SDO HMI 2014-05-27 08:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.68 | 150.69 | 21.18 | 76.50 | -12.80 | 62.75 | 3.18 | 195.03 | 0.2167 | 112.5 | 79.9 | |
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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 | 1.17 | 0.00 | 0.59 | -8.31 | 68.45 | 8.88 | 231.06 | 0.1972 | 853.0 | 668.2 | |
| 0.00 | 7.22 | 0.00 | 3.66 | -10.55 | 67.44 | 7.87 | 219.72 | 0.2116 | 578.0 | 836.9 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -9.36 | 67.26 | 7.69 | 223.03 | 0.1943 | 910.0 | 720.2 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -15.24 | 67.21 | 7.63 | 207.89 | 0.2751 | 794.0 | 615.1 | |
| 7.13 | 10.02 | 3.64 | 5.11 | -13.06 | 67.10 | 7.53 | 211.92 | 0.2426 | 1053.1 | 793.2 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -13.12 | 66.82 | 7.25 | 210.81 | 0.2410 | 798.0 | 678.3 | |
| 0.63 | 5.59 | 0.32 | 2.85 | -12.81 | 66.69 | 7.11 | 211.04 | 0.2353 | 1144.0 | 895.6 | |
| 0.00 | 0.72 | 0.00 | 0.36 | -4.90 | 66.54 | 6.97 | 242.13 | 0.1374 | -697.0 | -490.2 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -10.74 | 66.29 | 6.72 | 214.84 | 0.2022 | 748.0 | 688.9 | |
| 1.53 | 2.98 | 0.80 | 1.55 | -17.73 | 66.43 | 6.86 | 201.84 | 0.3073 | 968.7 | 775.2 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -15.21 | 66.35 | 6.77 | 205.23 | 0.2682 | 825.0 | 648.0 | |
| 6.68 | 9.84 | 3.40 | 5.00 | -12.53 | 66.09 | 6.51 | 209.47 | 0.2261 | 1167.4 | 813.5 | |
| 0.00 | 1.71 | 0.00 | 0.86 | -9.82 | 65.97 | 6.39 | 216.31 | 0.1861 | 965.0 | 721.1 | |
| 0.00 | 2.62 | 0.00 | 1.31 | -6.36 | 65.79 | 6.22 | 230.30 | 0.1406 | -870.0 | -653.2 | |
| 0.00 | 3.34 | 0.00 | 1.71 | -14.83 | 65.33 | 5.75 | 202.39 | 0.2555 | 926.0 | 865.2 | |
| 0.00 | 1.35 | 0.00 | 0.70 | -17.86 | 65.19 | 5.61 | 198.03 | 0.3021 | -939.0 | -732.7 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -13.21 | 65.00 | 5.43 | 203.94 | 0.2281 | 775.0 | 594.6 | |
| 0.00 | 1.71 | 0.00 | 0.88 | -14.49 | 65.00 | 5.43 | 201.77 | 0.2480 | 926.0 | 684.3 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -13.49 | 64.82 | 5.25 | 202.73 | 0.2313 | 1016.0 | 821.4 | |
| 0.00 | 1.26 | 0.00 | 0.65 | -15.55 | 64.43 | 4.85 | 198.24 | 0.2616 | 733.0 | 558.3 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -12.63 | 64.30 | 4.73 | 202.17 | 0.2142 | 843.0 | 626.2 | |
| 0.00 | 1.80 | 0.00 | 0.91 | -11.20 | 64.25 | 4.68 | 204.80 | 0.1916 | 817.0 | 653.2 | |
| 0.00 | 3.79 | 0.00 | 1.92 | -12.53 | 63.21 | 3.64 | 197.55 | 0.2064 | 747.0 | 680.8 | |
| 6.68 | 12.36 | 3.37 | 6.25 | -12.01 | 62.99 | 3.41 | 197.31 | 0.1966 | 1135.2 | 799.1 | |
| 0.63 | -24.00 | 0.32 | -24.00 | -12.04 | 62.74 | 3.17 | 196.08 | 0.1959 | 969.4 | 999999 | |
| 0.90 | 2.35 | 0.46 | 1.18 | -11.91 | 62.55 | 2.98 | 195.34 | 0.1930 | 1047.9 | 838.9 | |
| 0.90 | 3.70 | 0.45 | 1.86 | -11.51 | 62.39 | 2.82 | 195.12 | 0.1856 | 1194.1 | 840.7 | |
| 0.00 | 1.80 | 0.00 | 0.91 | -12.04 | 62.24 | 2.67 | 193.65 | 0.1937 | 775.0 | 588.7 | |
