SDO HMI 2014-04-22 04:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 108.79 | 437.37 | 112.42 | 449.32 | -13.23 | 225.88 | 61.36 | 257.56 | 0.8757 | 287.0 | 202.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.29 | 110.83 | 21.45 | 128.99 | -10.76 | 230.02 | 65.50 | 260.46 | 0.9083 | 486.0 | 164.5 | |
| 2.13 | -1.00 | 2.48 | -1.00 | -11.06 | 229.77 | 65.25 | 260.13 | 0.9065 | 554.8 | 999999 | |
| 1.69 | -1.00 | 1.93 | -1.00 | -11.12 | 229.28 | 64.77 | 260.06 | 0.9029 | 551.2 | 999999 | |
| 7.73 | -1.00 | 8.72 | -1.00 | -10.73 | 228.91 | 64.39 | 260.51 | 0.9001 | 660.6 | 999999 | |
| 0.00 | 3.29 | 0.00 | 3.57 | -10.80 | 227.88 | 63.36 | 260.42 | 0.8923 | 755.0 | 644.2 | |
| 0.00 | 1.07 | 0.00 | 1.15 | -9.97 | 227.58 | 63.06 | 261.36 | 0.8900 | 648.0 | 589.6 | |
| 0.00 | 0.89 | 0.00 | 0.96 | -10.63 | 227.81 | 63.30 | 260.63 | 0.8918 | 605.0 | 563.3 | |
| 0.00 | 0.89 | 0.00 | 0.96 | -10.40 | 227.53 | 63.01 | 260.88 | 0.8895 | 638.0 | 587.4 | |
| 3.11 | 4.88 | 3.35 | 5.27 | -12.18 | 227.61 | 63.09 | 258.88 | 0.8902 | -167.5 | -7.4 | |
| 0.00 | 0.27 | 0.00 | 0.28 | -9.83 | 226.59 | 62.07 | 261.53 | 0.8821 | -212.0 | -204.3 | |
| 0.62 | 1.86 | 0.64 | 1.93 | -9.88 | 226.35 | 61.83 | 261.48 | 0.8801 | -306.1 | -250.9 | |
| 12.17 | 72.29 | 12.34 | 72.45 | -10.05 | 225.69 | 61.17 | 261.28 | 0.8747 | 525.9 | 487.6 | |
| 1.86 | -12.00 | 1.85 | -12.00 | -9.71 | 225.01 | 60.49 | 261.68 | 0.8690 | 659.5 | 999999 | |
| 2.75 | -12.00 | 2.74 | -12.00 | -10.13 | 225.02 | 60.50 | 261.19 | 0.8690 | 741.2 | 999999 | |
| 4.00 | -12.00 | 3.99 | -12.00 | -10.77 | 225.16 | 60.64 | 260.46 | 0.8702 | -100.1 | 999999 | |
| 1.42 | -12.00 | 1.39 | -12.00 | -9.90 | 224.45 | 59.93 | 261.46 | 0.8641 | 708.2 | 999999 | |
| 0.00 | 1.86 | 0.00 | 1.84 | -11.07 | 224.82 | 60.31 | 260.11 | 0.8674 | -224.0 | -223.1 | |
| 0.00 | 1.78 | 0.00 | 1.73 | -10.31 | 224.27 | 59.75 | 260.98 | 0.8625 | 297.0 | 259.5 | |
| 0.00 | 0.53 | 0.00 | 0.53 | -12.20 | 224.86 | 60.34 | 258.81 | 0.8678 | 426.0 | 453.0 | |
| 22.73 | 125.04 | 23.73 | 130.48 | -16.19 | 226.44 | 61.92 | 254.30 | 0.8820 | 613.9 | 162.2 | |
| 3.46 | -20.00 | 3.56 | -20.00 | -15.98 | 225.99 | 61.47 | 254.52 | 0.8784 | 985.9 | 999999 | |
| 0.00 | 1.78 | 0.00 | 1.69 | -11.20 | 223.40 | 58.88 | 259.93 | 0.8550 | 204.0 | 188.4 | |
| 0.00 | 0.98 | 0.00 | 0.91 | -12.01 | 222.78 | 58.26 | 258.96 | 0.8496 | -41.0 | -108.5 | |
| 0.00 | 0.98 | 0.00 | 0.91 | -12.45 | 222.70 | 58.18 | 258.45 | 0.8490 | -405.0 | -257.1 | |
| 0.00 | 0.44 | 0.00 | 0.41 | -11.75 | 222.22 | 57.71 | 259.26 | 0.8445 | 480.0 | 515.4 | |
| 15.81 | 33.57 | 14.68 | 31.24 | -12.95 | 222.58 | 58.07 | 257.85 | 0.8481 | -356.5 | 148.1 | |
| 0.00 | 1.69 | 0.00 | 1.54 | -13.65 | 221.85 | 57.34 | 256.99 | 0.8417 | 498.0 | 529.1 | |
