 | -868.0 | -683.1 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -19.43 | 136.27 | -36.86 | 118.14 | 0.6438 | -599.0 | -502.5 | |
| 0.72 | 1.80 | 0.46 | 1.15 | -17.88 | 136.39 | -36.75 | 115.91 | 0.6352 | -847.8 | -769.2 | |
| 0.00 | 1.08 | 0.00 | 0.69 | -18.23 | 136.22 | -36.91 | 116.34 | 0.6388 | -720.0 | -536.5 | |
| 0.00 | 1.71 | 0.00 | 1.11 | -18.69 | 135.66 | -37.47 | 116.74 | 0.6476 | -584.0 | -404.5 | |
| 0.00 | 1.35 | 0.00 | 0.88 | -18.36 | 135.06 | -38.07 | 115.97 | 0.6533 | -711.0 | -608.9 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -17.79 | 135.12 | -38.01 | 115.17 | 0.6501 | -398.0 | -356.0 | |
| 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. | |