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Publié par | ernst-moritz-arndt-universitat_greifswald |
Publié le | 01 janvier 2009 |
Nombre de lectures | 11 |
Langue | English |
Poids de l'ouvrage | 2 Mo |
Extrait
geb
F
Sim
rer.
ulations
orgelegt
of
Indien
Dust
y
ersit?t
Plasmas
enk
I
in
n
er
a
an
u
g
der
u
ald
r
on
a
Ramana
l
am
d
alurip
i
ald,
s
(Dr.
s
nat.)
e
der
r
t
hen
a
akult?t
t
Ernst-Moritz-Arndt-Univ
i
Greifsw
o
v
n
v
zur
V
Erlangung
ata
des
Ikkurthi
ak
oren
01.08.1976
hen
Chilak
Grades
et,
do
Greifsw
Octob
rerum
2009
naturaliumag
Dek
vid
an:
............................
Prof.
y
Dr.
-
Klaus
Dr.
F
skhak
esser
.............................................
..............................................
Promotion:
1.
-
ter:
h
Da
ter
T
:
a
Prof.
a
Dr.
T
Andr?
der
Melzer
14
.................................................
12
2.
2009
hDer Weg ist das Ziel
(The path is the destination /the destination is not
important, but the path that leads there)
(Knowledge cannot be stolen by thieves,
It cannot be forcibly snatched by kings,
It cannot be devided among brothers,
It does not cause a load on shoulders,
If spent or shared, it indeed always keeps on growing.
The wealth of knowledge... is the most superior wealth of all!)
o
&
Lillu
T
Chikki3P M
and
b
a
tly
plasma
study
of
oating
has
harge
The
and
t
ion
rf
drag
the
force
to
on
with
b
sized
dust
particles
and
immersed
ulations
in
of
rf
p
disc
bulk
harges.
presheath
Kno
to
wledge
dust
of
nonlinear
dust
assumed
parameters
enden
lik
are
e
All
dust
e
is
harge,
et
oating
dom-
p
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oten
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shielding
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ion
drag
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force
v
is
higher
v
the
ery
the
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for
the
explaining
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lab
h
oratory
the
dust
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y
a
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eried
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h
dust
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erimen
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oid
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formation
een
in
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it
een
y
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t.
erimen
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ts
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ak
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eeld
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formation
dust
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arious
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Existing
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in
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ux
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sp
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ecies
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and
oten
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v
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er
endence
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oten
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o
endence
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v
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and
een
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y
.
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sim
the
ulations
dust
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ols
ts.
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and
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hange
aim
b
of
w
this
ions
the-
neutrals
sis
eing
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inan
to
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p
ion
erform
are
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sim
heating
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hanism
using
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P
ha
e
een
to
(
the
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parameters
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v
sizes
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lo
)
at
mo
t
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ositions
to
the
understand
disc
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w
harge
the
oating
dust
oten
parameters
in
v
presheath
ary
sligh
for
larger
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the
t
alues
p
the
ositions
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the
dust
electron
in
to
rf
dust
disc
in
harges
presheath.
and
rom
ho
to
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sheath
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parameters
and
on
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a
tial
dust
alues
ev
due
olv
the
e
of
in
electron
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t
the
of
A
neigh
dep
b
of
oring
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dust
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particles.
dust
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has
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rst,
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results
disc
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in
of
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e
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e
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de
tly
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ting
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y
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relev
an
parameters
t
also
to3P M
to
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lo
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are
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particles
ulated
t
dust
ph
oating
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oten
axis
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are
ion
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w
v
dust
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a
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from
to
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yd-Reynolds
disc
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the
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dier
and
dust
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the
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upp
mo
w
dels,
ell
but
ts
m
MD
uc
plasmas.
h
to
smaller
parameters
than
of
the
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v
t
alues
.
obtained
from
separation.
Orbit
ultiple
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p
Limited
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or
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The
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oten
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tial
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ers,
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particles
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ers
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es
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y
plasmas.
fully
k
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el-lik
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rev
The
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lengths
y
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or
et
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een
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ion
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and
aected
electron
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smaller
y
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e
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lengths.
the
F
on
urther,
particles
the
dieren
orbital
in
drag
and
force
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is
also
t
found
ypically
harges
larger
ultiple
than
the
the
do
uc
drag
single
force.
at
The
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total
harges
drag
dust
force
in
for
dier
the
dust
Due
is
in
larger
la
than
ion
for
to
the
the
la
in
and
v
it
as
scales
nonlinearly
are
with
as
the
exp
dust
dust
size.
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used
(PIC
drag
v
study
alues
of
and
in
sim
agrees
that
with
v
Zobnin's
the
mo
sheath.
del
℄
dust
The
the
their
harging
size.
and
particle
drag
harging
force
neigh
when
is
within
then
In
extended
ion
to
t
dust
w
onen
o
of
and
drag
m
not
ultiple
static
This
dust
attributed
particles
the
in
the
parameter
rf
alues
disc
to
harge
dust
to
Then
study
dust
the
harges
m
of
dust
neigh
lo
b
at
oring
t
dust
ositions
particles
the
on
harge
the
arranged
dust
the
parameters.
harge
Initially
are
,
the
is
dust
that
parameters
on
of
t
m
w
dust
o
in
dust
bulk
particles
presheath
are
not
m
for
h
v
the
arious
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in
alues
that
separation
the
and
for
of
dust
ultiple
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particles
placed
at
the
dieren
t
from
lo
single
parameter
in
alues.
the
to
rf
fo
disc
from
harge.
particles
It
the
is
er
observ
y
ed
the
that
for
dust
dust
separations
in
larger
lo
than
er
the
y
shielding
resulting
length
smaller
the