| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 169.13 | 781.60 | 87.37 | 404.07 | 8.98 | 99.91 | -10.55 | 39.08 | 0.2861 | 236.5 | 100.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-01-07 00:00:24 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 | 0.93 | 0.00 | 0.48 | 8.85 | 105.42 | -5.03 | 21.77 | 0.2347 | -152.0 | -131.5 | |
| 11.81 | 69.91 | 6.01 | 35.59 | 8.61 | 105.10 | -5.36 | 23.44 | 0.2331 | -1259.1 | -470.8 | |
| 10.96 | -2.00 | 5.58 | -2.00 | 8.47 | 104.71 | -5.74 | 25.21 | 0.2335 | -1248.1 | 999999 | |
| 0.00 | 1.61 | 0.00 | 0.82 | 7.65 | 104.57 | -5.88 | 27.35 | 0.2221 | -733.0 | -461.3 | |
| 0.00 | 3.40 | 0.00 | 1.73 | 8.32 | 104.23 | -6.22 | 27.30 | 0.2348 | -1061.0 | -760.3 | |
| 3.74 | 10.11 | 1.91 | 5.16 | 8.59 | 104.11 | -6.34 | 27.23 | 0.2399 | -1055.6 | -714.2 | |
| 0.00 | 4.33 | 0.00 | 2.20 | 7.66 | 103.91 | -6.54 | 29.89 | 0.2276 | -1215.0 | -954.0 | |
| 0.00 | 0.85 | 0.00 | 0.43 | 7.63 | 103.68 | -6.78 | 30.85 | 0.2292 | -1001.0 | -883.4 | |
| 0.00 | 2.38 | 0.00 | 1.21 | 7.81 | 103.64 | -6.81 | 30.56 | 0.2321 | -859.0 | -723.3 | |
| 1.87 | 97.78 | 0.96 | 50.21 | 8.67 | 102.43 | -8.03 | 32.90 | 0.2553 | -1142.9 | -685.2 | |
| 0.00 | 6.97 | 0.00 | 3.56 | 7.76 | 102.38 | -8.07 | 35.09 | 0.2431 | -1028.0 | -849.7 | |
| 2.55 | -10.00 | 1.31 | -10.00 | 9.30 | 102.29 | -8.16 | 32.00 | 0.2656 | -1016.5 | 999999 | |
| 2.63 | -10.00 | 1.35 | -10.00 | 8.94 | 102.18 | -8.27 | 33.10 | 0.2615 | -1064.2 | 999999 | |
| 1.53 | 10.70 | 0.78 | 5.48 | 8.07 | 102.02 | -8.44 | 35.57 | 0.2509 | -1127.2 | -757.8 | |
| 4.84 | -10.00 | 2.49 | -10.00 | 9.22 | 101.93 | -8.52 | 33.30 | 0.2676 | -1108.6 | 999999 | |
| 0.00 | 1.61 | 0.00 | 0.83 | 8.61 | 101.82 | -8.63 | 34.93 | 0.2603 | -1063.0 | -840.3 | |
| 10.53 | -10.00 | 5.42 | -10.00 | 9.43 | 101.69 | -8.77 | 33.61 | 0.2729 | -991.2 | 999999 | |
| 0.34 | -14.00 | 0.17 | -14.00 | 8.16 | 101.59 | -8.86 | 36.68 | 0.2564 | -884.0 | 999999 | |
| 5.44 | 72.38 | 2.79 | 37.15 | 8.56 | 101.13 | -9.32 | 37.15 | 0.2664 | -1027.9 | -219.9 | |
| 9.60 | -19.00 | 4.93 | -19.00 | 8.26 | 101.14 | -9.31 | 37.83 | 0.2623 | -967.6 | 999999 | |
| 0.00 | 0.68 | 0.00 | 0.35 | 7.57 | 100.88 | -9.57 | 40.29 | 0.2560 | 640.0 | 489.6 | |
| 2.12 | -19.00 | 1.09 | -19.00 | 7.87 | 100.76 | -9.70 | 39.90 | 0.2613 | 971.3 | 999999 | |
| 0.00 | 1.70 | 0.00 | 0.88 | 9.45 | 100.41 | -10.04 | 37.23 | 0.2855 | 946.0 | 742.2 | |
| 0.00 | 1.95 | 0.00 | 1.01 | 8.91 | 99.58 | -10.88 | 40.65 | 0.2874 | 522.0 | 386.4 | |
| 3.31 | 493.46 | 1.72 | 256.53 | 9.28 | 99.32 | -11.13 | 40.47 | 0.2948 | 1058.6 | 435.4 | |
| 5.18 | -25.00 | 2.68 | -25.00 | 8.32 | 99.23 | -11.22 | 42.96 | 0.2839 | 303.6 | 999999 | |
| 3.23 | -25.00 | 1.68 | -25.00 | 9.80 | 99.03 | -11.42 | 40.06 | 0.3045 | 1016.4 | 999999 | |
| 5.86 | -25.00 | 3.04 | -25.00 | 9.10 | 98.96 | -11.49 | 41.77 | 0.2966 | 1110.8 | 999999 | |
| 3.06 | -25.00 | 1.58 | -25.00 | 8.59 | 98.95 | -11.50 | 43.01 | 0.2904 | 1195.9 | 999999 | |
| 0.68 | -25.00 | 0.35 | -25.00 | 8.74 | 98.79 | -11.66 | 43.03 | 0.2941 | 1246.5 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 11.20 | 98.58 | -11.87 | 38.28 | 0.3272 | 801.0 | 676.8 | |
| 5.35 | -25.00 | 2.78 | -25.00 | 9.41 | 98.47 | -11.99 | 42.28 | 0.3059 | 1015.3 | 999999 | |
| 3.31 | -25.00 | 1.73 | -25.00 | 9.72 | 98.36 | -12.09 | 41.85 | 0.3108 | 925.4 | 999999 | |
| 36.19 | -25.00 | 18.79 | -25.00 | 8.99 | 98.36 | -12.10 | 43.50 | 0.3021 | 1486.1 | 999999 | |
| 3.14 | -25.00 | 1.64 | -25.00 | 9.93 | 98.11 | -12.34 | 41.97 | 0.3163 | 272.3 | 999999 | |
| 31.86 | -25.00 | 16.59 | -25.00 | 9.30 | 97.89 | -12.56 | 43.87 | 0.3111 | 1273.9 | 999999 | |
| 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. | |