SDO HMI 2014-05-10 06:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.26 | 308.67 | 52.97 | 271.64 | -13.29 | 230.22 | -55.31 | 103.85 | 0.8221 | 277.5 | 132.0 | |
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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 |
| 0.00 | 0.99 | 0.00 | 0.70 | -15.45 | 240.53 | -45.00 | 108.47 | 0.7209 | 602.0 | 553.8 | |
| 0.00 | 1.97 | 0.00 | 1.38 | -11.20 | 240.93 | -44.61 | 102.66 | 0.7083 | 711.0 | 578.2 | |
| 0.00 | 1.08 | 0.00 | 0.77 | -10.36 | 239.86 | -45.67 | 101.33 | 0.7200 | 554.0 | 511.4 | |
| 0.00 | 3.32 | 0.00 | 2.37 | -10.68 | 239.67 | -45.87 | 101.76 | 0.7227 | 714.0 | 530.4 | |
| 0.00 | 1.52 | 0.00 | 1.09 | -10.22 | 239.53 | -46.00 | 101.10 | 0.7237 | 632.0 | 501.8 | |
| 0.00 | 1.34 | 0.00 | 0.96 | -9.52 | 239.66 | -45.87 | 100.15 | 0.7215 | 757.0 | 610.5 | |
| 0.00 | 0.90 | 0.00 | 0.64 | -9.57 | 239.47 | -46.06 | 100.20 | 0.7237 | 723.0 | 609.6 | |
| 0.00 | 0.90 | 0.00 | 0.66 | -10.45 | 237.63 | -47.90 | 101.17 | 0.7461 | 505.0 | 428.3 | |
| 0.00 | 0.45 | 0.00 | 0.33 | -10.06 | 237.20 | -48.33 | 100.61 | 0.7506 | 570.0 | 493.6 | |
| 0.00 | 0.99 | 0.00 | 0.74 | -9.84 | 236.97 | -48.57 | 100.29 | 0.7531 | 569.0 | 433.2 | |
| 31.01 | 149.48 | 24.13 | 116.31 | -11.55 | 235.30 | -50.23 | 102.34 | 0.7732 | 886.3 | 287.3 | |
| 0.00 | 1.17 | 0.00 | 0.92 | -8.69 | 234.56 | -50.97 | 98.59 | 0.7789 | 365.0 | 321.3 | |
| 0.00 | 1.52 | 0.00 | 1.20 | -8.02 | 234.54 | -50.99 | 97.73 | 0.7788 | 469.0 | 500.0 | |
| 0.00 | 0.54 | 0.00 | 0.45 | -14.65 | 232.72 | -52.81 | 105.92 | 0.8037 | 395.0 | 366.2 | |
| 0.00 | 1.52 | 0.00 | 1.20 | -7.77 | 234.44 | -51.10 | 97.40 | 0.7798 | 624.0 | 525.9 | |
| 0.00 | 4.39 | 0.00 | 3.54 | -10.80 | 233.61 | -51.93 | 101.20 | 0.7905 | 687.0 | 491.3 | |
| 0.00 | 5.47 | 0.00 | 4.32 | -7.61 | 234.27 | -51.27 | 97.19 | 0.7816 | 326.0 | 330.9 | |
| 0.00 | 1.08 | 0.00 | 0.87 | -10.87 | 233.19 | -52.35 | 101.25 | 0.7950 | 301.0 | 176.5 | |
| 1.08 | 2.60 | 0.96 | 2.33 | -18.07 | 229.90 | -55.64 | 109.61 | 0.8352 | 532.1 | 439.4 | |
| 0.00 | 0.36 | 0.00 | 0.30 | -11.21 | 232.43 | -53.10 | 101.60 | 0.8030 | 194.0 | 222.0 | |
| 0.00 | 1.34 | 0.00 | 1.11 | -10.56 | 232.50 | -53.04 | 100.81 | 0.8019 | -681.0 | -514.6 | |
| 0.00 | 1.17 | 0.00 | 0.99 | -13.19 | 231.37 | -54.17 | 103.94 | 0.8155 | 638.0 | 474.3 | |
| 0.00 | 1.34 | 0.00 | 1.11 | -9.51 | 232.28 | -53.25 | 99.48 | 0.8034 | 547.0 | 443.4 | |
| 0.00 | 1.34 | 0.00 | 1.10 | -7.29 | 232.52 | -53.01 | 96.72 | 0.8000 | -637.0 | -571.5 | |
| 0.00 | 2.51 | 0.00 | 2.08 | -8.56 | 232.23 | -53.30 | 98.29 | 0.8035 | -104.0 | -48.2 | |
| 0.00 | 1.34 | 0.00 | 1.12 | -9.47 | 232.03 | -53.50 | 99.41 | 0.8059 | 248.0 | 210.4 | |
| 0.00 | 1.25 | 0.00 | 1.08 | -13.51 | 230.83 | -54.70 | 104.27 | 0.8210 | 404.0 | 287.0 | |