| 0.00 | 0.72 | 0.00 | 0.38 | -18.94 | 62.13 | 2.56 | 187.90 | 0.3083 | 912.0 | 741.2 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -11.20 | 62.02 | 2.44 | 193.59 | 0.1788 | 850.0 | 708.2 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -13.43 | 61.79 | 2.21 | 190.08 | 0.2155 | 975.0 | 795.2 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -11.42 | 61.55 | 1.98 | 190.85 | 0.1808 | 984.0 | 806.3 | |
| 3.34 | 9.75 | 1.68 | 4.91 | -11.82 | 60.66 | 1.08 | 185.75 | 0.1854 | -1123.8 | -780.7 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -13.68 | 60.51 | 0.93 | 184.20 | 0.2170 | -866.0 | -625.3 | |
| 1.35 | 3.34 | 0.69 | 1.70 | -14.08 | 60.32 | 0.75 | 183.25 | 0.2237 | -1166.9 | -957.7 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -14.62 | 60.23 | 0.65 | 182.73 | 0.2326 | -858.0 | -760.7 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -11.36 | 60.00 | 0.43 | 182.40 | 0.1766 | -763.0 | -551.1 | |
| 0.00 | 1.89 | 0.00 | 0.96 | -13.77 | 59.88 | 0.31 | 181.37 | 0.2180 | -1130.0 | -844.3 | |
| 0.45 | 5.32 | 0.23 | 2.71 | -14.68 | 59.85 | 0.28 | 181.15 | 0.2335 | -984.2 | -846.3 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -13.24 | 59.69 | 0.12 | 180.56 | 0.2089 | -739.0 | -666.4 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -13.49 | 59.35 | -0.22 | 178.97 | 0.2132 | -985.0 | -822.0 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -11.85 | 59.35 | -0.22 | 178.83 | 0.1850 | -1029.0 | -770.8 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -14.43 | 59.32 | -0.26 | 178.91 | 0.2292 | -785.0 | -666.4 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -14.96 | 59.25 | -0.32 | 178.69 | 0.2383 | -913.0 | -791.4 | |
| 0.00 | 2.44 | 0.00 | 1.23 | -12.72 | 59.26 | -0.32 | 178.45 | 0.1999 | -898.0 | -831.9 | |
| 0.99 | 2.44 | 0.50 | 1.23 | -13.37 | 59.16 | -0.41 | 178.10 | 0.2112 | -1138.1 | -905.2 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -12.81 | 59.04 | -0.53 | 177.40 | 0.2017 | -1047.0 | -906.3 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -12.62 | 59.04 | -0.53 | 177.36 | 0.1985 | -900.0 | -685.1 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -13.12 | 58.98 | -0.60 | 177.18 | 0.2070 | -959.0 | -791.4 | |
| 0.00 | 3.07 | 0.00 | 1.55 | -12.56 | 58.85 | -0.72 | 176.42 | 0.1976 | -1194.0 | -880.5 | |
| 7.04 | 14.53 | 3.58 | 7.38 | -13.96 | 57.72 | -1.85 | 171.89 | 0.2234 | -1138.5 | -759.8 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -13.18 | 57.70 | -1.88 | 171.24 | 0.2103 | -999.0 | -701.9 | |
| 3.43 | -51.00 | 1.74 | -51.00 | -13.93 | 57.53 | -2.04 | 171.06 | 0.2233 | -1011.5 | 999999 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -12.56 | 57.55 | -2.03 | 170.02 | 0.2002 | -921.0 | -707.8 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -12.62 | 57.33 | -2.25 | 169.03 | 0.2019 | -845.0 | -678.9 | |
| 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. | |