Accepted Manuscript Dynamic properties of micro-magnetic noise in soft ferromagnetic materials A. Stupakov, A. Perevertov PII: DOI: Reference:
S0304-8853(17)33849-0 https://doi.org/10.1016/j.jmmm.2018.02.069 MAGMA 63746
To appear in:
Journal of Magnetism and Magnetic Materials
Please cite this article as: A. Stupakov, A. Perevertov, Dynamic properties of micro-magnetic noise in soft ferromagnetic materials, Journal of Magnetism and Magnetic Materials (2018), doi: https://doi.org/10.1016/ j.jmmm.2018.02.069
This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain.
Dynamic properties of micro-magnetic noise in soft ferromagnetic materials A. Stupakova,∗, A. Perevertova a
Institute of Physics of the Czech Academy of Sciences, Na Slovance 2, 18221 Prague, Czechia
Abstract Dynamic response of magnetic hysteresis, magnetic Barkhausen noise and magneto-acoustic emission in a soft ribbon and electrical steels was studied comprehensively. The measurements were performed under controllable magnetization conditions: sinusoidal/triangular waveforms of the magnetic induction and a triangular waveform of the magnetic field. Magnetizing frequency was varied in a wide range: fmag = 0.5 − 500 and 0.1 − 100 Hz for the ribbon and the electrical steels, respectively. Magnetization amplitude was fixed on a near-saturation level Hmax ≃ 100 A/m. Barkhausen noise signal was detected by a sample-wrapping/surface-mounted coil and differently filtered. It was found that intensity of the Barkhausen noise rises approximately as a square root function of the magnetizing frequency. Whereas, level of the magneto-acoustic emission follows the hysteresis loss trend with an additional linear term (classical loss component). Keywords: Magnetization dynamics, Barkhausen noise, Magneto-acoustic emission, Magnetic hysteresis, Electrical steel
∗ Corresponding author. Tel: +420 26605 2114 E-mail:
[email protected], URL: www.fzu.cz/˜stupak
Preprint submitted to Journal of Magnetism and Magnetic Materials
February 21, 2018
1
1. Introduction
2
The classical problem of macroscale magnetization dynamics in conven-
3
tional ferromagnetic materials has not been fully understood so far. In partic-
4
ular, magnetic hysteresis in soft magnetic materials is commonly discussed in
5
terms of a phenomenological loss-separation model in spite of growing crit-
6
icism of dubious theory assumptions for a classical loss component and of
7
unclear nature of an excess loss [1, 2]. Promising direction of research that
8
should contribute in elucidation of this classical problem is investigation of
9
the magnetization dynamics on a microscale level by measuring Barkhausen
10
noise (BN) and magneto-acoustic emission (MAE). The BN/MAE signals
11
originate from irreversible motion of the magnetic domain walls (DW) and
12
are detected in the form of magnetic/acoustic impulses. Principal distinc-
13
tion between BN and MAE is that the motion of the 180◦ DWs should not
14
cause any change of the magneto-elastic energy and therefore should not con-
15
tribute to MAE [3, 4]. Local jumps of the magnetic DWs between material
16
pinning sites such as grain boundaries, inclusions and defects are damped by
17
microeddy currents, which give a considerable contribution to the hysteresis
18
losses [5]. Thereby, acquiring extensive knowledge about the magnetization
19
process on the microscopic scale builds a necessary base for deeper under-
20
standing of the dynamic properties and for better prediction of the magnetic
21
losses in electrical transformers and motors.
22
Dynamic properties of BN/MAE have been scantily investigated so far.
23
This is especially true for the measurements under controllable magnetization
24
conditions providing physically interpretable results [4, 6]. In this work,
25
we first present the dynamic data for a nanocrystalline soft ribbon with 2
26
a specific combination of the magneto-mechanical properties making this
27
investigation especially attractive. The principal issue is that a tiny thickness
28
of the ribbon and its high electrical resistivity suppress eddy currents and
29
ensure the homogeneous BN detection. Moreover, the long ribbon can be
30
homogeneously magnetized in a solenoid up to high magnetizing frequencies;
31
and its magnetic field can be easily controlled using the magnetizing current.
