The cooling of flare produced plasmas in the solar corona
- 1 December 1970
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 15 (2), 394-413
- https://doi.org/10.1007/bf00151847
Abstract
No abstract availableKeywords
This publication has 16 references indexed in Scilit:
- Further X-ray spectra of solar active regionsSolar Physics, 1970
- The helium-like calcium, silicon, and sulfur lines during the decay of a large flareSolar Physics, 1970
- Solar X-ray bursts at energies less than 10 keV observed with OSO-4Solar Physics, 1970
- Rapid Fine Structure in a Burst of Hard Solar X-Rays Observed by OSO-5The Astrophysical Journal, 1969
- On the localization, size and structure of the regions of the X-ray flares on the SunSolar Physics, 1969
- Ionization Equilibrium and Radiative Cooling of a Low-Density PlasmaThe Astrophysical Journal, 1969
- Interpretation of Solar Helium-Like Ion Line IntensitiesMonthly Notices of the Royal Astronomical Society, 1969
- The Hard Solar X-Ray Spectrum Observed from the Third Orbiting Solar ObservatoryThe Astrophysical Journal, 1969
- Thermal Continuum Radiation from Coronal Plasmas at Soft X-ray WavelengthsMonthly Notices of the Royal Astronomical Society, 1969
- A Proportional Counter Spectrometer for the Study of the Solar Soft X-Ray SpectrumIEEE Transactions on Nuclear Science, 1967