Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow
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Цитувати: | Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow / Yu.I. Dzhezherya, A.I. Tovstolytkin, E.S. Klymuk, L.S. Uspenskaya // Functional Materials. — 2010. — Т. 17, № 3. — С. 363-370. — Бібліогр.: 11 назв. — англ. |
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irk-123456789-1351312018-06-15T03:05:23Z Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow Dzhezherya, Yu.I. Tovstolytkin, A.I. Klymuk, E.S. Uspenskaya, L.S. Modeling and simulation 2010 Article Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow / Yu.I. Dzhezherya, A.I. Tovstolytkin, E.S. Klymuk, L.S. Uspenskaya // Functional Materials. — 2010. — Т. 17, № 3. — С. 363-370. — Бібліогр.: 11 назв. — англ. 1027-5495 http://dspace.nbuv.gov.ua/handle/123456789/135131 en Functional Materials НТК «Інститут монокристалів» НАН України |
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Modeling and simulation Modeling and simulation |
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Modeling and simulation Modeling and simulation Dzhezherya, Yu.I. Tovstolytkin, A.I. Klymuk, E.S. Uspenskaya, L.S. Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow Functional Materials |
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Article |
author |
Dzhezherya, Yu.I. Tovstolytkin, A.I. Klymuk, E.S. Uspenskaya, L.S. |
author_facet |
Dzhezherya, Yu.I. Tovstolytkin, A.I. Klymuk, E.S. Uspenskaya, L.S. |
author_sort |
Dzhezherya, Yu.I. |
title |
Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow |
title_short |
Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow |
title_full |
Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow |
title_fullStr |
Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow |
title_full_unstemmed |
Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow |
title_sort |
autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow |
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НТК «Інститут монокристалів» НАН України |
publishDate |
2010 |
topic_facet |
Modeling and simulation |
url |
http://dspace.nbuv.gov.ua/handle/123456789/135131 |
citation_txt |
Autostabilization of temperature in systems with combined magnetic and resistive transition under electric current flow / Yu.I. Dzhezherya, A.I. Tovstolytkin, E.S. Klymuk, L.S. Uspenskaya // Functional Materials. — 2010. — Т. 17, № 3. — С. 363-370. — Бібліогр.: 11 назв. — англ. |
series |
Functional Materials |
work_keys_str_mv |
AT dzhezheryayui autostabilizationoftemperatureinsystemswithcombinedmagneticandresistivetransitionunderelectriccurrentflow AT tovstolytkinai autostabilizationoftemperatureinsystemswithcombinedmagneticandresistivetransitionunderelectriccurrentflow AT klymukes autostabilizationoftemperatureinsystemswithcombinedmagneticandresistivetransitionunderelectriccurrentflow AT uspenskayals autostabilizationoftemperatureinsystemswithcombinedmagneticandresistivetransitionunderelectriccurrentflow |
first_indexed |
2025-07-09T21:08:37Z |
last_indexed |
2025-07-09T21:08:37Z |
_version_ |
1837205105313579008 |
fulltext |
Functional Materials, 17, 3, 2010 363
-
Autostabilization of temperature in systems
with combined magnetic and resistive transi-
tion under electric current flow
Yu.I. Dzhezherya, A.I. Tovstolytkin,
E.S. Klymuk*, L.S. Uspenskaya**
Institute of Magnetism, National Academy of Sciences of Ukraine and
Ministry for Education and Science of Ukraine,
36-b Vernadsky Blvd., 03142 Kyiv, Ukraine
*National Technical University “KPI”, 37 Peremogy Ave., 03056 Kyiv, Ukraine
**Institute of Solid State Physics, Russian Academy of Sciences, 142432
Chernogolovka, Russia
Received February 16, 2010
It is shown that the active thermostabilization regime can be realized in systems based on
materials exhibiting combined magnetic and resistive phase transition of first order, when the
sample temperature under electric current is self-maintained about the threshold equal to Tc (Tc
is the phase transition temperature). The dependences of the ferromagnetic phase fraction as
well as the sample temperature on the electric and magnetic field have been calculated. The sys-
tem working parameters necessary to realize the active thermostabilization regime have been
determined. It is found that the magnetic field can effectively influence the system temperature
under certain circumstances.
Показано, что на основе материалов с комбинированным резистивно-магнитным фазовым
переходом первого рода может быть реализован режим активной термостабилизации, когда
при протекании электрического тока в образце автоматически поддерживается температура
вблизи порога Tc (Tc – температура фазового перехода). Рассчитаны зависимости доли
ферромагнитной фазы и температуры в образце от электрического и магнитного полей.
