Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..277e&link_type=abstract
In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 277-2
Astronomy and Astrophysics
Astronomy
2
Astronomical Models, Mathematical Models, Solar Corona, Solar Wind, Solar Wind Velocity, Temperature Measurement, Eiscat Radar System (Europe), Extreme Ultraviolet Radiation, Plasma Acceleration, Remote Sensing, Velocity Distribution
Scientific paper
To increase the understanding of the acceleration of the solar wind, it is necessary to combine observations and theoretical approaches. The importance of coordinated measurements in the inner corona and interplanetary space to place constraints on solar wind models is demonstrated. Given the fact that the temperature in the inner corona is the most important parameter in solar wind modeling, observations from which reliable temperatures can be deduced are crucial for such coordinated approaches. The derivation of temperatures in the inner corona are addressed, as well as which assumptions and models are inherent in the temperatures derived using different observational techniques. Two examples of extreme ultraviolet (EUV) observations are chosen to demonstrate problems that can arise in the interpretation of measurements.
Arndt Martina Belz
Esser Ruth
Rifai Habbal Shadia
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