Radio burst characteristics of solar proton flares
Journal Article
·
· Astrophys. J.; (United States)
To isolate the properties of solar radio bursts indicative of energetic (E>20 MeV) proton acceleration, we compare several groups of solar bursts. Intense centimetric bursts and metric type II bursts associated with solar flares at magnetically well-connected longitudes, but not resulting in detected prompt proton events, are compared with the radio bursts of proton flares. The type II bursts not associated with proton flares are distinguished from those of proton flares by their short durations, associations with small H..cap alpha.. flares, and lack of associated type IV metric bursts. We find that, contrary to the claim of Svestka and Fritzova-Svestkova, the appearance of a type II burst, indicating a coronal shock, is not a sufficient condition for the occurrence of an interplanetary proton event. We further conclude that interplanetary energetic protons are not significantly produced in most type II burst shocks. The centimetric bursts were examined in detail using records from the Sagamore Hill Observatory. The distinguishing difference between the proton and nonproton centimetric bursts is that the proton-event burst durations ranged from 1 minute to 1 hour, but the burst durations of nonproton flares were less than 10 minutes. We argue that energetic electrons produced in postflare loop systems are the sources of the stationary metric and decimetric type IV bursts associated with proton flares.
- Research Organization:
- Air Force Geophysics Laboratory, Hanscom Air Force Base, Massachusetts
- OSTI ID:
- 6527326
- Journal Information:
- Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 261:2; ISSN ASJOA
- Country of Publication:
- United States
- Language:
- English
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Technical Report
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Tue Dec 31 23:00:00 EST 1985
·
OSTI ID:5312327
Electron acceleration in impulsive solar flares
Journal Article
·
Tue Nov 30 23:00:00 EST 1982
· Astrophys. J.; (United States)
·
OSTI ID:5577396
LARGE SOLAR ENERGETIC PARTICLE EVENTS ASSOCIATED WITH FILAMENT ERUPTIONS OUTSIDE ACTIVE REGIONS
Journal Article
·
Wed Jun 10 00:00:00 EDT 2015
· Astrophysical Journal
·
OSTI ID:22522348
Related Subjects
640104* -- Astrophysics & Cosmology-- Solar Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ACCELERATION
BARYONS
DATA ANALYSIS
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
FERMIONS
HADRONS
INTERPLANETARY SPACE
MAGNETIC FIELDS
NUCLEONS
PLASMA ACCELERATION
PROTONS
RADIATIONS
RADIOWAVE RADIATION
SHOCK WAVES
SOLAR ACTIVITY
SOLAR FLARES
SOLAR PARTICLES
SOLAR PROTONS
SOLAR RADIATION
SOLAR RADIO BURSTS
SPACE
STELLAR RADIATION
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ACCELERATION
BARYONS
DATA ANALYSIS
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
FERMIONS
HADRONS
INTERPLANETARY SPACE
MAGNETIC FIELDS
NUCLEONS
PLASMA ACCELERATION
PROTONS
RADIATIONS
RADIOWAVE RADIATION
SHOCK WAVES
SOLAR ACTIVITY
SOLAR FLARES
SOLAR PARTICLES
SOLAR PROTONS
SOLAR RADIATION
SOLAR RADIO BURSTS
SPACE
STELLAR RADIATION