Определены рабочие параметры системы, при которых реализуется режим активной
термостабилизации. Установлено, что при определенных условиях магнитное поле
эффективно влияет на температуру системы.
1. Introduction
In recent years, the first order magnetic phase transitions in substituted perovskite manga-
nites R1-xAxMnO3 (R – rare earth, A – alkaline or alkaline-earth element) are under a particular at-
tention [1, 2]. The magnetic phase layering phenomenon observed in such materials is accompanied
by the material separation into regions with different conductivities [3, 4]. So, the low-temperature
ferromagnetic (FM) phase is characterized by high conductivity (as high as that of typical metals),
while the conductivity of high-temperature paramagnetic (PM) phase is several orders lower [4, 5].
This unique combination of the peculiar features of different phases makes it possible to control
the system conductivity by varying the external magnetic field. At the same time, there is a pos-
Yu.I. Dzhezherya et al. / Autostabilization of temperature in systems ...
Functional Materials, 17, 3, 2010 364
sibility to exert influence on the parameters of the phase domain structure by its heating under
electric current [6, 7]. In this work, a mechanism is proposed to realize the active thermostabiliza-
tion regime for the systems based on materials exhibiting combined magnetic and resistive phase
transition of the first order.
2. Theoretical considerations
Let the sample be assumed to be a film of the thickness L. The film can be either in FM or
PM state depending on its temperature. At a certain temperature Тс, the values of thermodynamic
potentials for FM and PM phases (ФFM and ФPM, respectively) become equal to one another; this
means that under particular conditions, the phase coexistence is possible. This process is assumed
to occur through the first-order phase transition, with both magnetization М and conductivity s
exhibiting discontinuous changes. In this case s sFM PM>> .
As the FM phase is characterized by a high magnetization value, its response to external
magnetic field and internal magnetostatic field will be appreciable. That is why the absolute value
and the direction of the external field may affect the temperature at which the transition starts, as
well as the nature of the phase transition itself.
Let the sample initial temperature be much lower than Тс, and the sample is in a single-do-
main state. This condition can be realized easily by applying an external magnetic field Н. If the
field is perpendicular to the film plane, the single-domain state is attained for H M> 4p .
Consider a case when the electric field E e= E x0 is applied to the film. An electric current
starts to flow through the film. As only an insignificant fraction of electrons from the conduction
band near Fermi energy eF takes part in the transfer processes, the electric current exerts no di-
rect influence on the s f s d- -, interband exchange which makes the system turn to the FM state
below the phase transition point Tc .
At the same time, there is a mechanism of indirect influence of electric field on the mag-
netic subsystem, because the electric current flow is accompanied by heat release and the system
heating.
When the sample temperature approaches Тс, the PM phase (i.e. regions of low conductivity)
starts nucleating. A further heating results in the growth of the PM phase fraction which, in turn,
causes the decreasing current density and deceleration of heat release process. The latter even can
become negligibly small when the FM phase volume, VFV , lowers under the percolation threshold
V Vp ~ .0 3 × (V - the sample volume). In this case, the FM phase is a system of isolated domains
surrounded by the PM matrix.
As is shown in [8, 9], it is in the vicinity of the percolation threshold where the sharp conduc-
tivity and, correspondingly, the current density changes occur in a static regime.
To describe the system conductivity qualitatively, we use a series expansion of the effective
conductivity seff over the volume of FM phase near to the percolation threshold. Having neglected
the conductivity of PM phase, we can write:
s
seff
FM p
FM p
V V
V V V
=
<
× -( )
ì
í
ïïï
î
ïïï
0
0
, , (1)
where s0 - the expansion coefficient which is of the same order as sFM .
As follows from Eq. (1), the effective conductivity increases sharply as the volume fraction of
FM phase exceeds the percolation threshold. This effect can be used to develop the active thermo-
stabilization regime for the system.
The task will be solved in two steps.
3. The film phase layering in a perpendicular field
When solving the problem of phase layering for the film in a perpendicular field, let us as-
sume that the film thickness L exceeds considerably the domain structure period P:
Yu.I. Dzhezherya et al. / Autostabilization of temperature in systems ...
Functional Materials, 17, 3, 2010 365
L P>> (2)
This allows us to make two important simplifications. On the one hand, such assumption will
make it easier to determine the dependence of the FM phase volume on temperature and external
field. On the other hand, it will allow us to neglect the nonuniformity in the temperature distribu-
tion within the film plane when we solve the problem of heat exchange between the film and the
surrounding medium.
