A program to calculate coronal emission line strengths

Title of program: AATWAB
Catalogue Id: ACXE_v1_0

Nature of problem
This computer program is used to calculate the intensities of emission spectral lines from the upper solar atmosphere. The optically thin approximation is used and the validity of this assumption is checked by calculating line centre optical depths. Account may be taken of collisional transitions (by electron and proton impact) and spontaneous radiative transitions between all the selected levels of the chosen ion in calculating the intensities. The program integrates these intensities through w ...

Versions of this program held in the CPC repository in Mendeley Data
ACXE_v1_0; AATWAB; 10.1016/0010-4655(77)90024-8

This program has been imported from the CPC Program Library held at Queen's University Belfast (1969-2019)

程序名称：AATWAB
目录编号：ACXE_v1_0

问题本质
本计算机程序用于计算太阳高层大气的发射谱线强度。程序采用光学薄近似假设，并通过计算谱线中心光学厚度验证该假设的适用性。在计算谱线强度时，可纳入指定离子所有选定能级间的碰撞跃迁（由电子与质子碰撞诱发）及自发辐射跃迁。本程序将这些强度沿……（原文此处截断）进行积分。

存放在Mendeley数据（Mendeley Data）库的CPC存储库中的该程序版本信息为：ACXE_v1_0；AATWAB；10.1016/0010-4655(77)90024-8

本程序源自贝尔法斯特女王大学托管的CPC程序库（1969-2019年）