Semi-harmonic and intermittent solar decimetric spikes

Details Semi-harmonic and intermittent solar decimetric spikes Semi-harmonic and intermittent solar decimetric spikes

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..264...81f&link_type=abstract

Solar and Stellar Variability: Impact on Earth and Planets, Proceedings of the International Astronomical Union, IAU Symposium,

Astronomy and Astrophysics

Astronomy

Sun: Activity, Radio Radiation, Decimetric Spikes, Instrumentation: Spectrographs

Scientific paper

We present the analysis of the narrowband solar radio spike emissions observed by the Brazilian Solar Spectroscope (BSS) on 24 June, 1999, at 16:53:55-16:56:48 UT. The data were recorded with temporal resolution of 50 ms and frequency resolution of 5 MHz. The dynamic spectra of clusters of spikes were recorded in 100 channels in the 1.2-1.7 GHz frequency band. The groups of radio spikes observed clearly show spectral semi-harmonic structures and an intermittent temporal patter. The observational parameters were determined from the dynamic spectra analysis. The wavelet analysis technique able us to determine the temporal cadence for the clusters. The frequency ratio between two clusters of spikes recorded at same time were inferred. The preliminary results show average cadence of clusters of spikes occurrence of about 32 seconds and a semi-harmonic average frequency ratio of the order of 1:1.2.

Affiliated with

Also associated with

No associations

Rating

Semi-harmonic and intermittent solar decimetric spikes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Semi-harmonic and intermittent solar decimetric spikes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Semi-harmonic and intermittent solar decimetric spikes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1095523