Solar wind velocity and corrections

In summary, the solar wind velocity at 1 AU is highly variable and can have an impact on Earth's magnetosphere and ionosphere. A 1-minute Google search for "solar wind velocity distribution site:.edu" yielded useful information, including a PhD dissertation and data from the WIND spacecraft. The WIND data is available in daily and 27-day summary plots due to the rotation rate of the sun. Additionally, the solar wind velocity may play a role in spectroscopy measurements.
  • #1
Ennio
26
2
TL;DR Summary
distribution of solar wind
Greetings,

how do
- the velocity distribution of the solar wind at 1 AU
- the velocity distribution of the solar wind in our line of sight
look like?

I have found the 400 Km/sec but no further information. Is it an average values? Is this radially on the sun the same?
Links with graphs are welcome.

Last but not least:
Does the solar wind velocity play a role in the spectroscopy measurements? How?

Thank you very much.
E.
 
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  • #2
The solar wind is highly variable, and variations in the solar wind can have a direct impact on the Earth's magnetosphere (and hence ionosphere). Did you do a google search? A 1-minute google search (solar wind velocity distribution site:.edu) yielded a lot of good stuff. For example, look at chapter 3 of the PhD dissertation by Steven Peter Joy:
http://www.igpp.ucla.edu/public/sjoy/

If you want to see more actual data, NASA still posts data from the WIND spacecraft .
https://wind.nasa.gov/links.php
at the bottom of the page you will see links to WIND daily summary plots and WIND 27-day summary plots. They are 27 days because that is the rotation rate of the sun.

jason
 
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Likes jefo, davenn, Ennio and 1 other person

1. What is solar wind velocity?

Solar wind velocity refers to the speed at which charged particles from the Sun, primarily protons and electrons, are moving away from the Sun. This velocity can range from 300 to 800 kilometers per second.

2. How is solar wind velocity measured?

Solar wind velocity is measured using spacecraft instruments, such as the Solar Wind Electron Proton Alpha Monitor (SWEPAM) on the Advanced Composition Explorer (ACE) spacecraft. These instruments measure the velocity of the solar wind particles as they pass by the spacecraft.

3. Why is it important to correct for solar wind velocity?

Correcting for solar wind velocity is important because it affects the accuracy of space weather predictions. The faster the solar wind is moving, the more intense the effects on Earth's magnetic field and atmosphere, which can disrupt satellite communications and power grids.

4. What factors can affect solar wind velocity?

Solar wind velocity can be affected by various factors, such as the strength of the solar wind source regions on the Sun, the location and size of coronal holes, and the presence of solar flares or coronal mass ejections. The solar wind can also be influenced by the structure of the interplanetary magnetic field.

5. How are corrections for solar wind velocity made?

Corrections for solar wind velocity are made by comparing data from multiple spacecraft and using models to account for variations in the solar wind. These corrections are constantly updated as new data becomes available, allowing for more accurate space weather predictions.

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