As follows from Eq. (1), in the vicinity of the percolation threshold, the system conductivity
heavily depends on the FM phase fraction. That is why we will concentrate attention on the deter-
mination of the V VFM dependence on the system temperature and external field.
That dependence can be obtained from the condition of energy minimum for a magnetic sub-
system, which is given by the following expression in the case under consideration [10, 11]:
D SE dv Sm
VFM
= - × - ×( )+ ×ò e M H M H 2 , (3)
where e = - -F FFM PM is the difference of the thermodynamic potentials for FM and PM phases,
respectively, which can be presented in the vicinity of the phase transition point as a series ex-
pansion over temperature: e = -( )k T Tc . Here, k- is the expansion coefficient (a phenomenologi-
cal parameter); Tc, the temperature at which the thermodynamic potentials of the phases become
equal to one another; M = M ∙ ez, the magnetization of FM phase; H = H ∙ ez, the external magnetic
field directed perpendicular to the film plane; Hm, magnetostatic field of the sample; S, S, the sur-
face energy density and the total area of the phase interfaces, respectively. Integration in expres-
sion (3) is carried out over the volume of FM phase. The form of the expression (3) implies that the
crystallographic anisotropy is neglected.
For a system, a fragment of which is shown in Fig. 1, the magnetostatic field is about
H M em FM zM V V»- =- ×( )4 4p p , when the condition L P>> is met. As a result, the integral
(3) can be easily calculated:
D SE
V
MH k T T V
V
M V
V
Sc
FM FM»- - -( )( ) +
æ
è
ççç
ö
ø
÷÷÷÷ + ×2 2
2
p . (4)
The total interface area depends on the characteristic period of domain structure rather than
on the FM phase volume. Therefore, the V VFM value can be easily determined from the condition
of the system magnetic energy minimum (see Eq. (4)):
V
V
HM k T T
M
FM c=
- -( )
4 2p
. (5)
Since the FM phase relative volume varies from zero to unity, the system temperature in the
phase separation regime lies within the range:
T T MH k T T MH kc M c- + < < + . (6)
Here, to make the expression more explicit, a temperature parameter T M kM = 4 2p is introduced.
This parameter determines the width of the temperature interval where the FM and PM phases
coexist.
The k parameter value can be determined in an indirect way, for example, using the experi-
mental results from [8, 9]. According to these data, for the Ca-substituted perovskite manganites
with M ~ 320 G and Tc ~ 240 K, the percolation onset temperature rises with the magnetic field
increase at an average rate of 0.8 K/kOe. This corresponds to the value of k ~ 4 105× erg⋅cm–3⋅K–1.
So, for the material considered in [9], the temperature interval of the phase coexistence should
be TM ~ .2 5 K. However, the experimentally observed value is several times larger than that es-
Yu.I. Dzhezherya et al. / Autostabilization of temperature in systems ...
Functional Materials, 17, 3, 2010 366
timated in the above way. This effect, at least in
part, may originate from the inhomogeneous Ca
ion distribution over the sample volume. As a re-
sult, Tc displays a considerable space dispersion.
Such a dispersion can no doubt influence sig-
nificantly the course of the phase transition. How-
ever, the account for this effect is beyond the scope
of this work. In what follows, we will concentrate
on the development of the approach for a hypothet-
ical, ideally homogeneous material.
The Eq. (5) links the sample phase compo-
sition with the system temperature and magnetic
field. As the main task of this work is to describe
the active thermostabilization regime, we should supplement the system of equations by those of a
heat balance with the surrounding medium.
4. Temperature distribution and heat balance conditions
When determining the equilibrium distribution of phases (see Eq. (5)), we assumed that the
sample temperature is the same over its whole volume. In practice, such a condition can be satisfied
only under a certain approximation.
For the system shown fragmentarily in Fig. 1, the temperature distribution inhomogeneities
originate from a spatial inhomogeneity of conductivity resulting from the phase separation, as well
as from a permanent heat exchange with the surrounding medium across the film surface. How-
ever, for some particular relationships between physical and geometrical parameters of a magnetic
film and thermo-isolating layer, the temperature distribution inhomogeneity can be neglected.
To derive the equation of thermal balance and determine the condition when the tempera-
ture field can be considered as homogeneous, let us consider the heat conduction equation:
c T
t
x y T x yr k s¶
¶
-Ñ ( )×Ñ( )= ( ), , E2 , (7)
where k sx y x y, , ,( ) ( )-are the film heat conduction coefficient and conductivity, modulated in the
xOy plane; c, r, the material heat capacity and density being practically independent of whether
the film is in a phase separated state or not; Ñ= ¶ ¶e xi i ; the right part of Eq. (7) takes into ac-
count the power of heat sources in a sample.
