Estimating density and magnetic field turbulence in solar flares using radio zebra observations

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00534172" target="_blank" >RIV/67985815:_____/20:00534172 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/202037936" target="_blank" >https://doi.org/10.1051/0004-6361/202037936</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202037936" target="_blank" >10.1051/0004-6361/202037936</a>

Result language
angličtina
Original language name
Estimating density and magnetic field turbulence in solar flares using radio zebra observations
Original language description
In this paper we present a new method for estimating levels of the density and magnetic field turbulence in time and space during solar flares at positions of radio zebra sources. First, considering the double-plasma resonance model of zebras, we describe a new method for determining the gyro-harmonic numbers of zebra stripes based on the assumption that the ratio R = L-b/L-n (L-n and L-b are the density and magnetic field scales) is constant in the whole zebra source. Applying both the method proposed in this work and one from a previous paper for comparison, in the 14 February 1999 zebra event we determined the gyro-harmonic numbers of zebra stripes.
Czech name
—
Czech description
—

Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Similar results(10)