Model to explain impulsive mm-wave solar bursts (1991)
- Authors:
- Autor USP: OPHER, REUVEN - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Inglês
- Imprenta:
- Source:
- Título: Resumos
- Conference titles: Brazilian Plasma Astrophysics Workshop
-
ABNT
OPHER, E e GALVAO, R M e OPHER, Reuven. Model to explain impulsive mm-wave solar bursts. 1991, Anais.. São Paulo: Fapesp, 1991. . Acesso em: 13 fev. 2026. -
APA
Opher, E., Galvao, R. M., & Opher, R. (1991). Model to explain impulsive mm-wave solar bursts. In Resumos. São Paulo: Fapesp. -
NLM
Opher E, Galvao RM, Opher R. Model to explain impulsive mm-wave solar bursts. Resumos. 1991 ;[citado 2026 fev. 13 ] -
Vancouver
Opher E, Galvao RM, Opher R. Model to explain impulsive mm-wave solar bursts. Resumos. 1991 ;[citado 2026 fev. 13 ] - Magnetic field effect on 3d hydrodynamical, adiabatic and auto-gravitational stellar core collapse
- Large scale structure with cosmological constant
- Calculo do espectro de flutuacoes de plasma pela teoria cinetica de plasma e seus efeitos sobre a nucleossintese primordial
- Origin of primordial magnetic fields
- Conceptual problem for noncommutative inflation and the new approach for nonrelativistic inflationary equation of state
- Criacao dos vazios em larga-escala por explosoes de supernovas primordiais
- Plasma effects on primordial nucleosynthesis
- Suppression of small baryonic structures due to a primordial magnetic field
- Can the first stars formed be pre-galactic?
- Challenges of relativistic astrophysics
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