| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89.59 | 450.88 | 47.07 | 237.13 | -10.73 | 265.50 | 5.98 | 199.37 | 0.3355 | 315.1 | 91.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-25 08:00:34 UT
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 | 2.21 | 0.00 | 1.27 | -18.03 | 276.54 | 17.03 | 213.71 | 0.5037 | 564.0 | 503.0 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -9.59 | 273.55 | 14.04 | 220.38 | 0.3707 | 672.0 | 425.9 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -10.43 | 273.28 | 13.76 | 218.38 | 0.3784 | 714.0 | 592.7 | |
| 0.00 | 1.50 | 0.00 | 0.80 | -10.45 | 272.93 | 13.41 | 217.63 | 0.3752 | 793.0 | 616.8 | |
| 0.00 | 1.24 | 0.00 | 0.65 | -8.53 | 272.70 | 13.18 | 220.52 | 0.3486 | 849.0 | 750.6 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -10.13 | 272.70 | 13.18 | 217.68 | 0.3688 | 679.0 | 500.4 | |
| 0.00 | 0.80 | 0.00 | 0.43 | -11.23 | 272.62 | 13.10 | 215.74 | 0.3823 | 722.0 | 613.2 | |
| 0.00 | 1.42 | 0.00 | 0.74 | -7.14 | 271.85 | 12.33 | 221.36 | 0.3221 | -771.0 | -549.9 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -6.18 | 271.79 | 12.28 | 223.28 | 0.3097 | 562.0 | 393.3 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -14.72 | 271.47 | 11.95 | 208.63 | 0.4196 | 788.0 | 642.0 | |
| 19.19 | 150.70 | 10.06 | 78.99 | -8.60 | 270.62 | 11.10 | 215.60 | 0.3284 | 1317.3 | 382.0 | |
| 15.83 | -11.00 | 8.29 | -11.00 | -8.68 | 270.25 | 10.73 | 214.53 | 0.3261 | 1319.7 | 999999 | |
| 1.59 | -11.00 | 0.83 | -11.00 | -8.34 | 270.21 | 10.69 | 215.04 | 0.3210 | 1181.7 | 999999 | |
| 0.00 | 1.95 | 0.00 | 0.99 | -3.21 | 269.66 | 10.14 | 225.20 | 0.2488 | 763.0 | 541.9 | |
| 0.00 | 1.24 | 0.00 | 0.70 | -20.13 | 270.16 | 10.64 | 200.93 | 0.4873 | 741.0 | 557.4 | |
| 0.00 | 1.95 | 0.00 | 1.02 | -8.54 | 269.50 | 9.98 | 212.87 | 0.3173 | 827.0 | 618.1 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -8.10 | 269.21 | 9.70 | 212.88 | 0.3085 | 960.0 | 778.5 | |
| 16.45 | 36.97 | 8.59 | 19.30 | -9.00 | 268.99 | 9.47 | 210.75 | 0.3193 | 1159.3 | 813.8 | |
| 0.97 | 3.98 | 0.51 | 2.09 | -9.65 | 268.85 | 9.33 | 209.36 | 0.3275 | 952.9 | 697.5 | |
| 0.00 | 2.12 | 0.00 | 1.08 | -1.69 | 268.58 | 9.06 | 226.61 | 0.2176 | 842.0 | 695.5 | |
| 0.00 | 1.59 | 0.00 | 0.83 | -7.77 | 268.62 | 9.10 | 211.81 | 0.2987 | 953.0 | 750.5 | |
| 2.30 | -18.00 | 1.20 | -18.00 | -8.58 | 268.58 | 9.06 | 210.31 | 0.3099 | 1255.1 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.42 | -10.37 | 268.62 | 9.11 | 207.72 | 0.3361 | 698.0 | 593.7 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -1.57 | 268.46 | 8.94 | 226.64 | 0.2146 | 910.0 | 678.1 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -8.83 | 268.55 | 9.03 | 209.84 | 0.3133 | 962.0 | 782.4 | |
| 0.00 | 1.42 | 0.00 | 0.75 | -10.91 | 268.61 | 9.09 | 206.94 | 0.3439 | 794.0 | 534.3 | |
