SDO HMI 2014-07-04 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 235.00 | 1152.00 | 211.38 | 1029.65 | -7.71 | 219.20 | -55.24 | 101.56 | 0.8319 | 189.1 | -18.4 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.54 | 5.63 | 2.78 | 4.42 | -5.65 | 224.27 | -50.16 | 99.96 | 0.7780 | 642.4 | 452.9 | |
| 0.00 | 0.73 | 0.00 | 0.57 | -5.82 | 224.01 | -50.42 | 100.12 | 0.7811 | 257.0 | 251.4 | |
| 0.00 | 1.27 | 0.00 | 1.02 | -6.58 | 223.47 | -50.96 | 100.98 | 0.7882 | 426.0 | 404.1 | |
| 1.64 | 653.26 | 1.35 | 551.22 | -8.82 | 222.49 | -51.95 | 103.55 | 0.8026 | 837.9 | 214.9 | |
| 2.63 | -4.00 | 2.20 | -4.00 | -9.00 | 221.99 | -52.44 | 103.65 | 0.8079 | 669.8 | 999999 | |
| 1.54 | -4.00 | 1.29 | -4.00 | -8.81 | 222.03 | -52.40 | 103.43 | 0.8071 | 747.8 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.78 | -10.28 | 221.40 | -53.04 | 105.05 | 0.8163 | -178.0 | -153.1 | |
| 119.37 | -4.00 | 100.26 | -4.00 | -8.18 | 221.70 | -52.73 | 102.58 | 0.8093 | 911.7 | 999999 | |
| 2.45 | -4.00 | 2.06 | -4.00 | -7.40 | 221.64 | -52.79 | 101.62 | 0.8085 | 683.2 | 999999 | |
| 3.54 | 7.54 | 2.92 | 6.22 | -5.20 | 221.91 | -52.52 | 98.96 | 0.8022 | -583.6 | -395.9 | |
| 0.00 | 1.54 | 0.00 | 1.35 | -9.74 | 220.21 | -54.22 | 104.13 | 0.8267 | -275.0 | -218.3 | |
| 0.00 | 0.91 | 0.00 | 0.81 | -10.75 | 219.90 | -54.53 | 105.27 | 0.8315 | 547.0 | 383.8 | |
| 1.27 | 10.36 | 1.15 | 9.38 | -10.35 | 219.08 | -55.35 | 104.61 | 0.8384 | 408.7 | 206.1 | |
| 1.82 | -13.00 | 1.65 | -13.00 | -10.24 | 218.84 | -55.59 | 104.42 | 0.8404 | 242.5 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.72 | -7.88 | 219.39 | -55.04 | 101.75 | 0.8313 | 297.0 | 261.2 | |
| 0.00 | 1.27 | 0.00 | 1.13 | -7.48 | 219.36 | -55.07 | 101.26 | 0.8309 | 262.0 | 222.0 | |
| 0.00 | 0.55 | 0.00 | 0.48 | -5.68 | 219.51 | -54.93 | 99.14 | 0.8270 | -467.0 | -436.5 | |
| 1.00 | 4.45 | 0.91 | 4.04 | -8.94 | 218.61 | -55.82 | 102.85 | 0.8403 | -694.1 | -534.3 | |
| 0.00 | 1.73 | 0.00 | 1.56 | -8.37 | 218.74 | -55.69 | 102.21 | 0.8382 | -360.0 | -214.2 | |
| 12.54 | 180.78 | 11.24 | 165.60 | -7.47 | 218.88 | -55.56 | 101.16 | 0.8356 | 572.6 | -204.0 | |
| 1.54 | -20.00 | 1.38 | -20.00 | -6.38 | 218.91 | -55.52 | 99.88 | 0.8337 | 544.5 | 999999 | |
| 1.18 | -20.00 | 1.06 | -20.00 | -6.73 | 218.79 | -55.64 | 100.27 | 0.8353 | 536.2 | 999999 | |
| 0.00 | 1.91 | 0.00 | 1.80 | -11.20 | 217.72 | -56.71 | 105.30 | 0.8521 | -548.0 | -562.6 | |
| 0.82 | 2.27 | 0.78 | 2.16 | -11.25 | 217.42 | -57.01 | 105.28 | 0.8549 | -664.3 | -590.3 | |
| 0.45 | 1.73 | 0.42 | 1.59 | -8.68 | 218.12 | -56.31 | 102.45 | 0.8444 | -663.0 | -627.4 | |
| 0.00 | 2.18 | 0.00 | 2.04 | -10.04 | 217.72 | -56.72 | 103.95 | 0.8502 | -63.0 | -177.9 | |
