Magicplot student pro#
Magicplot student series#

Fitting of series results in parameters summary table.įormat one figure and save a template. The simplest way to process and fit multiple data in the same way without scripting. Smoothing, FFT, integration, differentiation, histograms, convolution, correlation algorithms are included in ‘Processing’ menu.Įxplore hidden details of your plot with navigation tools: Mouse wheel with Shift/Ctrl changes scale and scrolls. Journal-quality plots can be saved in vector formats: EPS, PDF, SVG, EMF.

You can freely change curve style and axes style using inspector toolbar. Column delimiters and decimal separators are auto recognized.Įnjoy peak-by-peak fit model creation and moving peaks and baseline with mouse. Use ‘?Import Text Table’ menu item to open your data saved in text files. MagicPlot was verified with NIST datasets for testing fitting algorithms.

Magicplot student pro#

Get MagicPlot Pro and take it for a spin to see what it can actually do for you!Įnter equation, edit data range visually and perform a fit. MagicPlot Pro is powerful enough and consistent. The insights obtained from the results of this study can be applied to analyse the vacancy transfer mechanisms in very-heavy systems (combined atomic number > 100).MagicPlot Pro is a handy tool for scientific and engineer data processing, plotting and nonlinear fitting. The significant discrepancies observed between the experimental and theoretical values have been explained qualitatively within the framework of quasi-molecular orbital formation using level correlations. Moreover, the cross-sections measured in this study were found to be several orders of magnitude higher than those obtained in other reported studies on low-energy lighter-ion-impact on Au and Pb. The measured cross-sections were underestimated by these theories. The collision-induced X-ray spectra of both the collision partners were examined, and the corresponding intensity ratios and cross-sections were compared with those calculated using two well-known ionisation theories, viz. This study was conducted to evaluate the inner-shell ionisation of Au (135 and 508 μ g / cm 2) and Pb (107, 157 and 390 μ g / cm 2) targets due to low-energy (2–5 MeV) 54Xe q +-ion impact. To date, only a few studies have been reported on the investigation of very-low-energy heavy-ion impact on heavy atoms using X-rays, especially M-shell X-rays of the heavy atom. However, both experimental and theoretical investigations on ion–atom collision-induced X-rays have remained mostly restricted to high-energy light-ion impact on heavy atoms. The detection and analysis of collision-induced X-rays is a widely-used powerful technique for analysing atomic-scale phenomena. Despite the multitude of studies conducted over the years, our understanding of the atomic vacancy transfer mechanisms remains exiguous. The generation of collision-induced vacancies and their transfer within the electronic inner shells are the source of several unprecedented phenomena, which have been revealed in recent experimental studies conducted using state-of-the-art next-generation accelerators and detectors.