Let us solve the problem of the temperature distribution determination in a simplified way,
assuming the thermostat temperature to be constant and equal to Te . Under such conditions, the
system will eventually achieve a thermal balance with ¶ ¶ =T t 0 .
At a stationary regime, the latent heat of a phase transition present in dynamics and accom-
panying the changes in the sample phase distribution is also insignificant. This allows us to exclude
the temporal part of the task and concentrate attention on the study of the spatial temperature
distribution.
It should be noted that for the regime settled, the heat conduction problem will include two
dimensional parameters, the domain structure period P in the film plane and the film thickness L.
To simplify the form of the expressions, we introduce the variables: ρρ= +( ) =x y P z Lx ye e , z .
The heat conduction equation takes the form:
¶
¶
( )× ¶
¶
æ
è
çççç
ö
ø
÷÷÷÷ =
æ
è
ççç
ö
ø
÷÷÷÷ × - ( )¶
¶
- ( )
ρρ
ρρ ρρ ρρk
r
k
z
sT P
L
T
2 2
2 E22 2L
æ
è
ççççç
ö
ø
÷÷÷÷÷
. (8)
As follows from expression (2), the right part of Eq. (8) is a correction squared with respect to
the small parameter P L . Thus, the solution of Eq. (8) can be written as a series expansion over
P L( )2 :
Fig. 1. A fragment of the sample with the ferro-
magnetic phase domains (schematic view).
Yu.I. Dzhezherya et al. / Autostabilization of temperature in systems ...
Functional Materials, 17, 3, 2010 367
T T P L Tρρ ρρ, , ...z z z( ) = ( )+( ) × ( )+0
2
1 (9)
The unknown function T0 x( ) should be fitted to satisfy the Fredholm alternative for a non-
uniform equation:
¶
¶
( )× ¶
¶
æ
è
çççç
ö
ø
÷÷÷÷ =- ( )
¶ ( )
¶
- ( )
ρρ
ρρ
ρρ
ρρ ρρk k
z
z
s
T T
L1
2
0
2
2 2E . (10)
In our case, the necessary and sufficient condition for obtaining a non-trivial solution of this
equation is that the average value of the right part of Eq. (10) is zero in the xOy-plane:
¶ ( )
¶
=-
( )
( )
×
2
0
2
2
2T E
L
z
z
s
k
ρρ
ρρ
__________
________ . (11)
Here, the overbars mean averaging over the film plane.
The calculation of k ρρ( )
______
is quite easy and results in
k k k k kρρ( ) = = + -( )×( )
______
eff PM FM PM FMV V .
However, the determination of the average power of heat sources, s ρρ( )E2
___________
, is troublesome, be-
cause both the conductivity and local electric field intensity depend considerably on the state of
the phase domain system. However, since the sharp discontinuities of the conductivity and heat
producing are observed near the percolation threshold, let us use the phenomenological formula of
the conductivity expansion (1) and introduce the average capacity of heat sources in the form:
s
s
ρρ( ) =
-( ) >
<
ì
í
ïïï
î
ïïï
E E V V V V V
V V
FM P FM P
FM P
2 0 0
2
0
___________ ,
,
(12)
Now the solution of Eq. (8), symmetrical relative to the z = 0 plane, can be presented as
T z T E z V V
Veff
FM P
0 0
0 0
2 2
0
2
( ) = ( )-
×
×
-s
k
, (13)
where T0(0) is the integration constant which is determined from the condition of the heat flux con-
tinuity in the direction perpendicular to the film surface:
k keff
e
z L
T z
z
T T z
h
¶ ( )
¶
=
- ( )
=
0
0
0
2
. (14)
So, the temperature distribution within the film is determined by the expression:
T z T V V
V
z L
L he
FM P
eff
0
0
2
1
2
( ) = + ×
-
× - ×
-( )
×
æ
è
çççççç
ö
ø
÷÷÷÷÷÷÷
Q
k
k
, (15)
where the designation Q=
×
s
k
0 0
2
02
E Lh is introduced. It is this quantity that is an important heat
parameter of the problem. It has the temperature dimensionality and characterizes the sample
heating process resulted from the electric current. Its value grows with the increase in both the
thermal isolation efficiency ( h k0 ) and heat source intensity (s0 0
2E ).
It follows from (15) that the increase in the thermo-isolating parameter k keff 0 gives rise to
more homogeneous temperature distribution over the sample.
