Cheng et al., 1981 - Google Patents
What produces the high densities observed in solar flare plasmasCheng et al., 1981
View HTML- Document ID
- 7104059168900937167
- Author
- Cheng C
- Feldman U
- Doschek G
- Publication year
- Publication venue
- Astronomy and Astrophysics, vol. 97, no. 1, Apr. 1981, p. 210-212.
External Links
Snippet
Attention is drawn to the implications of the high densities observed in flare plasmas in the wide temperature range from 10 to the 4th K to more than 10 to the 7th K. The chromospheric evaporation theory for the decay phase is discussed, and it is found that it is …
- 210000002381 Plasma 0 title abstract description 53
Classifications
-
- Y—GENERAL TAGGING OF NEW TECHNOLOGICAL DEVELOPMENTS; GENERAL TAGGING OF CROSS-SECTIONAL TECHNOLOGIES SPANNING OVER SEVERAL SECTIONS OF THE IPC; TECHNICAL SUBJECTS COVERED BY FORMER USPC CROSS-REFERENCE ART COLLECTIONS [XRACs] AND DIGESTS
- Y02—TECHNOLOGIES OR APPLICATIONS FOR MITIGATION OR ADAPTATION AGAINST CLIMATE CHANGE
- Y02E—REDUCTION OF GREENHOUSE GASES [GHG] EMISSION, RELATED TO ENERGY GENERATION, TRANSMISSION OR DISTRIBUTION
- Y02E30/00—Energy generation of nuclear origin
- Y02E30/30—Nuclear fission reactors
Similar Documents
| Publication | Publication Date | Title |
|---|---|---|
| Scalo | Heating of dense interstellar clouds by magnetic ion slip-A constraint on cloud field strengths | |
| BOROWSKI | A comparison of fusion/antiproton propulsion systems for interplanetary travel | |
| Weaver et al. | Dissipation in supernova shock waves | |
| Cheng et al. | What produces the high densities observed in solar flare plasmas | |
| Sinha et al. | Upper critical field and (non)-superconductivity of magnetars | |
| Hlubina | Effect of impurities on the transport properties in the Van Hove scenario | |
| Yoshiki et al. | Feasibility study of a strong ultra cold neutron source | |
| Mullan | Mean colors of stellar flare continuum. | |
| Oster et al. | Thermal dissipation and its application to flare phenomena | |
| Dixit et al. | Monopole annihilation and baryogenesis at the electroweak scale | |
| Kammash et al. | An americium‐fueled gas core nuclear rocket | |
| Mullan | A model for nonmonotonic optical light curves of stellar flares | |
| Emslie | Adiabatic and nonadiabatic processes in thermal models of solar hard X-ray bursts | |
| Brown | Comments on the role of conduction in optical flare heating | |
| Gentile | Electrical and Thermal Conductivities in Neutron Stars | |
| Hilton | Plasma and engineering parameters for a fusion powered rocket | |
| GB930518A (en) | High temperature thermocouple | |
| Athay | Sources of solar ultraviolet radiation | |
| Ergma et al. | Numerical models of hydrogen and helium burning flashes on the surface of neutron stars | |
| Giachetti et al. | Non-stationary heating of solar flare plasma by non-thermal electrons | |
| Arnett | Nuclear Reactions and Neutrinos in Stellar Evolution Abstracts of Short Communications Presented after Paper by Arnett | |
| Walder et al. | Theoretical considerations on colliding clumped winds | |
| Colgate et al. | Helium/3/rich solar flares | |
| Manos et al. | Thermal Protection of Structural, Propulsion, and Temperature-sensitive Materials for Hypersonic and Space Flight | |
| Shalybkov | The effect of direct Urca processes on the ohmic decay of the magnetic field |