All Figures

$\begin{figure} \par\hbox to \hsize{\hfill a)\epsfig{file=MS4049f1a.eps,scale=0.3... ...mm}b)\raisebox{5mm}{\epsfig{file=MS4049f1b.eps,scale=0.3} }\hfill}\end{figure}$ Figure 1: Source model from optical, X-ray and radio measurements (see Paper I). a) The loop LS1 is the main source of BBP and ZP: fast electron streams exciting BBP are injected at the SW footpoint. ZP stripes arise at the DPR levels (stippled) in the NE part of LS1. b) Enlargement of the encircled SW range: the leading spot in conflict with the emerging parasitic polarity loop (EL). The wavy circle is a site of reconnection and electron acceleration.
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In the text

$\begin{figure} \par\hbox to \hsize{\hfill\hspace{5mm}\raisebox{-2ex}{a)}% \epsfi... ...}\raisebox{-2ex}{c)}% \epsfig{file=aa4049f2c.eps,scale=0.58}\hfill} \end{figure}$ Figure 2: The DPR source of ZP: a) gyroharmonics sf_B and plasma frequency $f_{\rm p}$ via height h. Intersection points are DPR levels. b) Positive frequency drift due to magnetic field decrease. Solid sf_B(t₁) and dotted sf_B(t₂) are gyroharmonics at times t₂>t₁. The DPR level moves to higher frequencies. c) Frequency drift due to plasma cooling. Solid and dotted $f_{\rm p}$ are plasma frequency at t₂ and t₁. The decrease of the scale of $f_{\rm p}$ (and of electron density) results from plasma cooling ( T(t₂)<T(t₁)). Again, the DPR level moves to higher frequencies.
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In the text

$\begin{figure} \par\hbox to \hsize{\hfill \raisebox{-2ex}{a)}% \epsfig{file=aa40... ...aisebox{-2ex}{b)}% \epsfig{file=aa4049f3b.eps,scale=0.6} % \hfill}\end{figure}$ Figure 3: Magnetic field line selected from extrapolated LS1 (see Fig. 2 of Paper I): a) perspective view; b) height dependence of field strength.
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In the text

$\begin{figure} \par\hbox to \hsize{\hfill\epsfig{file=MS4049f4.eps,scale=0.3} % \hfill}\end{figure}$ Figure 4: The dynamic spectrum of ZP 10:08: $20 \div 10$ :08:50. The white dotted line enhances the time evolution of a single zebra stripe (s=17 according to our counting). Dark dotted lines mark two instantaneous spectra used in Fig. 5.
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In the text

$\begin{figure} \par\hbox to \hsize{\hfill \raisebox{-2ex}{a)}% \epsfig{file=aa40... ...m}\raisebox{-2ex}{b)}% \epsfig{file=aa4049f5b.eps,scale=.9}\hfill}\end{figure}$ Figure 5: Observations versus theory: horizontal lines are peak frequencies of zebra stripes. A grid of gyroharmonics $s = 11\div 27$ is plotted using the field along the selected extrapolated field line (Fig. 3). Intersections are marked by dots and represent the DPR levels. Thick line is the barometric plasma frequency (electron density) law over height for a) the spectrum at 10:08:23 UT ( $T=1.18\times 10^6$ K); b) the spectrum at 10:08:33 UT ( $T=0.80\times 10^6$ K). The dotted line in b) is the thick line of a).
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In the text

$\begin{figure} \par\hbox to \hsize{\hfill\epsfig{file=aa4049f6.eps,scale=0.7}\hfill}\end{figure}$ Figure A.1: Plasma waves perpendicular to the magnetic field in the equilibrium plasma: qualititative dispersion curves for Bernstein modes and plasma waves at the frequency of upper hybrid resonance. Straight lines mark the instability boundaries for two different ratios $v_{\rm e}/v_{\rm T}$ at $s\simeq 15$ .

In the text

$\begin{figure} \par\hbox to \hsize{\hfill a)\epsfig{file=aa4049f7a.eps,scale=0.75} % \hspace*{5mm}b)\epsfig{file=aa4049f7b.eps,scale=0.75}\hfill}\end{figure}$ Figure B.1: The growth rate of the waves in the hybrid band $14<\omega _{\rm uh}/\omega _B<15$ for $v_{\rm e}/v_{\rm T}=20$ : a) $k_{\perp }$ -dependence of $\gamma$ for the optimal values of $k_{\parallel }$ ; b) the dependence of maximum growth rate on the position of $\omega$ inside the hybrid band.

In the text

$\begin{figure} \par\hbox to \hsize{\hfill \raisebox{-2ex}{a)}% \epsfig{file=aa40... ...aisebox{-2ex}{b)}% \epsfig{file=aa4049f3b.eps,scale=0.6} % \hfill}\end{figure}$	Figure 3: Magnetic field line selected from extrapolated LS1 (see Fig. 2 of Paper I): a) perspective view; b) height dependence of field strength.
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$\begin{figure} \par\hbox to \hsize{\hfill\epsfig{file=MS4049f4.eps,scale=0.3} % \hfill}\end{figure}$	Figure 4: The dynamic spectrum of ZP 10:08: $20 \div 10$ :08:50. The white dotted line enhances the time evolution of a single zebra stripe (s=17 according to our counting). Dark dotted lines mark two instantaneous spectra used in Fig. 5.
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