At this stage, we can formulate the condition that, being satisfied, enables us to consider the
temperature distribution as a homogeneous one over the whole film volume. It is clear that the
temperature modulation over the film thickness should be considerably less than the temperature
interval of a magnetic phase transition:
Yu.I. Dzhezherya et al. / Autostabilization of temperature in systems ...
Functional Materials, 17, 3, 2010 368
V V
V
L
h
TFM P
eff
M-
× <<
k
k
0
4 Q
. (16)
Then, as follows from the expression (15), we can neglect the temperature changes within the film
thickness and consider the sample temperature T to be constant within the whole volume, so
T T V V Ve FM p= + × -( )Q . (17)
As was mentioned above, this approach is correct in the vicinity of the percolation threshold
when V V VFM p-( ) <<1 . Therefore, taking into account that the material temperature in a phase
separated state is close to Tc , it follows from (17) that:
V V
V
T TFM p c e- -
<<~
Q
1 . (18)
This condition can be satisfied in various ways, for example, by increasing the system ther-
mal insulation or raising the electric field intensity.
Thus, expressions (5) and (17) give the solution of the problem under consideration, which
makes it possible to determine the temperature Т and the fraction of the FM phase V VFM in the
sample using the preset intensity values of the electric and magnetic fields:
V V
V
H M V V T T T
T
T Tc
TM
H M Vp V Tc Te
T
FM p p c e M
M
-
=
- + -( )
+
-
=
- - -( )
+
4
1
4
1
p
p
Q
Q
MM Q
.
(19)
The condition (16) for the applicability of the theory results, i.e. the condition which deter-
mines if the temperature distribution over the sample can be considered as homogeneous over the
whole volume, takes the form:
H M T T T V V
T
h
L
c e M p
M
eff4
1
4
0
p k
k
+ -( ) -
+
<<
Q
. (20)
In other words, this result implies that high heat conductivity of a material and good ther-
mal insulation of a system, both favor the homogeneous temperature distribution over the sample
volume.
It follows from Fig. 2 that for great values of Q TM , the film temperature responses weak-
ly to the temperature of the surrounding medium. So, for Q TM ~ 150 , even the change of the
temperature of the surrounding medium by DT Te M~ ~20 50 K results in the film temperature
Fig. 2. Dependence of the sample temperature Т on
the heat parameter Q=
×
s
k
0 0
2
02
E Lh . The two lower
curves are plotted for magnetic field H M= 4p ,
and correspond to different values of the thermo-
stat temperature Te . The upper pair of curves is
built for magnetic field H M= 8p for the same
thermostat temperatures.
Yu.I. Dzhezherya et al. / Autostabilization of temperature in systems ...
Functional Materials, 17, 3, 2010 369
change by DT TM~ . ~ .0 1 0 25 K . At the same time, the film temperature can be effectively tuned
by means of external magnetic field. For the case where Q TM is sufficiently great, an asymptoti-
cal approximation
T Tc TM H M Vp V- = × -( )4p (21)
can be used. According to this approximation, the magnetic field strength increase by DH M= 4p
brings about the rise of the film temperature by DT TM~ .
5. Conclusion
Thus, the active thermal stabilization regime can be realized in the systems with combined
magnetic and resistive phase transition of the first order placed in a perpendicular magnetic field
with electric current flowing through the film.
As a concluding remark, let us note that electric current influences the system magnetic
susceptibility. In fact, as the system average magnetization is M M V Vz FM= × , we can find
c
p
= =
+( )
d M
dH T
z
M
1
4 1Q
, (22)
with taking into account expression (19). It follows from Eq. (22) that the system susceptibility
decreases with the increasing heat parameter Q TM .
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Yu.I. Dzhezherya et al. / Autostabilization of temperature in systems ...
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Автостабілізація температури
у матеріалі з резистивно-магнітним
фазовим переходом першого роду
при протіканні електричного струму
Ю.І.Джежеря, O.І.Товстолиткін
О.С.Клімук, Л.С.Успенська
Показано, що на основі матеріалів з комбінованим резистивно-магнітним фазовим
переходом першого роду може бути реалізований режим активної термостабілізації, коли
під час протікання електричного струму у зразку автоматично підтримується температура
поблизу порогу Tc (Tc – температура фазового переходу). Розраховано залежності частки
феромагнітної фази та температури у зразку від електричного та магнітного полів.
Визначено робочі параметри системи, за яких реалізується режим активної термостабілізації.
Встановлено, що за визначених умов магнітне поле ефективно впливає на температуру
системи.
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