After a great summer I would like to share with you what I worked on. 😊 But before that I would like to thank everyone who made that possible. Thank you Shane that you was my mentor this summer and guided me through every problem. I definitely learnt a lot and it was fun. 😃 Thanks for the SunPy community taking me in, and for their every help and I also want to thank ESA and Maxime Perrotin who organized this great program! And now, we can check out the results! 😉 You can find the documentation in the project wiki and the theoretical background in my previous posts. Now I want to concentrate on the actual usage of the library in case of an actual problem from A-Z. Lets say that we have a fits file with several RHESSI visibilities and we would like to process it. First we would like to get the xrayvision module (I assuming that SunPy is already installed). To get the module we have to check it out from GitHub: git clone https://github.com/sunpy/xrayvision.git After t
There was a big silence from my side regarding the improvements in the past month... Sorry about that, but do not worry, I am summarizing up everything below now: 😉 In the official repo you can find right now these two classes: Transform Visibility Transform 's basic purpose to provide a DFT (Discrete Fourier Transformation) and an IDFT (Inverse Discrete Fourier Transformation) method which can be used to create visbility values from intensity maps and in the other way around. An example for the usage of the DFT method: Converting an intensity map into visibility values with DFT method You can find more information about the Transform class on the github wiki of the project. And now about the Visibility class. During synthesis imaging the data comes from different telescopes with different distance from each other. As a result of this we can create images with the same angular resolution what we would get by using a telescope with the size of what is t