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• Sunspot Band6 SingleDish for CASA 5.1
  [[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.
  5 KB (769 words) - 16:33, 19 August 2021
• Sunspot Band6 Feathering for CASA 5.1
  [[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,
  8 KB (1,332 words) - 16:42, 19 August 2021
• Sunspot Band6 SingleDish for CASA 4.7
  ...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
  4 KB (710 words) - 09:22, 11 January 2018
• Sunspot Band6 Feathering for CASA 4.7
  ...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==
  9 KB (1,473 words) - 09:42, 11 January 2018
• Sunspot Band6 SingleDish for CASA 6.5.4
  [[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.
  9 KB (1,096 words) - 16:50, 12 April 2024
• Sunspot Band6
  [[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
  6 KB (955 words) - 15:48, 16 April 2024
• Sunspot Band6 Feathering for CASA 6.5.4
  [[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:
  14 KB (2,204 words) - 17:10, 17 April 2024
• Sunspot Band6 Imaging for CASA 6.5.4
  [[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.]]
  7 KB (1,154 words) - 14:35, 16 April 2024
• Analysis Utilities
  : generates a plot of the Sun's az vs. el during an ms or ASDM
  8 KB (1,235 words) - 11:11, 22 April 2024
• Sunspot Band6 Calibration for CASA 5.1
  [[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
  40 KB (4,408 words) - 16:31, 19 August 2021
• Sunspot Band6 Calibration for CASA 4.7
  [[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
  41 KB (4,534 words) - 08:50, 11 January 2018
• Sunspot Band6 Calibration for CASA 6.5.4
  [[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
  50 KB (5,729 words) - 12:35, 22 April 2024
• Sunspot Band6 Imaging for CASA 5.1
  [[Category:ALMA]][[Category:Imaging]][[Category:Sun]]
  6 KB (1,016 words) - 16:37, 19 August 2021
• Sunspot Band6 Imaging for CASA 4.7
  [[Category:ALMA]][[Category:Imaging]][[Category:Sun]]
  7 KB (1,182 words) - 09:10, 11 January 2018
• Imaging Prep CASA 6.1.1
  ...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
  22 KB (2,892 words) - 16:28, 28 February 2024
• Imaging Prep CASA 6.5.4
  ...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
  23 KB (2,951 words) - 13:49, 7 December 2023
• OT tutorial SISS 2018
  ...ponds to a 1σ molecular mass sensitivity of 8 x 10⁴ M_Sun per beam per 10 km/s channel, enough to detect Orion-like clouds at S
  25 KB (4,152 words) - 11:36, 16 May 2018
• VLA CASA Imaging-CASA4.6.0
  ...' and ''BARY'' are the most popular Local Standard of Rest (kinematic) and sun-earth Barycenter references. ''veltype'' defines whether the data will be g
  60 KB (9,464 words) - 18:16, 25 May 2016
• VLA CASA Imaging-CASA4.5.2
  ...ty frame where ''LSRK'' (Local Standard of Rest (kinematic)) and ''BARY'' (Sun-Earth Barycenter) are the most popular references. Parameter ''veltype'' de
  60 KB (9,489 words) - 15:18, 25 May 2016
• TWHydraBand7 Imaging 4.4
  ...on (note that you can also do this using the mouse and the color stretch - sun - icon). I left the scaling power cycles at 0 and set the data range to [-0
  63 KB (9,660 words) - 21:36, 6 July 2015

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