32
To ensure consistency of the data and profound analysis of the magnetization
33
dynamics, the measurements are additionally performed for soft electrical
34
steels in another magnetizing configuration.
35
2. Experimental
36
2.1. Ribbon
37
The measurements were performed for an as-cast nanocrystalline Hitperm
38
ribbon with the following composition: Fe54 Co27 Nb7 B12 [7]. It was chosen
39
because of the similar grain structure as industrial ferromagnetic steels. To
40
receive evidence that the data obtained for this ribbon demonstrate a gen-
41
eral trend, other ribbons from the same Hitperm series with different Fe-
42
Co composition and a few industrial samples were additionally tested. The
43
tested ribbon was 1 m long, 7 mm wide and 10 µm thick. It was mag-
44
netized inside a 30-cm long solenoid; the magnetic field H was calculated
45
from the current in the solenoid winding. A sample-wrapping coil of 4 cm
46
length and 2700 turns was positioned in the solenoid center to estimate the
47
magnetization and the BN signal. For this measurement configuration, a
48
49
considerable air induced component ∼ dH/dt was digitally compensated to evaluate the magnetic polarization J. The hardware details and the set-up 3
50
scheme were described in [7]. The magnetization waveform was controlled by
51
a digital feedback with a combined phase-amplitude adjustment, details can
52
be found in [8]. Magnetization conditions, namely the sinusoidal/triangular
53
waveforms of the magnetic polarization J(t) or the triangular waveform of
54
the magnetic field H(t), were controlled in a wide range of the magnetizing
55
frequency fmag = 0.5 − 500 Hz. The measurements without the J(t)/H(t)
56
control, namely at the sinusoidal/triangular waveforms of the magnetizing
57
voltage V (t), were also recorded. Magnetization amplitude was fixed on a
58
near-saturation level of Jmax = 0.9 T or Hmax = 100 A/m.
59
In addition to the measurement with the sample-wrapping coil, BN was
60
alternatively recorded by a small surface-mounted coil also placed in the
61
central part of the solenoid. It was a bobbin coil of 1 cm diameter with
62
800 turns and a pen-type core of ferrite. Its resonance frequency was about
63
60 kHz. The BN signal measured by both coils at different magnetization
64
conditions was filtered within three bandwidths 2–40, 10–40 and 40–80 kHz.
65
MAE was detected by a piezoelectric transducer from Dunegan/Endevco,
66
type S9204, placed again in the solenoid center. The amplified MAE signal
67
was filtered in a 100–300 kHz range; the resonance frequency of the MAE
68
transducer was about 150 kHz [4]. The BN/MAE signals were sampled at a
69
2 MS/s rate.
70
2.2. Electrical steels
71
Industrial electrical steels, two grain-oriented (GO) grades and one non-
72
oriented (NO) steel with distinct magnetic parameters, were chosen for the
73
measurements. Steel strips of the Epstein dimensions 300×30×0.25−0.5 mm
74
were magnetized along the rolling direction by a U-shaped transformer yoke 4
75
of the same length and width through a 3 mm air gap; two magnetizing coils
76
were positioned on the yoke poles. The tangential component of the surface
77
magnetic field was measured directly by a Hall sensor at 1.5 mm above the
78
yoke-free sample side. This method of surface field determination ensured
79
a good measurement accuracy for the magnetically open configuration used.
80
By introducing the air gap, a total inductance of the magnetizing circuit
81
decreased, which stabilized the feedback procedure. For this configuration,
82
the air induced component ∼ dH/dt was negligible, so the magnetic induction
83
B = µ0 H + J was estimated directly by a sample-wrapping coil with 100
84
turns. Waveform of B(t) was adjusted to the sinusoidal/triangular shapes
85
in a fmag = 0.5 − 100 Hz range; additional measurements at the sinusoidal
86
V (t) waveform were conducted. Magnetization amplitudes were Bmax =
87
1.5 and 1.2 T for the GO and the NO steels, respectively. Accuracy of
88
the measurement configuration and efficiency of the digital feedback were
89
comprehensively discussed in [8].
