SDO HMI 2014-11-10 06:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.64 | 148.97 | 31.67 | 216.12 | -11.19 | 305.05 | -68.80 | 103.22 | 0.9406 | -307.1 | -304.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.26 | 0.00 | 0.23 | -11.16 | 318.61 | -55.23 | 105.70 | 0.8393 | 212.0 | 195.0 | |
| 0.00 | 0.95 | 0.00 | 0.87 | -11.41 | 317.95 | -55.90 | 105.83 | 0.8458 | 488.0 | 378.3 | |
| 0.86 | 2.24 | 0.96 | 2.50 | -11.73 | 311.72 | -62.13 | 104.89 | 0.8975 | 453.5 | 344.9 | |
| 0.00 | 2.24 | 0.00 | 2.83 | -12.70 | 308.51 | -65.34 | 105.37 | 0.9211 | 389.0 | 282.0 | |
| 0.00 | 0.26 | 0.00 | 0.33 | -11.69 | 308.03 | -65.81 | 104.20 | 0.9231 | 333.0 | 391.0 | |
| 0.00 | 0.52 | 0.00 | 0.67 | -11.25 | 307.63 | -66.21 | 103.67 | 0.9253 | 512.0 | 487.5 | |
| 0.00 | 0.26 | 0.00 | 0.34 | -11.60 | 307.39 | -66.45 | 104.01 | 0.9272 | 214.0 | 208.0 | |
| 0.00 | 1.72 | 0.00 | 2.21 | -10.42 | 307.77 | -66.07 | 102.80 | 0.9236 | 446.0 | 407.9 | |
| 0.00 | 0.60 | 0.00 | 0.79 | -11.17 | 307.36 | -66.48 | 103.55 | 0.9269 | 231.0 | 185.3 | |
| 0.52 | 1.64 | 0.67 | 2.12 | -10.32 | 307.44 | -66.41 | 102.64 | 0.9256 | 98.2 | 108.2 | |
| 0.00 | 0.26 | 0.00 | 0.36 | -12.78 | 306.07 | -67.78 | 105.05 | 0.9364 | -503.0 | -442.3 | |
| 0.00 | 3.10 | 0.00 | 4.61 | -14.30 | 304.88 | -68.97 | 106.46 | 0.9446 | -531.0 | -498.2 | |
| 0.00 | 3.19 | 0.00 | 4.34 | -11.29 | 306.45 | -67.40 | 103.53 | 0.9327 | -460.0 | -430.7 | |
| 0.00 | 1.12 | 0.00 | 1.56 | -11.95 | 306.03 | -67.82 | 104.17 | 0.9359 | -411.0 | -370.3 | |
| 0.00 | 1.38 | 0.00 | 2.08 | -14.03 | 304.62 | -69.23 | 106.14 | 0.9458 | -342.0 | -280.6 | |
| 0.00 | 7.67 | 0.00 | 11.02 | -12.66 | 305.39 | -68.46 | 104.82 | 0.9403 | -498.0 | -471.5 | |
| 1.64 | 22.93 | 2.22 | 31.04 | -10.59 | 306.38 | -67.46 | 102.77 | 0.9325 | -641.1 | -534.4 | |
| 0.00 | 1.21 | 0.00 | 1.71 | -11.37 | 305.51 | -68.33 | 103.47 | 0.9384 | -483.0 | -451.8 | |
| 1.38 | 3.53 | 1.94 | 4.99 | -10.73 | 305.50 | -68.34 | 102.80 | 0.9380 | -637.2 | -576.0 | |
| 0.00 | 18.19 | 0.00 | 26.64 | -11.35 | 304.85 | -69.00 | 103.35 | 0.9422 | -500.0 | -530.9 | |
| 0.00 | 1.72 | 0.00 | 2.77 | -13.86 | 303.29 | -70.55 | 105.76 | 0.9526 | -459.0 | -407.0 | |
| 0.78 | 21.30 | 1.10 | 30.66 | -10.04 | 305.33 | -68.52 | 102.04 | 0.9384 | -680.1 | -271.6 | |
| 0.00 | 0.86 | 0.00 | 1.25 | -10.73 | 304.91 | -68.93 | 102.72 | 0.9414 | -550.0 | -542.7 | |
| 0.00 | 3.79 | 0.00 | 6.32 | -14.05 | 302.68 | -71.17 | 105.87 | 0.9558 | 202.0 | 205.0 | |
| 5.00 | 25.87 | 7.34 | 38.85 | -10.41 | 304.64 | -69.20 | 102.34 | 0.9427 | -611.4 | -343.7 | |
| 0.00 | 0.86 | 0.00 | 1.36 | -12.56 | 303.43 | -70.42 | 104.42 | 0.9509 | -373.0 | -331.3 | |
| 0.00 | 2.07 | 0.00 | 3.10 | -11.01 | 304.25 | -69.60 | 102.92 | 0.9454 | -506.0 | -424.8 | |
| 0.00 | 3.97 | 0.00 | 6.53 | -13.43 | 302.75 | -71.10 | 105.23 | 0.9550 | -311.0 | -165.0 | |
| 0.00 | 2.07 | 0.00 | 3.27 | -12.32 | 303.40 | -70.45 | 104.17 | 0.9509 | -386.0 | -308.2 | |
| 0.69 | 1.90 | 1.13 | 3.11 | -13.15 | 302.75 | -71.09 | 104.94 | 0.9548 | -235.4 | -202.1 | |
| 0.00 | 1.29 | 0.00 | 2.18 | -13.70 | 302.36 | -71.49 | 105.46 | 0.9572 | 394.0 | 350.5 | |
| 0.00 | 0.60 | 0.00 | 0.93 | -11.34 | 303.80 | -70.05 | 103.20 | 0.9481 | -285.0 | -260.9 | |
| 3.53 | -25.00 | 5.29 | -25.00 | -10.22 | 304.21 | -69.63 | 102.08 | 0.9450 | -415.6 | 999999 | |
| 7.24 | -25.00 | 11.02 | -25.00 | -10.64 | 303.91 | -69.93 | 102.48 | 0.9469 | -422.0 | 999999 | |
| 0.00 | 9.40 | 0.00 | 14.55 | -9.96 | 303.45 | -70.40 | 101.71 | 0.9490 | -24.0 | 50.3 | |
| 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. | |