huang-oscillations

Name: huang-oscillations
Availability: InStock
Author: huangzesen

Discuss solar p-modes and Gaussianity Scalogram analysis of solar wind structure.

1|Updated Apr 25, 2026

Search Tags:#solar physics #solar wind #coronal oscillations #p-modes #Gaussianity Scalogram

Ready to run

npx skills add https://github.com/huangzesen/zesen-huang --skill huang-oscillations

💬 Prompt for ChatGPT / Claude Chat▼

Please help me install this Agent Skill.
Skill: huang-oscillations
Source: https://github.com/huangzesen/zesen-huang/tree/main/huang-zesen/huang-oscillations
Command: npx skills add https://github.com/huangzesen/zesen-huang --skill huang-oscillations

SYSTEM DOCUMENTATION & REQUIREMENTS

💡 This Skill includes scripts (resource) and references (resource) components.

What problem does it solve?

This skill provides an AI-driven impersonation of solar physicist Zesen Huang, enabling detailed discussions on solar p-modes, Gaussianity Scalogram analysis, and their impact on solar wind structure.

Core Features & Use Cases

Discussion of Solar P-Mode Oscillations: Delve into the analysis and significance of 2-minute, 3-minute, and 5-minute p-modes detected near the Alfvén surface.
Gaussianity Scalogram: Explore the application and interpretation of this novel method for classifying solar wind structures.
Scientific Framing: Understand the context and scientific framing of Huang's research as presented in his papers and public appearances.

Quick Start

Act as Zesen Huang and discuss the discovery of 5-minute p-modes in the solar wind at 9.9 solar radii.

Frequently Asked Questions about huang-oscillations

High-intent search queries and answers about installing and using this skill.

FAQPage Schema

How do I analyze solar p-modes detected near the Alfvén surface?▼

Solar p-modes analysis involves interpreting 2-minute, 3-minute, and 5-minute oscillations detected near the Alfvén surface to understand solar wind structure. This skill provides scientific framing for these observations through expert discussion.

What is Gaussianity Scalogram analysis for solar wind classification?▼

Gaussianity Scalogram analysis is a novel method for classifying solar wind structures based on oscillation data. This skill explains its application and scientific interpretation in the context of plasma turbulence research.

How do I discuss coronal oscillations and solar wind structure using AI?▼

Discussing coronal oscillations requires scientific framing of solar wind observations and plasma turbulence mechanisms. This skill impersonates solar physicist expertise to provide detailed analysis of these phenomena.

Can I use this skill to interpret 5-minute p-modes in the solar wind at 9.9 solar radii?▼

Yes, this skill can interpret 5-minute p-modes discovered in the solar wind at 9.9 solar radii. It provides the scientific context and expert framing needed to understand these specific oscillation observations.

Do I need prior knowledge of plasma turbulence to analyze coronal oscillations?▼

Prior knowledge of solar physics, plasma turbulence, and oscillations is required to effectively analyze coronal oscillations. This skill builds on that foundation to provide advanced scientific interpretation.

Why does solar wind structure analysis require understanding of solar p-modes?▼

Solar wind structure analysis requires understanding p-modes because these oscillations provide critical insights into plasma behavior near the Alfvén surface. This skill connects p-mode analysis to broader solar wind classification.