90
BN was detected similarly by the sample-wrapping coil and a bigger
91
surface-mounted coil placed in the central part of the strips. It was a bobbin
92
coil of a 16 mm diameter with 1000 turns of fine copper wire inside a Cu-
93
shielded grounded case. A core with a 4 × 4 mm cross-section was made from
94
a laminated GO steel and gently pressed by a spring to the strip surfaces.
95
A resonance frequency of this coil with the GO core was about 120 kHz [9].
96
The BN signal was filtered within three bandwidths 2–70, 20–100 and 70–
97
170 kHz. The MAE signal was detected by the same Dunegan transducer
98
and filtered in a 100–500 kHz range.
5
(a)
(b) 3
W, J/m 1
tri V(t): 50 34+0.688⋅√f - 0.1% tri H(t): 34+0.737⋅√f-0.14%
J, T
ribbon 0.5
ribbon
45
H, A/m -50
50 -0.5
-1
100
sin J(t):
fmag= 5 Hz
50 Hz tri H(t):
500 Hz fmag=50 Hz
40 sin J(t): 34.8+0.384⋅√f +0.4% tri J(t): 34.6+0.32⋅√f + 0.3% sin V(t): 34.7+0.775⋅√f+0.1%
35 0
100
200
300
400
500
fmag , Hz
Figure 1: (a) Typical hysteresis loops J(H) obtained for the tested Hitperm ribbon at the different magnetizing waveforms and frequencies. (b) Dependence of the hysteresis loss W on the magnetizing frequency fmag for the same ribbon at the different magnetizing waveforms. Relations are fitted by the loss-separation function with the negligible linear coefficients.
99
3. Results
100
3.1. Ribbon
101
Typical hysteresis loops measured under the sinusoidal waveform of the
102
magnetic polarization J(t) at three magnetizing frequencies fmag = 5, 50 and
103
500 Hz are shown in Fig. 1(a) together with the loop measured at the tri-
104
angular field H(t) and fmag = 50 Hz. The loops become slightly wider with
105
increasing fmag ; dc coercive field Hc ≃ 12 A/m. Figure 1(b) presents depen-
106
dence of the hysteresis loss W on the magnetizing frequency for the different
107
magnetizing waveforms. The loss dependence for the triangular voltage V (t)
108
and field H(t) are very close to each other because the field generated inside 6
109
110
111
112
113
the solenoid is nearly proportional to the magnetizing voltage (the circuit resistance prevails over its inductive reactance), i.e. H(t) ∼ I(t) ≈ V (t). Other relations are quite different, but all of them are fitted well by the loss-separation formula W = Wdc + a ·
q
fmag + b · fmag , where Wdc is an ex-
trapolated static loss at zero fmag . The classical linear term Wcl = b · fmag is
114
derived from the Maxwell equations under dubious assumptions that a thin
115
and infinite sheet with constant permeability is magnetized unidirectionally
116
and homogeneously. There is still debate about the origin of the square root
117
term, so-called excess loss Wex = a ·
q
fmag , which was added to fit the ex-
118
perimental loss dependence for the electrical steels [1, 2]. The least-square
119
fittings of the experimental loss dependence are shown by the correspond-
120
ing lines. Graph labels give the fitting formulas with the linear coefficient
121
b presented as a percentage ratio to the square root coefficient b/a; the fol-
122
123
124
125
lowing linear term fmag is omitted for the sake of simplicity (e.g. a formula q √ 2 + 10 · f + 1% in the label means the fitting 2 + 10 · fmag + 0.1 · fmag ). It should be noted that the used coefficient ratio b/a does not agree with a corresponding term ratio Wcl /Wex = (b/a) ·
q
fmag . Two terms of the loss-
126
separation formula become comparable Wcl = Wex at a critical magnetizing
127
frequency fcr = (a/b)2 ; so the linear term contribution is negligible in the
128
considered fmag range for the ratio b/a varying on a common error level of
129
a few percents (for b/a = 1, 2 and 5 %, fcr = 10, 2.5 and 0.4 kHz, respec-
130
tively). For the thin ribbons, the classical linear component Wcl is known to
131
be negligible [1, 5]. This is also proved by our data: the ratio b/a reaches a
132
