ខ្យល់ព្រះអាទិត្យ

ខ្យល់ព្រះអាទិត្យ ជាចរន្តនៃអ៊ីយ៉ុង ដែលបញ្ចេញដោយស្រទាប់ក្រៅបំផុតនៃបរិយាកាស។ ខ្យល់ព្រះអាទិត្យ បានរុញច្រានមណ្ឌលម៉ាញេតូចូលទៅក្នុងលំហ ចេញឆ្ងាយពីព្រះអាទិត្យបន្ថែមទៀត។

The heliospheric current sheet results from the influence of the Sun's rotating magnetic field on the plasma in the solar wind.

The solar wind is a stream of charged particles (a plasma) released from the upper atmosphere of the Sun. It mostly consists of electrons and protons with energies usually between 1.5 and 10 keV. The stream of particles varies in density, temperature, and speed over time and over longitude. These particles can escape the Sun's gravity because of their high kinetic energy and the high temperature of the corona.

មើលផងដែរ

• Condegram spiral plot
• Dyson-Harrop satellite
• Electric sail
• Heliosphere
• Helium Focusing Cone
• Interplanetary Magnetic Field
• Interplanetary medium
• List of plasma (physics) articles
• Magnetic sail
• Parker spiral
• Plasmasphere
• Solar Cycle
• Solar sail
• Solar and Heliospheric Observatory
• Solar Probe Plus
• Solar Wind Composition Experiment
• Space weather
• Stellar wind
• STEREO
• Sunspot
• WIND (spacecraft)

ឯកសារយោង

Fox, Karen C. (2012) "NASA Study Using Cluster Reveals New Insights Into Solar Wind" NASA.

តំណភ្ជាប់ខាងក្រៅ

• Real-time plots of solar wind activity from the Advanced Composition Explorer
• Current solar wind pressure NOAA Space Weather Prediction Center
• Solar wind MSFC solar wind site
• Sun|trek website An educational resource for teachers and students about the Sun and its effect on the Earth
• Cluster shows how solar wind is heated
• Could solar wind power Earth? October 4, 2010 by Miranda Marquit
• Solar Or Wind Power? Why Not Both? By Eric Bland, Wed September 29, 2010
• The Solar Wind Power Satellite as an alternative to a traditional Dyson Sphere and its implications for remote detection International Journal of Astrobiology (2010), 9: 89-99