| 0.00 | 1.82 | 0.00 | 1.72 | -10.40 | 217.33 | -57.10 | 104.29 | 0.8543 | 178.0 | 143.6 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -9.23 | 217.65 | -56.79 | 103.00 | 0.8496 | -633.0 | -619.7 | |
| 0.00 | 2.36 | 0.00 | 2.27 | -11.14 | 216.93 | -57.50 | 105.06 | 0.8589 | -581.0 | -517.4 | |
| 0.00 | 0.91 | 0.00 | 0.85 | -9.06 | 217.46 | -56.97 | 102.76 | 0.8509 | -436.0 | -411.9 | |
| 1.00 | -20.00 | 0.91 | -20.00 | -6.37 | 217.97 | -56.46 | 99.70 | 0.8425 | 164.1 | 999999 | |
| 1.00 | 2.82 | 0.95 | 2.67 | -9.72 | 217.17 | -57.26 | 103.48 | 0.8545 | -629.5 | -566.7 | |
| 0.00 | 0.55 | 0.00 | 0.51 | -8.88 | 217.16 | -57.27 | 102.50 | 0.8534 | -554.0 | -427.3 | |
| 1.36 | 4.81 | 1.32 | 4.68 | -11.04 | 216.50 | -57.94 | 104.85 | 0.8625 | -615.5 | -512.9 | |
| 1.27 | -20.00 | 1.18 | -20.00 | -7.13 | 217.44 | -57.00 | 100.51 | 0.8484 | 245.4 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.35 | -11.91 | 216.09 | -58.34 | 105.75 | 0.8674 | -337.0 | -237.6 | |
| 0.00 | 0.27 | 0.00 | 0.26 | -9.72 | 216.65 | -57.78 | 103.37 | 0.8591 | -560.0 | -546.7 | |
| 0.00 | 6.72 | 0.00 | 6.38 | -7.04 | 216.71 | -57.72 | 100.29 | 0.8548 | -372.0 | -372.9 | |
| 5.00 | 199.86 | 4.84 | 199.43 | -8.71 | 216.27 | -58.16 | 102.13 | 0.8609 | -666.3 | -509.1 | |
| 0.00 | 1.54 | 0.00 | 1.48 | -6.60 | 216.27 | -58.16 | 99.70 | 0.8582 | -448.0 | -464.6 | |
| 5.09 | -20.00 | 4.87 | -20.00 | -5.96 | 216.21 | -58.22 | 98.95 | 0.8579 | -817.3 | 999999 | |
| 0.45 | 1.36 | 0.45 | 1.36 | -8.36 | 215.23 | -59.20 | 101.55 | 0.8694 | -331.8 | -277.3 | |
| 16.99 | -39.00 | 16.97 | -39.00 | -7.81 | 215.06 | -59.37 | 100.89 | 0.8701 | -711.4 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.27 | -8.22 | 214.83 | -59.60 | 101.32 | 0.8725 | -298.0 | -313.0 | |
| 0.00 | 8.09 | 0.00 | 7.93 | -5.50 | 215.34 | -59.09 | 98.30 | 0.8651 | -439.0 | -479.8 | |
| 0.00 | 1.00 | 0.00 | 0.98 | -4.95 | 215.43 | -59.01 | 97.67 | 0.8637 | -641.0 | -595.8 | |
| 0.00 | 0.27 | 0.00 | 0.27 | -6.25 | 215.14 | -59.29 | 99.13 | 0.8676 | -572.0 | -544.3 | |
| 22.80 | -39.00 | 22.97 | -39.00 | -6.74 | 214.62 | -59.81 | 99.61 | 0.8726 | -803.2 | 999999 | |
| 1.18 | -39.00 | 1.18 | -39.00 | -6.25 | 214.66 | -59.77 | 99.05 | 0.8717 | -685.5 | 999999 | |
| 0.55 | 1.73 | 0.56 | 1.76 | -7.97 | 214.28 | -60.15 | 100.95 | 0.8768 | -304.2 | -187.5 | |
| 0.00 | 0.27 | 0.00 | 0.28 | -7.79 | 214.07 | -60.36 | 100.72 | 0.8783 | -259.0 | -232.0 | |
| 18.71 | -39.00 | 19.23 | -39.00 | -6.35 | 213.89 | -60.54 | 99.05 | 0.8782 | -512.3 | 999999 | |
| 0.00 | 1.45 | 0.00 | 1.54 | -6.91 | 213.07 | -61.36 | 99.57 | 0.8855 | -201.0 | -164.2 | |
| 4.27 | 34.43 | 4.50 | 36.52 | -6.26 | 213.08 | -61.35 | 98.85 | 0.8847 | -325.1 | 131.1 | |
| 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. | |