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1
Introduction
2
Fisks Contributions
3
The Heliosphere
4
Boundary Value Problems
5
Polar coronal holes
6
Supergranules
7
Wave Heating
8
Slow Solar Wind
9
Heliosphere
10
Interstellar Dust
11
Interstellar Neutral Gas
12
Interstellar Neutral Particles
13
Galactic Cosmic Rays
14
Heliosphere phenomena
15
The importance of the heliosphere
Description:
Explore the groundbreaking Parker Lecture delivered by L. A. Fisk at the 1999 AGU Spring Meeting, delving into the complexities of the heliosphere and its interactions with interstellar space. Gain insights into Fisk's significant contributions to solar physics, including boundary value problems, polar coronal holes, and supergranules. Discover the intricacies of wave heating, slow solar wind, and the heliosphere's role in modulating interstellar dust, neutral gas, and cosmic rays. Examine the various phenomena within the heliosphere and understand its crucial importance in shaping our understanding of the Sun's influence on the surrounding space environment. Despite potential imperfections due to the age of the original file, this 51-minute lecture offers valuable knowledge for those interested in solar physics and space science.

The Heliosphere: Structure, Dynamics, and Interactions - 1999 Parker Lecture

AGU
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