SDO HMI 2011-06-22 06:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.80 | 512.57 | 45.53 | 295.52 | 17.26 | 168.92 | 27.01 | 302.10 | 0.5131 | -494.8 | -305.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.82 | 0.00 | 1.13 | 16.51 | 176.40 | 34.49 | 295.47 | 0.6035 | -662.0 | -544.5 | |
| 0.00 | 0.91 | 0.00 | 0.55 | 14.05 | 175.14 | 33.23 | 292.16 | 0.5762 | -720.0 | -617.0 | |
| 0.00 | 1.09 | 0.00 | 0.67 | 22.24 | 173.00 | 31.09 | 306.43 | 0.5962 | -756.0 | -603.3 | |
| 0.00 | 1.18 | 0.00 | 0.70 | 18.71 | 171.73 | 29.82 | 301.99 | 0.5574 | -647.0 | -468.9 | |
| 69.99 | 439.11 | 40.65 | 254.82 | 17.15 | 169.87 | 27.96 | 300.85 | 0.5239 | -1485.2 | -432.5 | |
| 0.00 | 1.09 | 0.00 | 0.62 | 18.36 | 167.34 | 25.43 | 305.18 | 0.5006 | -711.0 | -464.7 | |
| 3.00 | 4.90 | 1.71 | 2.80 | 18.77 | 167.19 | 25.29 | 306.03 | 0.5021 | 685.3 | 587.3 | |
| 0.00 | 1.63 | 0.00 | 0.93 | 18.71 | 166.83 | 24.92 | 306.30 | 0.4971 | 385.0 | 445.7 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 14.44 | 165.76 | 23.85 | 299.41 | 0.4514 | -798.0 | -617.8 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 16.36 | 165.06 | 23.15 | 303.87 | 0.4562 | 741.0 | 635.8 | |
| 0.00 | 2.91 | 0.00 | 1.60 | 14.92 | 164.72 | 22.81 | 301.41 | 0.4407 | -760.0 | -645.8 | |
| 0.00 | 1.18 | 0.00 | 0.66 | 18.14 | 164.50 | 22.59 | 307.79 | 0.4637 | 775.0 | 542.3 | |
| 0.00 | 0.91 | 0.00 | 0.51 | 18.11 | 164.21 | 22.31 | 308.06 | 0.4600 | 816.0 | 622.8 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 18.62 | 164.11 | 22.20 | 309.09 | 0.4633 | 744.0 | 530.8 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 17.64 | 163.43 | 21.52 | 308.14 | 0.4463 | 971.0 | 786.1 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 17.80 | 163.38 | 21.47 | 308.49 | 0.4471 | 764.0 | 685.5 | |
| 2.54 | 5.90 | 1.39 | 3.22 | 15.60 | 162.95 | 21.04 | 304.75 | 0.4226 | 944.7 | 807.9 | |
| 0.00 | 1.63 | 0.00 | 0.90 | 17.78 | 162.62 | 20.71 | 309.39 | 0.4376 | 791.0 | 673.4 | |
| 0.00 | 2.54 | 0.00 | 1.41 | 18.70 | 162.63 | 20.73 | 311.06 | 0.4464 | 838.0 | 695.9 | |
| 0.00 | 2.09 | 0.00 | 1.15 | 18.45 | 162.50 | 20.59 | 310.78 | 0.4424 | 882.0 | 651.3 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 17.88 | 162.39 | 20.49 | 309.87 | 0.4358 | 704.0 | 541.9 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 17.50 | 162.14 | 20.24 | 309.49 | 0.4292 | 737.0 | 489.5 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 17.34 | 161.85 | 19.95 | 309.57 | 0.4242 | 783.0 | 625.9 | |
| 0.00 | 2.00 | 0.00 | 1.10 | 19.22 | 162.01 | 20.10 | 312.80 | 0.4441 | 706.0 | 602.5 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 19.51 | 161.71 | 19.80 | 313.72 | 0.4436 | 745.0 | 672.2 | |
| 0.36 | 3.09 | 0.20 | 1.70 | 19.32 | 161.54 | 19.64 | 313.61 | 0.4398 | 967.5 | 753.0 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 21.34 | 161.57 | 19.66 | 316.96 | 0.4611 | 771.0 | 695.8 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 18.27 | 161.01 | 19.10 | 312.48 | 0.4231 | 789.0 | 627.6 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 17.35 | 160.70 | 18.80 | 311.19 | 0.4104 | 817.0 | 641.6 | |
| 0.00 | 3.54 | 0.00 | 1.92 | 17.51 | 160.52 | 18.61 | 311.77 | 0.4097 | 711.0 | 592.6 | |
| 2.91 | 10.71 | 1.58 | 5.81 | 17.80 | 160.15 | 18.24 | 312.87 | 0.4082 | 922.1 | 812.7 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 16.92 | 160.02 | 18.11 | 311.34 | 0.3978 | 837.0 | 681.9 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 20.42 | 159.93 | 18.03 | 317.83 | 0.4338 | 568.0 | 457.7 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 21.75 | 159.65 | 17.75 | 320.38 | 0.4458 | 855.0 | 685.8 | |
| 0.00 | 1.91 | 0.00 | 1.04 | 19.21 | 159.18 | 17.27 | 316.93 | 0.4123 | 718.0 | 643.8 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 19.25 | 158.85 | 16.94 | 317.53 | 0.4091 | 697.0 | 594.6 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 19.35 | 158.32 | 16.41 | 318.57 | 0.4046 | 733.0 | 457.7 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 17.63 | 154.71 | 12.81 | 322.25 | 0.3465 | 839.0 | 681.8 | |
| 0.00 | 2.09 | 0.00 | 1.12 | 20.44 | 154.67 | 12.76 | 327.07 | 0.3824 | 763.0 | 680.8 | |
| 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. | |