Debye Shielding - Histórico de revisões

Ist426982 em 19h36min de 2 de março de 2017

2017-03-02T19:36:39Z

2017-03-02T19:36:09Z

2017-03-02T19:31:45Z

2017-02-19T15:39:47Z

2017-02-19T15:39:26Z

2017-02-19T15:39:14Z

2017-02-19T15:37:11Z

2017-02-19T15:35:34Z

2017-02-19T15:34:31Z

2017-02-19T15:03:19Z

@@ Linha 18: / Linha 18: @@
 (F. F. Chen ~ 1.3) On a log-log plot of \(n\) [\(m^{-3}\)] vs kTe (eV) draw lines
-of constant \(\lambda_D\) and \(Lambda\). On the graph place the following points:
+of constant \(\lambda_D\) and \(\Lambda\). On the graph place the following points:
 a) Tokamak (\(T_{e}\) \(\simeq\) 1 keV, \( n_e\simeq10^{13} \, cm^{-3} \))

@@ Linha 18: / Linha 18: @@
 (F. F. Chen ~ 1.3) On a log-log plot of \(n\) [\(m^{-3}\)] vs kTe (eV) draw lines
-of constant \(\lambda_D\) and \(N_D\). On the graph place the following points:
+of constant \(\lambda_D\) and \(Lambda\). On the graph place the following points:
 a) Tokamak (\(T_{e}\) \(\simeq\) 1 keV, \( n_e\simeq10^{13} \, cm^{-3} \))

@@ Linha 18: / Linha 18: @@
 (F. F. Chen ~ 1.3) On a log-log plot of \(n\) [\(m^{-3}\)] vs kTe (eV) draw lines
-of constant \(\lambda_D\) and \(\Delta\). On the graph place the following points:
+of constant \(\lambda_D\) and \(N_D\). On the graph place the following points:
 a) Tokamak (\(T_{e}\) \(\simeq\) 1 keV, \( n_e\simeq10^{13} \, cm^{-3} \))

@@ Linha 40: / Linha 40: @@
 (b)
 </div>
 </div>

@@ Linha 38: / Linha 38: @@
 <div class="mw-collapsible-content">
 (a)
 (b)
 </div>
 </div>

@@ Linha 37: / Linha 37: @@
 '''Answer'''
 <div class="mw-collapsible-content">
-(a) \(x \) particles and (b) \(3\) particles
+(a)
 </div>
 </div>

← Revisão anterior		Revisão das 15h37min de 19 de fevereiro de 2017
Linha 27:		Linha 27:

	d) Laser fusion (\( T_e \simeq 1 \; keV, \, n_e\simeq 10^{20} cm^{-3} \) )		d) Laser fusion (\( T_e \simeq 1 \; keV, \, n_e\simeq 10^{20} cm^{-3} \) )
		+
		+	e) Gaseous electronics (\( T_e \simeq 1 \; eV, \, n_e\simeq 10^{10} cm^{-3} \) )
		+
		+	f) Interstellar medium (\( T_e \simeq 1 \; eV, \, n_e\simeq 10^{-1} cm^{-3} \) )
		+
		+	g) Flame (\( T_e \simeq 0.1 \; eV, \, n_e\simeq 10^{8} cm^{-3} \) )

	<div class="toccolours mw-collapsible mw-collapsed" style="width:210px">		<div class="toccolours mw-collapsible mw-collapsed" style="width:210px">

@@ Linha 26: / Linha 26: @@
 c) Ionosphere, ~ 300 km above Earth’s surface ( \( T_e \simeq0.1eV, \, n_e\simeq 10^6 \, cm^{-3} \))
-d) Laser fusion (\( T_e \simeq 1 keV, \, n_e\simeq 10^{20} cm^{-3} \) )
+d) Laser fusion (\( T_e \simeq 1 \; keV, \, n_e\simeq 10^{20} cm^{-3} \) )
 <div class="toccolours mw-collapsible mw-collapsed" style="width:210px">

← Revisão anterior		Revisão das 15h34min de 19 de fevereiro de 2017
Linha 25:		Linha 25:

	c) Ionosphere, ~ 300 km above Earth’s surface ( \( T_e \simeq0.1eV, \, n_e\simeq 10^6 \, cm^{-3} \))		c) Ionosphere, ~ 300 km above Earth’s surface ( \( T_e \simeq0.1eV, \, n_e\simeq 10^6 \, cm^{-3} \))
		+
		+	d) Laser fusion (\( T_e \simeq 1 keV, \, n_e\simeq 10^{20} cm^{-3} \) )

	<div class="toccolours mw-collapsible mw-collapsed" style="width:210px">		<div class="toccolours mw-collapsible mw-collapsed" style="width:210px">

@@ Linha 24: / Linha 24: @@
 b) Solar wind near the Earth ( \( T_e \simeq 10 eV, n_e\simeq10 \, cm^{-3} \) )
-c) Ionosphere, ~ 300 km above Earth’s surface ( \( T_e \simeq0.1eV, \, n_e\simeq 10^6 \n cm^{-3} \))
+c) Ionosphere, ~ 300 km above Earth’s surface ( \( T_e \simeq0.1eV, \, n_e\simeq 10^6 \, cm^{-3} \))
 <div class="toccolours mw-collapsible mw-collapsed" style="width:210px">