Sunspot Band6 Feathering for CASA 4.7: Difference between revisions
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==Obtaining the RA/Dec coordinate of the sun center at the reference time== | ==Obtaining the RA/Dec coordinate of the sun center at the reference time== | ||
Before starting the combination process on CASA, we need to know the RA/Dec coordinate of the sun center at the reference time that is used for the image synthesis, because the observing time of the TP-array is not the same as the reference time exactly. The Sun was moving on the RA/Dec coordinate frame during the gap between the times. To combine the synthesized image with the full-sun image obtained from the TP array, we need to shift the coordinate of the full-sun image based on the coordinate of the sun center at the reference time. Hence, we obtain the solar coordinate from the JPL’s HORIZONS system[[http://ssd.jpl.nasa.gov/horizons.cgi]]. | |||
The reference time in this tutorial is 19:49:00UT, December 18 2015. At the time, the RA/Dec coordinate of the sun center estimated by JPL’s HORIZONS system is RA: 266.01898 degree, Dec: -23.38648 degrees. | |||
==Preparation for Feathering task: The Single-Dish data== | ==Preparation for Feathering task: The Single-Dish data== | ||
==Preparation for Feathering task: The Synthesized image== | ==Preparation for Feathering task: The Synthesized image== | ||
==Combining, primary beam correction, and creating of the FITS file.== | ==Combining, primary beam correction, and creating of the FITS file.== | ||
==Alternative way of Combining Images== | ==Alternative way of Combining Images== | ||
Revision as of 13:25, 11 January 2018
Overview
This portion of the Sunspot Band6 CASA Guide for CASA 4.7 covers the combine process between the synthesized solar image and the full-sun image obtained with TP array. It begins where the calibration of the visibility data and single-dish data, image synthesis, and creating of the full-sun map are completed. If you do not complete them, at first,
1) Download the file of the un-calibrated data package ‘Sunspot_Band6_UncalibratedData.tgz’, do the calibration of the data, and create the images from the interferometric data and single-dish data, along with the ‘Sunspot_Band6_*_for_CASA_4.7’ tutorials.
or
2) Download the file of the calibrated data package ‘Sunspot_Band6_CalibratedData.tgz’, and synthesize the image from interferometric data along the ‘Sunspot_Band6_Imaging_for_CASA_4.7’ tutorial.
In case 1), we assume that you are working on the working directory ‘Sunspot_Band6_UncalibratedData’. On the other hand, when you started the tutorial from the calibrated package (case 2), we assume that the working directory is ‘Sunspot_Band6_CalibratedData.’
From next, we will show all commands for combining the images. If you do not want to cut-&-past the commands, you can use the script as described in #Alternative way of Combining Images.
Obtaining the RA/Dec coordinate of the sun center at the reference time
Before starting the combination process on CASA, we need to know the RA/Dec coordinate of the sun center at the reference time that is used for the image synthesis, because the observing time of the TP-array is not the same as the reference time exactly. The Sun was moving on the RA/Dec coordinate frame during the gap between the times. To combine the synthesized image with the full-sun image obtained from the TP array, we need to shift the coordinate of the full-sun image based on the coordinate of the sun center at the reference time. Hence, we obtain the solar coordinate from the JPL’s HORIZONS system[[1]].
The reference time in this tutorial is 19:49:00UT, December 18 2015. At the time, the RA/Dec coordinate of the sun center estimated by JPL’s HORIZONS system is RA: 266.01898 degree, Dec: -23.38648 degrees.