| 0.00 | 1.15 | 0.00 | 1.05 | -14.00 | 221.75 | 57.24 | 256.57 | 0.8410 | 408.0 | 324.5 | |
| 0.00 | 2.58 | 0.00 | 2.33 | -13.73 | 221.60 | 57.08 | 256.87 | 0.8394 | 736.0 | 649.6 | |
| 0.00 | 0.27 | 0.00 | 0.24 | -13.12 | 221.14 | 56.62 | 257.58 | 0.8349 | 472.0 | 541.0 | |
| 3.82 | 7.37 | 3.45 | 6.65 | -14.14 | 221.47 | 56.95 | 256.38 | 0.8384 | 663.4 | 539.8 | |
| 0.00 | 2.22 | 0.00 | 2.00 | -13.63 | 221.27 | 56.75 | 256.98 | 0.8364 | 766.0 | 631.9 | |
| 0.00 | 0.89 | 0.00 | 0.81 | -15.73 | 221.77 | 57.26 | 254.51 | 0.8422 | 286.0 | 224.2 | |
| 0.36 | 1.60 | 0.32 | 1.46 | -15.98 | 221.71 | 57.19 | 254.20 | 0.8418 | 433.5 | 323.9 | |
| 0.00 | 2.66 | 0.00 | 2.38 | -14.54 | 221.05 | 56.53 | 255.87 | 0.8348 | 339.0 | 375.8 | |
| 0.00 | 0.62 | 0.00 | 0.56 | -15.63 | 221.04 | 56.52 | 254.57 | 0.8354 | 589.0 | 549.3 | |
| 0.00 | 1.51 | 0.00 | 1.34 | -14.85 | 220.61 | 56.09 | 255.46 | 0.8309 | -433.0 | -336.2 | |
| 0.00 | 1.95 | 0.00 | 1.74 | -15.49 | 220.70 | 56.18 | 254.70 | 0.8322 | 281.0 | 284.2 | |
| 0.00 | 1.24 | 0.00 | 1.10 | -16.34 | 220.60 | 56.09 | 253.67 | 0.8320 | 632.0 | 539.1 | |
| 1.07 | 10.48 | 0.92 | 9.14 | -16.16 | 219.63 | 55.11 | 253.79 | 0.8227 | -464.2 | 199.9 | |
| 0.00 | 1.24 | 0.00 | 1.10 | -17.93 | 220.25 | 55.73 | 251.73 | 0.8302 | 454.0 | 351.4 | |
| 0.00 | 1.07 | 0.00 | 0.92 | -16.46 | 219.37 | 54.85 | 253.40 | 0.8205 | -586.0 | -471.1 | |
| 0.00 | 2.13 | 0.00 | 1.95 | -20.44 | 221.33 | 56.81 | 248.88 | 0.8428 | 65.0 | 183.4 | |
| 0.00 | 1.60 | 0.00 | 1.37 | -16.74 | 219.27 | 54.75 | 253.04 | 0.8198 | -453.0 | -296.4 | |
| 0.71 | 7.28 | 0.61 | 6.31 | -17.05 | 219.35 | 54.83 | 252.67 | 0.8209 | -278.0 | 183.6 | |
| 5.06 | 8.97 | 4.27 | 7.57 | -16.74 | 218.40 | 53.88 | 252.94 | 0.8114 | -585.9 | -418.7 | |
| 0.00 | 1.60 | 0.00 | 1.37 | -19.75 | 218.85 | 54.33 | 249.32 | 0.8194 | -262.0 | -194.2 | |
| 0.00 | 0.80 | 0.00 | 0.67 | -18.31 | 217.79 | 53.27 | 250.92 | 0.8074 | -468.0 | -412.3 | |
| 0.00 | 2.31 | 0.00 | 1.86 | -15.84 | 216.58 | 52.07 | 253.83 | 0.7923 | -560.0 | -522.8 | |
| 0.00 | 0.53 | 0.00 | 0.43 | -15.69 | 216.43 | 51.91 | 253.99 | 0.7905 | -661.0 | -607.5 | |
| 0.00 | 1.69 | 0.00 | 1.39 | -19.15 | 217.10 | 52.59 | 249.78 | 0.8018 | -409.0 | -305.9 | |
| 0.00 | 2.84 | 0.00 | 2.29 | -19.41 | 216.02 | 51.50 | 249.26 | 0.7916 | -220.0 | -209.4 | |
| 0.00 | 0.71 | 0.00 | 0.55 | -19.99 | 213.80 | 49.28 | 248.07 | 0.7701 | -256.0 | -296.4 | |
| 0.00 | 0.71 | 0.00 | 0.55 | -20.01 | 213.46 | 48.95 | 247.96 | 0.7667 | -542.0 | -457.9 | |
| 0.00 | 1.86 | 0.00 | 1.42 | -20.10 | 213.11 | 48.59 | 247.77 | 0.7632 | -676.0 | -583.0 | |
| 0.00 | 1.24 | 0.00 | 0.97 | -22.31 | 213.90 | 49.38 | 245.15 | 0.7762 | -449.0 | -387.1 | |
| 0.00 | 1.33 | 0.00 | 0.96 | -21.93 | 209.13 | 44.61 | 244.26 | 0.7256 | -58.0 | -98.9 | |
| 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. | |