| 0.00 | 0.90 | 0.00 | 0.77 | -13.11 | 230.96 | -54.57 | 103.80 | 0.8193 | 418.0 | 388.9 | |
| 0.00 | 0.90 | 0.00 | 0.77 | -12.87 | 231.04 | -54.49 | 103.51 | 0.8183 | 433.0 | 350.8 | |
| 0.00 | 1.52 | 0.00 | 1.40 | -18.02 | 228.88 | -56.65 | 109.39 | 0.8442 | -241.0 | -185.2 | |
| 0.00 | 1.88 | 0.00 | 1.54 | -4.59 | 232.70 | -52.84 | 93.33 | 0.7979 | 427.0 | 276.2 | |
| 0.00 | 1.25 | 0.00 | 1.04 | -7.22 | 232.18 | -53.36 | 96.61 | 0.8036 | -600.0 | -484.9 | |
| 0.00 | 1.25 | 0.00 | 1.06 | -7.42 | 231.26 | -54.28 | 96.83 | 0.8130 | -718.0 | -556.6 | |
| 1.25 | 2.33 | 1.07 | 1.99 | -8.17 | 230.95 | -54.58 | 97.74 | 0.8163 | -528.8 | -467.2 | |
| 0.00 | 1.88 | 0.00 | 1.66 | -11.18 | 229.82 | -55.71 | 101.34 | 0.8288 | -227.0 | -261.0 | |
| 0.00 | 0.54 | 0.00 | 0.48 | -10.92 | 229.57 | -55.97 | 101.01 | 0.8311 | -685.0 | -612.0 | |
| 0.00 | 0.45 | 0.00 | 0.40 | -11.10 | 229.40 | -56.13 | 101.21 | 0.8328 | -537.0 | -497.6 | |
| 0.00 | 0.72 | 0.00 | 0.64 | -10.88 | 229.30 | -56.23 | 100.94 | 0.8336 | -365.0 | -330.4 | |
| 0.00 | 1.43 | 0.00 | 1.31 | -11.79 | 228.45 | -57.08 | 101.97 | 0.8421 | -609.0 | -534.4 | |
| 0.00 | 1.08 | 0.00 | 0.98 | -11.66 | 228.32 | -57.21 | 101.81 | 0.8432 | -494.0 | -425.6 | |
| 2.06 | 3.76 | 2.07 | 3.79 | -17.04 | 225.43 | -60.11 | 107.78 | 0.8725 | 421.0 | 343.4 | |
| 0.00 | 1.25 | 0.00 | 1.17 | -11.14 | 227.68 | -57.86 | 101.15 | 0.8488 | -480.0 | -391.4 | |
| 3.76 | 5.65 | 4.02 | 6.02 | -18.76 | 223.68 | -61.85 | 109.53 | 0.8877 | -500.8 | -318.4 | |
| 0.00 | 2.06 | 0.00 | 2.07 | -15.84 | 225.35 | -60.19 | 106.41 | 0.8721 | -324.0 | -286.3 | |
| 0.63 | 1.88 | 0.62 | 1.86 | -14.24 | 225.79 | -59.75 | 104.61 | 0.8673 | 287.6 | 179.6 | |
| 1.34 | 14.52 | 1.35 | 14.68 | -15.15 | 225.24 | -60.29 | 105.60 | 0.8724 | -703.5 | -416.0 | |
| 0.00 | 1.17 | 0.00 | 1.18 | -15.57 | 224.97 | -60.57 | 106.06 | 0.8750 | -517.0 | -461.8 | |
| 0.90 | -46.00 | 0.92 | -46.00 | -15.37 | 224.74 | -60.79 | 105.81 | 0.8767 | -360.7 | 999999 | |
| 0.00 | 1.08 | 0.00 | 1.11 | -14.86 | 224.41 | -61.12 | 105.19 | 0.8790 | -553.0 | -477.7 | |
| 10.31 | 55.92 | 11.28 | 61.38 | -17.13 | 222.70 | -62.84 | 107.59 | 0.8938 | 603.2 | 94.9 | |
| 0.00 | 0.99 | 0.00 | 1.03 | -14.77 | 223.99 | -61.54 | 105.06 | 0.8823 | -307.0 | -300.2 | |
| 0.00 | 0.72 | 0.00 | 0.77 | -15.41 | 222.99 | -62.55 | 105.70 | 0.8905 | -331.0 | -322.2 | |
| 0.00 | 1.08 | 0.00 | 1.18 | -14.32 | 222.38 | -63.15 | 104.43 | 0.8945 | -535.0 | -479.3 | |
| 4.93 | 7.26 | 5.46 | 8.03 | -14.59 | 222.17 | -63.37 | 104.72 | 0.8962 | -440.0 | -359.5 | |
| 0.99 | 3.32 | 1.09 | 3.66 | -13.63 | 222.17 | -63.37 | 103.64 | 0.8958 | -414.8 | -458.1 | |
| 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. | |