SDO HMI 2014-09-10 21:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.23 | 106.11 | 13.55 | 61.94 | -19.94 | 107.14 | 16.76 | 210.86 | 0.5299 | 367.2 | 350.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.07 | 0.00 | 0.64 | -20.33 | 110.99 | 20.62 | 215.94 | 0.5646 | 573.0 | 515.0 | |
| 0.00 | 1.78 | 0.00 | 1.07 | -20.73 | 110.98 | 20.60 | 215.48 | 0.5692 | 636.0 | 570.0 | |
| 0.00 | 1.51 | 0.00 | 0.90 | -20.44 | 110.53 | 20.15 | 215.21 | 0.5620 | 778.0 | 629.4 | |
| 0.00 | 1.07 | 0.00 | 0.63 | -20.17 | 109.88 | 19.50 | 214.62 | 0.5536 | 826.0 | 575.5 | |
| 3.03 | 10.77 | 1.80 | 6.42 | -20.54 | 109.86 | 19.48 | 214.19 | 0.5578 | 804.2 | 666.7 | |
| 0.00 | 2.85 | 0.00 | 1.69 | -20.52 | 109.38 | 19.00 | 213.56 | 0.5536 | 384.0 | 493.7 | |
| 0.00 | 1.16 | 0.00 | 0.69 | -20.71 | 109.06 | 18.68 | 212.92 | 0.5534 | 691.0 | 564.8 | |
| 4.36 | 25.55 | 2.54 | 14.86 | -19.00 | 108.58 | 18.21 | 214.10 | 0.5290 | 783.2 | 653.7 | |
| 0.00 | 4.45 | 0.00 | 2.65 | -21.01 | 108.75 | 18.38 | 212.20 | 0.5545 | 720.0 | 639.9 | |
| 5.79 | -8.00 | 3.36 | -8.00 | -18.79 | 108.36 | 17.98 | 214.01 | 0.5246 | 1097.0 | 999999 | |
| 0.00 | 1.42 | 0.00 | 0.84 | -20.99 | 108.45 | 18.07 | 211.78 | 0.5520 | 762.0 | 657.2 | |
| 1.60 | -8.00 | 0.93 | -8.00 | -18.84 | 108.13 | 17.75 | 213.61 | 0.5234 | 992.1 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.64 | -22.09 | 108.28 | 17.90 | 210.46 | 0.5640 | 525.0 | 383.1 | |
| 0.00 | 1.51 | 0.00 | 0.90 | -21.11 | 108.05 | 17.68 | 211.10 | 0.5505 | 732.0 | 586.0 | |
| 3.38 | 23.59 | 1.97 | 13.76 | -20.02 | 107.25 | 16.87 | 211.04 | 0.5310 | 974.9 | 726.5 | |
| 0.00 | 0.98 | 0.00 | 0.59 | -23.31 | 107.65 | 17.27 | 208.45 | 0.5746 | 577.0 | 463.8 | |
| 2.49 | -15.00 | 1.45 | -15.00 | -19.94 | 106.94 | 16.56 | 210.66 | 0.5276 | 1054.9 | 999999 | |
| 2.58 | -15.00 | 1.50 | -15.00 | -20.14 | 106.73 | 16.35 | 210.14 | 0.5285 | 978.5 | 999999 | |
| 0.00 | 1.42 | 0.00 | 0.80 | -16.48 | 106.38 | 16.00 | 213.60 | 0.4795 | 772.0 | 700.7 | |
| 0.00 | 0.89 | 0.00 | 0.54 | -23.92 | 106.97 | 16.60 | 206.99 | 0.5776 | 780.0 | 696.6 | |
| 0.00 | 1.69 | 0.00 | 0.99 | -20.47 | 106.46 | 16.08 | 209.41 | 0.5307 | 882.0 | 664.3 | |
| 0.00 | 0.71 | 0.00 | 0.42 | -21.33 | 105.78 | 15.40 | 207.55 | 0.5370 | 472.0 | 413.8 | |
| 0.00 | 1.25 | 0.00 | 0.78 | -27.26 | 106.18 | 15.80 | 203.29 | 0.6145 | -643.0 | -359.4 | |
| 0.00 | 1.51 | 0.00 | 0.87 | -19.96 | 104.58 | 14.20 | 206.94 | 0.5109 | 624.0 | 491.5 | |
| 0.00 | 0.89 | 0.00 | 0.51 | -18.76 | 104.14 | 13.77 | 207.37 | 0.4920 | 775.0 | 645.9 | |
| 0.00 | 2.76 | 0.00 | 1.56 | -18.73 | 103.26 | 12.88 | 205.88 | 0.4856 | -756.0 | -572.3 | |
| 0.00 | 2.67 | 0.00 | 1.51 | -18.49 | 103.01 | 12.63 | 205.68 | 0.4806 | -704.0 | -545.0 | |
| 0.00 | 1.87 | 0.00 | 1.05 | -18.48 | 102.78 | 12.40 | 205.28 | 0.4790 | -797.0 | -622.7 | |
| 0.00 | 1.34 | 0.00 | 0.75 | -18.72 | 102.73 | 12.36 | 204.97 | 0.4819 | -635.0 | -496.3 | |
| 0.00 | 1.16 | 0.00 | 0.65 | -18.87 | 102.38 | 12.01 | 204.22 | 0.4819 | -821.0 | -660.2 | |
| 0.00 | 1.51 | 0.00 | 0.85 | -18.10 | 102.17 | 11.79 | 204.53 | 0.4697 | -701.0 | -522.0 | |
| 0.00 | 1.34 | 0.00 | 0.75 | -18.36 | 102.09 | 11.71 | 204.14 | 0.4729 | -910.0 | -802.6 | |
| 0.00 | 1.42 | 0.00 | 0.80 | -18.53 | 102.04 | 11.66 | 203.90 | 0.4749 | -700.0 | -598.3 | |
| 0.00 | 1.87 | 0.00 | 1.05 | -18.52 | 101.81 | 11.43 | 203.49 | 0.4734 | -985.0 | -838.7 | |
| 0.00 | 1.25 | 0.00 | 0.69 | -17.71 | 101.53 | 11.15 | 203.70 | 0.4603 | -772.0 | -544.9 | |
| 0.00 | 1.78 | 0.00 | 1.09 | -27.16 | 101.04 | 10.66 | 196.29 | 0.5890 | -423.0 | -394.6 | |
| 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. | |