Helioseismology

Virginia Open Data2026-05-02 收录

日震学

天体内部结构模拟

数据链接：

https://data.zh-cn.virginia.gov/dataset/helioseismology 数据链接链接失效反馈

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资源简介：

Oscillations detected on the solar surface provide a unique opportunity for investigations of the interior properties of a star. Through major observational efforts, including...

Validating time-distance helioseismology with realistic quiet-sun simulations

日震学

流体动力学模拟

Linear time-distance helioseismic inversions are carried out for vector flow velocities using travel times measured from two ~100Â² MmÂ² Ã 20 Mm realistic magnetohydrodynamic...

University Corporation for Atmospheric Research90

A simple star

天体内部结构模拟

Eddington模型

Abstract In this work we present the problem of obtaining and integrating numerically the hydrostatic equilibrium equations for a star with a polytropic equation of state, which is the well known Edd

NIAID Data Ecosystem80

Local structure and density of liquid Fe-C-S alloys at Moon's core conditions

极端条件材料

天体内部结构模拟

This file includes the raw CAESAR and absorption data measured in each P-T condition and the Python codes for diffraction and absorption data analysis. Matlab codes for P-T calibration are also encl

NIAID Data Ecosystem60

Can superionic ammonia exist in different structures?

极端条件物质相变

天体内部结构模拟

The aim of this proposal is to study the properties (structure, dilatation coefficient) and thermodynamic P-T boundaries of the superionic phase of ammonia in the range 40-100 GPa and 300-3500 K. Supe

ESRF Portal2026-01-01 更新80

Solar acoustic modes in period 1996-2014

日震学

太阳活动周期

Solar activity has significantly changed over the last two Schwabe cycles. After a long and deep minimum at the end of Cycle 23, the weaker activity of Cycle 24 contrasts with...

B2FIND60

Helioseismology

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