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首页> 外文期刊>The Astrophysical journal >A MODEL OF ZEBRA EMISSION IN SOLAR TYPE Ⅳ RADIO BURSTS
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A MODEL OF ZEBRA EMISSION IN SOLAR TYPE Ⅳ RADIO BURSTS

机译:太阳能Ⅳ型爆发的斑马发射模型。

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摘要

Solar type Ⅳ radio bursts present a theoretical challenge because they are composed of both continuum emission and fine structures. The latter include " zebra bursts," which appear as harmonically spaced multi-plets that shift in frequency with time. Similarities between these features and terrestrial auroral emissions suggest a new model to explain zebra-structured type IV emissions. In this model, the basic generation mechanism is identical with that proposed by Winglee and Dulk: mode conversion of Z-mode waves generated by the cyclotron maser mechanism under the condition f_(uh) ― Nf_(ce), with N an integer; however, we propose a twist on this model whereby the " zebra bursts" do not arise from multiple N-values. Rather, the presence of localized density irregularities within the type IV leads to trapping of the upper hybrid Z-mode waves in density enhancements, which results in a discrete spectrum of upper hybrid modes with nearly constant frequency spacing. The number m of quasi-harmonics is limited by the trapping (quantization) conditions. The problem is described by an equivalent Schroedinger equation for the trapped mode, which is solved for an (idealized) cylindrical square density irregularity. In this model, the eigenfrequency spacing matches the observed type IV frequency spacings for less than 10% density enhancements with individual scale sizes of 30-1000 thermal electron gyroradii, corresponding to 1-100 m scales in coronal loops. To produce the observed emitted power for a reasonable (< 1%) efficiency requires a large number of such individual microscopic sources occurring over a portion of a magnetic type IV loop at a restricted altitude within which the magnetic field and density are approximately constant. The loop plasma in the zebra emission source is thus highly turbulent in the sense that it contains a large number of density fluctuations. In this case transition radiation can effectively contribute to the radiation background and may also provide the wave power required in the upper hybrid range for generating zebra emissions.
机译:太阳Ⅳ型无线电爆发是一个理论挑战,因为它们由连续发射和精细结构组成。后者包括“斑马爆发”,出现为谐波间隔的多小波,随时间变化频率。这些特征与地面极光排放之间的相似性表明了一种新的模型来解释斑马结构的IV型排放。在该模型中,基本的产生机制与Winglee和Dulk提出的机制相同:在条件f_(uh)〜Nf_(ce)下,回旋加速器maser机制产生的Z模波的模转换,其中N为整数。但是,我们对此模型提出了一种扭曲,即“斑马纹”不是由多个N值引起的。相反,IV型内存在局部密度不规则会导致上混合Z模波在密度增强中的陷获,从而导致上混合模的离散频谱具有几乎恒定的频率间隔。准谐波的数量m受陷波(量化)条件的限制。该问题由陷波模式的等效Schroedinger方程描述,该问题针对(理想化的)圆柱正方形密度不规则度求解。在此模型中,本征频率间隔与观察到的IV型频率间隔匹配,不足以10%的密度增强,而单个尺度的大小为30-1000个热电子陀螺半径,相当于日冕环中的1-100 m尺度。为了以合理的效率(<1%)产生观测到的发射功率,需要在有限的高度(磁场和密度大致恒定)内的IV型磁性回路的一部分上出现大量的此类单个微观源。斑马发射源中的环形等离子体因此在其包含大量密度波动的意义上是高度湍流的。在这种情况下,过渡辐射可以有效地贡献于辐射背景,并且还可以提供在较高混合范围内产生斑马辐射所需的波功率。

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