| 1.68 | 15.65 | 0.88 | 8.17 | -9.27 | 268.53 | 9.01 | 209.09 | 0.3194 | 1021.3 | 628.8 | |
| 0.00 | 2.74 | 0.00 | 1.44 | -9.65 | 268.54 | 9.02 | 208.55 | 0.3250 | 797.0 | 599.6 | |
| 0.00 | 3.54 | 0.00 | 1.84 | -8.02 | 268.47 | 8.95 | 210.96 | 0.3009 | 874.0 | 769.6 | |
| 0.00 | 2.21 | 0.00 | 1.15 | -8.42 | 268.33 | 8.81 | 209.88 | 0.3055 | 857.0 | 739.0 | |
| 0.00 | 16.89 | 0.00 | 8.78 | -8.60 | 267.90 | 8.38 | 208.38 | 0.3046 | 496.0 | 580.1 | |
| 0.00 | 3.01 | 0.00 | 1.60 | -12.82 | 267.58 | 8.06 | 202.07 | 0.3654 | 385.0 | 257.0 | |
| 0.00 | 1.59 | 0.00 | 0.82 | -8.36 | 266.61 | 7.09 | 204.89 | 0.2914 | -866.0 | -759.7 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -16.19 | 265.90 | 6.38 | 195.22 | 0.4083 | 694.0 | 502.2 | |
| 0.00 | 2.39 | 0.00 | 1.23 | -8.11 | 264.37 | 4.86 | 197.90 | 0.2738 | 925.0 | 721.7 | |
| 0.00 | 1.95 | 0.00 | 1.01 | -9.73 | 264.21 | 4.69 | 195.71 | 0.2992 | -918.0 | -803.1 | |
| 0.00 | 2.21 | 0.00 | 1.14 | -9.10 | 263.74 | 4.23 | 194.76 | 0.2869 | -839.0 | -707.7 | |
| 0.00 | 1.50 | 0.00 | 0.78 | -9.75 | 263.05 | 3.53 | 191.93 | 0.2949 | -791.0 | -636.7 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -11.58 | 262.88 | 3.37 | 190.26 | 0.3242 | -768.0 | -517.9 | |
| 0.00 | 1.86 | 0.00 | 0.97 | -10.94 | 262.36 | 2.84 | 188.99 | 0.3123 | -877.0 | -739.2 | |
| 0.00 | 4.07 | 0.00 | 2.12 | -11.16 | 262.14 | 2.62 | 188.22 | 0.3154 | -969.0 | -740.4 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -14.61 | 260.81 | 1.29 | 183.39 | 0.3697 | -752.0 | -563.0 | |
| 0.00 | 1.24 | 0.00 | 0.66 | -14.83 | 259.84 | 0.32 | 180.85 | 0.3728 | 660.0 | 545.1 | |
| 0.80 | 2.74 | 0.43 | 1.47 | -15.55 | 259.69 | 0.17 | 180.43 | 0.3844 | 945.2 | 830.3 | |
| 2.21 | 152.65 | 1.17 | 80.82 | -13.70 | 259.16 | -0.36 | 179.02 | 0.3544 | -1185.5 | -442.5 | |
| 10.79 | -45.00 | 5.70 | -45.00 | -13.45 | 259.10 | -0.42 | 178.84 | 0.3502 | -1446.4 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -15.09 | 258.97 | -0.55 | 178.59 | 0.3771 | -820.0 | -611.7 | |
| 14.77 | -45.00 | 7.83 | -45.00 | -13.86 | 258.94 | -0.57 | 178.43 | 0.3571 | -1181.2 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -12.04 | 258.92 | -0.60 | 178.20 | 0.3270 | -672.0 | -474.6 | |
| 1.68 | 3.63 | 0.88 | 1.90 | -11.75 | 258.68 | -0.84 | 177.43 | 0.3225 | -1015.2 | -788.6 | |
| 0.80 | 2.21 | 0.42 | 1.15 | -11.47 | 258.37 | -1.15 | 176.44 | 0.3180 | -976.6 | -754.8 | |
| 0.00 | 1.68 | 0.00 | 0.90 | -16.01 | 258.34 | -1.18 | 177.10 | 0.3922 | -930.0 | -664.5 | |
| 0.53 | 2.48 | 0.28 | 1.30 | -11.69 | 257.79 | -1.73 | 174.71 | 0.3224 | -967.2 | -770.0 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -12.94 | 257.74 | -1.77 | 174.93 | 0.3430 | 894.0 | 711.8 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |