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[[Category:ALMA]][[Category:Sun]][[Category:Continuum]][[Category:Calibration‏‎]] ...ll show all commands for the calibration and be creating the map of a full Sun with Band6. ...

[[Category:ALMA]][[Category:Imaging]][[Category:Sun]] ...ility data and single-dish data, image synthesis, and creating of the full-sun map are completed. If you do not complete them, at first, ...

...ll show all commands for the calibration and be creating the map of a full Sun with Band6. If you do not want to cut-&-paste the commands, you can use the ...tion, the atmospheric calibration was done before the fast-scanning of the Sun. We use the calibration date to apply the solar data using the option ‘ps’ ...

...ility data and single-dish data, image synthesis, and creating of the full-sun map are completed. If you do not complete them, at first, ==Obtaining the RA/Dec coordinate of the sun center at the reference time== ...

[[Category:ALMA]][[Category:Sun]][[Category:Continuum]][[Category:Calibration‏‎]] ...the data obtained with the Total Power array. We create the map of a full Sun with Band6. ...

[[Category:ALMA]][[Category:Sun]][[Category:Continuum]][[Category:Calibration‏‎]] ...the data obtained with the Total Power array. We create the map of a full Sun with Band6. ...

[[Category:ALMA]][[Category:Sun]][[Category:Continuum]] ...ined with TP-array, and combined image from the synthesized image and full-sun map. ...

[[Category:ALMA]][[Category:Sun]][[Category:Continuum]] ...g mode. The field of view of the map is a circle with 2400” diameter (Full Sun). The frequency of the LO1 is the same as the previous dataset, but no corr ...

[[Category:ALMA]][[Category:Imaging]][[Category:Sun]] ...s the combination process between the synthesized solar image and the full-sun image obtained with the TP array. It is the final step after: ...

[[Category:ALMA]][[Category:Imaging]][[Category:Sun]] ...s the combination process between the synthesized solar image and the full-sun image obtained with the TP array. It is the final step after: ...

[[Category:ALMA]][[Category:Imaging]][[Category:Sun]] ...me_CASA_6.5.4.png|thumb|right|'''Fig. 1.''' The plot of the FieldID of the Sun scans as a function of the time.]] ...

[[Category:ALMA]][[Category:Imaging]][[Category:Sun]] ...me_CASA_6.5.4.png|thumb|right|'''Fig. 1.''' The plot of the FieldID of the Sun scans as a function of the time.]] ...

: generates a plot of the Sun's az vs. el during an ms or ASDM ...

[[Category:ALMA]][[Category:Calibration]][[Category:Sun]] 18-Dec-2015/19:15:42.3 - 19:16:47.5 1 0 Sun 236530 [0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18 ...

[[Category:ALMA]][[Category:Calibration]][[Category:Sun]] 18-Dec-2015/19:15:42.3 - 19:16:47.5 1 0 Sun 236530 [0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18 ...

[[Category:ALMA]][[Category:Calibration]][[Category:Sun]] WARNING: The command in the [[#Tsys+Tant calibration of the Sun]] section of this guide takes a long time to run. Depending on your machine ...

[[Category:ALMA]][[Category:Calibration]][[Category:Sun]] WARNING: The command in the [[#Tsys+Tant calibration of the Sun]] section of this guide takes a long time to run. Depending on your machine ...

[[Category:ALMA]][[Category:Imaging]][[Category:Sun]] ...

[[Category:ALMA]][[Category:Imaging]][[Category:Sun]] ...

...d sky frequencies because the vector of the motion of the Earth around the Sun will be different at different times. ...most common use case for this is where the motion of the Earth around the Sun causes the sky frequencies of the lines to shift too much between execution ...