A SOLAR WIND BACKGROUND MODEL
maps of polarized brightness (pB) of K-corona at 1.36 solar radii observed by MKIII. in High Altitude Observator (HAO) are used to derive corona density...
Quiet Corona Density Model for the Last Maximum of Solar Activity
Quiet Corona Density Model for the Last Maximum of Solar Activity. Authors:, Leblanc, Y.; Leroy, J. L.; Pecantet, P. Publication:, Solar Physics, Vol...
Solar Physics Glossary
The corona consists of a highly rarefied gas with a low density and a temperature greater than one million degrees Kelvin. It is visible to the naked eye...
Hot Oxygen Corona at Mars and Its Effect on Solar Wind Deceleratio
Hot Oxygen Corona at Mars and Its Effect on Solar Wind Deceleratio... 10–15 km/s when we invoke the well established hot oxygen corona density profiles...
A solar wind background model
It is very important to establish the global model of solar corona and... by MKIII in High Altitude Observator (HAO) are used to derive corona density...
Corona Density Profiles in Polymeric Micelles: Small-Angle Neutron ...
Corona Density Profiles in Polymeric Micelles: Small-Angle. Neutron Scattering Results Compared with Self-Consistent. Lattice-Field Calculations...
