LONG-DURATION LOW-FREQUENCY TYPE III BURSTS AND SOLAR ENERGETIC PARTICLE EVENTS
Journal Article
·
· Astrophysical Journal Letters
- NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
We analyzed the coronal mass ejections (CMEs), flares, and type II radio bursts associated with a set of three complex, long-duration, low-frequency (<14 MHz) type III bursts from active region 10588 in 2004 April. The durations were measured at 1 and 14 MHz using data from Wind/WAVES and were well above the threshold value (>15 minutes) normally used to define these bursts. One of the three type III bursts was not associated with a type II burst, which also lacked a solar energetic particle (SEP) event at energies >25 MeV. The 1 MHz duration of the type III burst (28 minutes) for this event was near the median value of type III durations found for gradual SEP events and ground level enhancement events. Yet, there was no sign of an SEP event. On the other hand, the other two type III bursts from the same active region had similar duration but were accompanied by WAVES type II bursts; these bursts were also accompanied by SEP events detected by SOHO/ERNE. The CMEs for the three events had similar speeds, and the flares also had similar size and duration. This study suggests that the occurrence of a complex, long-duration, low-frequency type III burst is not a good indicator of an SEP event.
- OSTI ID:
- 21452798
- Journal Information:
- Astrophysical Journal Letters, Journal Name: Astrophysical Journal Letters Journal Issue: 1 Vol. 721; ISSN 2041-8205
- Country of Publication:
- United States
- Language:
- English
Similar Records
ARE THERE TWO DISTINCT SOLAR ENERGETIC PARTICLE RELEASES IN THE 2012 MAY 17 GROUND LEVEL ENHANCEMENT EVENT?
The 2024 July 16 solar event: a challenge to the coronal mass ejection origin of long-duration gamma-ray flares
LARGE SOLAR ENERGETIC PARTICLE EVENTS ASSOCIATED WITH FILAMENT ERUPTIONS OUTSIDE ACTIVE REGIONS
Journal Article
·
Fri Feb 19 23:00:00 EST 2016
· Astrophysical Journal
·
OSTI ID:22521525
The 2024 July 16 solar event: a challenge to the coronal mass ejection origin of long-duration gamma-ray flares
Journal Article
·
Thu Dec 04 19:00:00 EST 2025
· Astronomy & Astrophysics
·
OSTI ID:3023523
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
79 ASTRONOMY AND ASTROPHYSICS
ATMOSPHERES
ENERGY RANGE
FREQUENCY RANGE
MAIN SEQUENCE STARS
MASS
MEV RANGE
MEV RANGE 10-100
MHZ RANGE
MHZ RANGE 01-100
RADIATIONS
SOLAR ACTIVITY
SOLAR ATMOSPHERE
SOLAR CORONA
SOLAR FLARES
SOLAR RADIATION
STARS
STELLAR ACTIVITY
STELLAR ATMOSPHERES
STELLAR CORONAE
STELLAR FLARES
STELLAR RADIATION
SUN
ATMOSPHERES
ENERGY RANGE
FREQUENCY RANGE
MAIN SEQUENCE STARS
MASS
MEV RANGE
MEV RANGE 10-100
MHZ RANGE
MHZ RANGE 01-100
RADIATIONS
SOLAR ACTIVITY
SOLAR ATMOSPHERE
SOLAR CORONA
SOLAR FLARES
SOLAR RADIATION
STARS
STELLAR ACTIVITY
STELLAR ATMOSPHERES
STELLAR CORONAE
STELLAR FLARES
STELLAR RADIATION
SUN