SDO HMI 2014-07-05 18:00:40 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.70 | 116.57 | 13.31 | 62.62 | 11.36 | 279.09 | 21.22 | 292.32 | 0.3861 | -345.0 | -374.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-05 18:00:40 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 | 2.36 | 0.00 | 1.30 | 11.78 | 282.52 | 24.64 | 290.40 | 0.4373 | -724.0 | -575.5 | |
| 0.00 | 5.99 | 0.00 | 3.28 | 11.33 | 282.03 | 24.15 | 289.72 | 0.4280 | -737.0 | -697.4 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 12.75 | 282.13 | 24.26 | 292.78 | 0.4364 | -595.0 | -504.1 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 10.60 | 281.69 | 23.82 | 288.27 | 0.4198 | -938.0 | -812.8 | |
| 0.00 | 2.45 | 0.00 | 1.34 | 10.38 | 281.68 | 23.80 | 287.78 | 0.4186 | -917.0 | -713.4 | |
| 0.00 | 0.91 | 0.00 | 0.51 | 16.14 | 282.15 | 24.28 | 299.81 | 0.4571 | -708.0 | -563.0 | |
| 0.00 | 5.54 | 0.00 | 3.01 | 10.17 | 281.42 | 23.55 | 287.45 | 0.4139 | -877.0 | -748.6 | |
| 0.00 | 3.99 | 0.00 | 2.15 | 8.23 | 280.48 | 22.60 | 283.25 | 0.3925 | -870.0 | -701.1 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 7.08 | 280.38 | 22.50 | 280.35 | 0.3878 | -664.0 | -557.4 | |
| 0.00 | 1.63 | 0.00 | 0.88 | 8.40 | 280.16 | 22.28 | 283.82 | 0.3879 | -911.0 | -744.3 | |
| 2.18 | 49.57 | 1.18 | 26.69 | 10.66 | 280.18 | 22.31 | 289.43 | 0.3972 | -772.6 | -638.3 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 8.40 | 279.96 | 22.08 | 283.93 | 0.3848 | -883.0 | -649.5 | |
| 20.16 | -11.00 | 10.86 | -11.00 | 10.95 | 279.87 | 21.99 | 290.35 | 0.3938 | -1117.3 | 999999 | |
| 1.82 | 5.27 | 0.98 | 2.83 | 11.42 | 279.67 | 21.80 | 291.64 | 0.3932 | -906.7 | -858.0 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 14.66 | 279.81 | 21.94 | 298.99 | 0.4149 | -831.0 | -680.8 | |
| 0.54 | 4.90 | 0.29 | 2.63 | 11.21 | 279.22 | 21.35 | 291.50 | 0.3854 | -1079.7 | -805.9 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 11.51 | 278.25 | 20.37 | 293.10 | 0.3724 | -848.0 | -659.5 | |
| 0.00 | 3.54 | 0.00 | 1.89 | 11.79 | 278.07 | 20.19 | 293.97 | 0.3714 | -802.0 | -750.4 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 12.41 | 276.13 | 18.26 | 297.66 | 0.3470 | 830.0 | 604.6 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 11.99 | 275.61 | 17.74 | 297.17 | 0.3364 | 781.0 | 637.5 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 13.36 | 275.19 | 17.31 | 301.35 | 0.3405 | 890.0 | 699.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 12.31 | 275.05 | 17.17 | 298.76 | 0.3304 | 884.0 | 718.7 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 11.33 | 274.59 | 16.72 | 296.61 | 0.3168 | 800.0 | 664.7 | |
| 0.00 | 1.73 | 0.00 | 0.91 | 14.73 | 274.74 | 16.86 | 305.46 | 0.3459 | 714.0 | 581.2 | |
| 0.00 | 3.27 | 0.00 | 1.72 | 14.52 | 274.62 | 16.75 | 305.10 | 0.3424 | 612.0 | 552.9 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 14.02 | 274.35 | 16.48 | 304.28 | 0.3345 | 265.0 | 290.1 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 11.47 | 273.95 | 16.08 | 297.85 | 0.3083 | 1011.0 | 886.7 | |
| 0.00 | 2.36 | 0.00 | 1.24 | 14.47 | 273.96 | 16.09 | 306.01 | 0.3331 | 915.0 | 668.6 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 14.32 | 273.69 | 15.81 | 306.07 | 0.3281 | 804.0 | 617.8 | |
| 0.00 | 2.63 | 0.00 | 1.39 | 15.47 | 273.58 | 15.70 | 309.10 | 0.3376 | 800.0 | 710.2 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 8.41 | 273.09 | 15.22 | 289.17 | 0.2761 | 846.0 | 629.6 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 15.25 | 273.43 | 15.56 | 308.84 | 0.3336 | 693.0 | 585.9 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 15.85 | 272.85 | 14.98 | 311.30 | 0.3324 | 846.0 | 608.4 | |
| 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. | |