SDO HMI 2014-07-07 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 85.70 | 567.14 | 50.29 | 333.90 | -19.20 | 255.16 | 23.76 | 224.83 | 0.5414 | 794.6 | 322.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.73 | 0.00 | 0.49 | -21.71 | 266.88 | 35.48 | 232.34 | 0.6835 | 634.0 | 471.1 | |
| 0.00 | 0.73 | 0.00 | 0.48 | -20.35 | 266.20 | 34.79 | 233.57 | 0.6672 | 614.0 | 562.1 | |
| 0.00 | 0.54 | 0.00 | 0.37 | -21.32 | 266.41 | 35.01 | 232.48 | 0.6761 | 647.0 | 462.2 | |
| 0.00 | 1.18 | 0.00 | 0.78 | -20.23 | 265.77 | 34.37 | 233.40 | 0.6620 | 731.0 | 615.8 | |
| 0.00 | 1.36 | 0.00 | 0.90 | -20.03 | 265.64 | 34.24 | 233.57 | 0.6592 | 84.0 | 169.6 | |
| 0.00 | 1.54 | 0.00 | 1.02 | -20.52 | 265.53 | 34.12 | 232.85 | 0.6614 | 582.0 | 437.1 | |
| 0.00 | 1.54 | 0.00 | 1.00 | -18.62 | 265.00 | 33.59 | 234.96 | 0.6427 | -549.0 | -407.0 | |
| 0.00 | 1.27 | 0.00 | 0.83 | -21.06 | 264.68 | 33.28 | 231.51 | 0.6564 | 729.0 | 620.4 | |
| 0.00 | 0.45 | 0.00 | 0.30 | -21.53 | 264.80 | 33.40 | 231.01 | 0.6611 | 541.0 | 443.8 | |
| 0.00 | 1.63 | 0.00 | 1.07 | -21.45 | 264.55 | 33.14 | 230.90 | 0.6579 | 741.0 | 526.1 | |
| 0.00 | 1.18 | 0.00 | 0.75 | -20.83 | 262.08 | 30.68 | 229.67 | 0.6278 | 753.0 | 540.6 | |
| 0.00 | 1.09 | 0.00 | 0.69 | -23.89 | 259.57 | 28.17 | 223.53 | 0.6289 | -726.0 | -514.5 | |
| 0.00 | 1.09 | 0.00 | 0.71 | -27.03 | 258.71 | 27.31 | 219.11 | 0.6502 | -773.0 | -663.4 | |
| 0.00 | 1.27 | 0.00 | 0.77 | -21.98 | 255.77 | 24.37 | 221.93 | 0.5747 | -783.0 | -659.1 | |
| 81.89 | 520.68 | 48.06 | 305.52 | -18.96 | 255.09 | 23.69 | 225.14 | 0.5381 | 1402.7 | 383.2 | |
| 0.00 | 1.82 | 0.00 | 1.10 | -22.74 | 255.37 | 23.96 | 220.52 | 0.5787 | -978.0 | -842.8 | |
| 0.91 | -15.00 | 0.53 | -15.00 | -18.64 | 254.41 | 23.01 | 224.78 | 0.5279 | 1406.1 | 999999 | |
| 1.54 | -15.00 | 0.90 | -15.00 | -18.80 | 254.26 | 22.86 | 224.37 | 0.5279 | 1392.8 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.99 | -22.83 | 254.77 | 23.37 | 219.73 | 0.5740 | -954.0 | -814.3 | |
| 0.00 | 1.09 | 0.00 | 0.66 | -22.76 | 254.65 | 23.24 | 219.68 | 0.5722 | -417.0 | -391.0 | |
| 1.00 | -15.00 | 0.58 | -15.00 | -18.69 | 253.72 | 22.32 | 223.86 | 0.5211 | 902.3 | 999999 | |
| 0.00 | 2.81 | 0.00 | 1.68 | -22.14 | 254.25 | 22.85 | 219.97 | 0.5621 | 815.0 | 670.1 | |
| 0.36 | 6.90 | 0.22 | 4.16 | -23.02 | 254.30 | 22.90 | 218.95 | 0.5717 | -991.8 | -812.7 | |
| 0.00 | 1.09 | 0.00 | 0.65 | -22.71 | 254.10 | 22.70 | 219.09 | 0.5667 | -972.0 | -847.8 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -21.79 | 253.91 | 22.51 | 219.99 | 0.5552 | 671.0 | 517.3 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -20.62 | 252.60 | 21.20 | 219.84 | 0.5303 | 692.0 | 564.8 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -21.04 | 252.10 | 20.70 | 218.65 | 0.5303 | -716.0 | -493.6 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -18.63 | 251.37 | 19.96 | 220.84 | 0.4966 | -742.0 | -595.6 | |
| 0.00 | 1.72 | 0.00 | 0.99 | -20.15 | 251.18 | 19.78 | 218.55 | 0.5118 | -596.0 | -432.3 | |
| 0.00 | 2.27 | 0.00 | 1.30 | -20.11 | 250.90 | 19.50 | 218.21 | 0.5087 | -778.0 | -526.0 | |
| 0.00 | 2.27 | 0.00 | 1.30 | -19.93 | 250.53 | 19.13 | 217.92 | 0.5033 | -690.0 | -520.0 | |
| 0.00 | 1.63 | 0.00 | 0.96 | -25.36 | 246.62 | 15.22 | 206.22 | 0.5389 | -742.0 | -633.8 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -24.79 | 245.79 | 14.38 | 205.49 | 0.5261 | -687.0 | -552.8 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -25.23 | 245.49 | 14.09 | 204.64 | 0.5301 | -614.0 | -474.2 | |
| 0.00 | 0.73 | 0.00 | 0.42 | -25.30 | 245.29 | 13.89 | 204.28 | 0.5298 | -646.0 | -525.6 | |
| 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. | |