SITCoM: SiRGraF Integrated Tool for Coronal dynaMics

IF 2.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Frontiers in Astronomy and Space Sciences Pub Date : 2023-09-15 DOI:10.3389/fspas.2023.1227872
Purvi Udhwani, Arpit Kumar Shrivastav, Ritesh Patel
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Abstract

SiRGraF Integrated Tool for Coronal dynaMics (SITCoM) is based on the Simple Radial Gradient Filter used to filter the radial gradient in the white-light coronagraph images and bring out dynamic structures. SITCoM has been developed in Python and integrated with SunPy and can be installed by users with the command pip install sitcom. This enables the user to pass the white-light coronagraph data to the tool and generate radially filtered output with an option to save in various formats as required. We implemented the functionality of tracking the transients such as coronal mass ejections, outflows, and plasma blobs, using height–time plots and deriving their kinematics. In addition, SITCoM also supports oscillation and wave studies such as for streamer waves. This is performed by creating a distance–time plot at a user-defined location (artificial slice) and fitting a sinusoidal function to derive the properties of waves, such as time period, amplitude, and damping time (if any). We provide the option to manually or automatically select the data points to be used for fitting. SITCoM is a tool to analyze some properties of coronal dynamics quickly. We present an overview of the SITCoM with the applications for deriving coronal dynamics’ kinematics and oscillation properties. We discuss the limitations of this tool along with prospects for future improvement.
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SiRGraF日冕动力学集成工具
SiRGraF日冕动力学集成工具(SITCoM)是基于简单径向梯度滤波器,用于过滤白光日冕图像中的径向梯度,从而得到动态结构。SITCoM是用Python开发的,与SunPy集成,用户可以使用pip install SITCoM命令进行安装。这使用户能够将白光日冕仪数据传递给工具,并生成径向过滤输出,并可根据需要以各种格式保存。我们实现了跟踪瞬态的功能,如日冕物质抛射、外流和等离子体斑点,使用高度时间图并推导它们的运动学。此外,SITCoM还支持振荡和波动研究,如拖波。这是通过在用户定义的位置(人工切片)创建距离-时间图并拟合正弦函数来导出波的属性,例如时间段,振幅和阻尼时间(如果有的话)来执行的。我们提供手动或自动选择用于拟合的数据点的选项。SITCoM是一种快速分析日冕动力学特性的工具。我们概述了SITCoM及其在推导日冕动力学的运动学和振荡特性方面的应用。我们讨论了该工具的局限性以及未来改进的前景。
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来源期刊
Frontiers in Astronomy and Space Sciences
Frontiers in Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
3.40
自引率
13.30%
发文量
363
审稿时长
14 weeks
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