maximal value 0.4% for the sinusoidal J(t). Pearson correlation coefficients
133
of the fits equal R = 0.992 for the controlled J(t) and R = 0.997 for the
7
(a)
U
rms
(b)
, mV
U
rms
, mV
sin J(t)
2
2
sin J(t), filter
tri J(t) sin V(t)
2 - 40 kHz
tri V(t)
10 - 40 kHz
BN, ribbon
1
sample-wrapping
0.28 + 0.117
0
100
sample-wrapping coil
tri H(t), filter
1
2 - 40 kHz
filter 10 - 40 kHz
10 - 40 kHz
coil -0.05 + 0.22
BN, ribbon
tri H(t)
40 - 80 kHz
40 - 80 kHz
-0.08 + 0.16
f + 1.1%
-0.05 + 0.18
f + 2.2%
f + 7.4% f + 0.1%
200
f
mag
, Hz
f
300
0
50
mag
100
, Hz
150
Figure 2: Dependence of the rms value Urms of BN on the magnetizing frequency fmag : (a) for all filtering bandwidths and two magnetizing waveforms, the sinusoidal polarization J(t) and the triangular field H(t); (b) for the medium filtering bandwidth 10–40 kHz and all magnetizing waveforms. The BN signal from the tested Hitperm ribbon is detected by the sample-wrapping coil. Representative relations are fitted by the same loss-separation function with the linear coefficients showed in the labels as the percentage ratio b/a.
134
other waveforms.
135
Figure 2 presents similar dynamic dependence of the rms intensity Urms of
136
the one-cycle BN signal detected by the sample-wrapping coil. Low-frequency
137
hysteresis component distinctly distorts the BN output, when fmag value
138
reaches ∼ 1% of a low cutoff frequency of the band-pass filter. Therefore, the
139
measurements at the low filtering bandwidth 2–40 kHz are not representative
140
enough. Constant terms of the loss-separation fits Udc are relatively high:
141
0.05–0.08 mV for the two lower filtering bandwidths and 0.28 mV for the
142
40–80 kHz bandwidth. Level of a background noise can be estimated at the
143
saturation regions, where the BN activity is minimal, i.e. as Urms (Hmax ≃ 8
144
145
±100 A/m), or by reading the empty BN response without applying the voltage into the magnetizing coil, i.e. as Urms (H ≡ 0). Thus determined
146
background noise is several times lower than Udc and also dependent on the
147
filtering: for the two lower bandwidths, the background noise level is about
148
0.01 mV; for the 40–80 kHz bandwidth, it is 0.1 mV [6, 10]. Shape of the
149
magnetizing waveform has a qualitatively similar impact on the rms value
150
and the hysteresis loss: the sinusoidal V (t) and the triangular J(t) give the
151
maximal and the minimal values, respectively. However, quantitatively the
152
waveform shape influence is weaker for Urms . For the two lower filtering
153
bandwidths, the Urms relations divide into two groups for the data obtained
154
with and without the J(t) control (see Fig. 2(b)). However, the difference
155
between these two groups vanishes for the higher filtering bandwidth 40–
156
80 kHz (see Fig. 2(a)). The relative linear coefficients of the loss-separation
157
fits are slightly higher than those for the hysteresis loss: b/a ≃ 1 − 2% for
158
the medium filtering bandwidth 10–40 kHz, which is a still negligible level.
159
For the high filtering bandwidth 40–80 kHz, the linear coefficient is even
160
smaller by an order of magnitude b/a ≃ 0.1%. Correlation coefficients of the
161
fits are R = 0.9998 and 0.9989 for the medium and the high bandwidths,
162
respectively.
163
Figure 3 presents similar dependence of the rms value Urms of BN recorded
164
by the surface-mounting coil with the different filtering bandwidths. Interfer-
165
ence of the low-frequency hysteresis contribution is significantly smaller for
166
the detection by the surface coil, so the measurements with the low filtering
167
168
bandwidth 2–40 kHz can be performed up to fmag ≃ 50 Hz (see Fig. 3(a)). The loss-separation fits of these relations with the correlation coefficients
9
(a)
U
rms
(b)
U
, mV
rms
0.2
surface-mounted coil
0.4
surface-mounted coil
, mV
filter 2 - 40 kHz
filter 10 - 40 kHz
sin J(t)
BN, ribbon
BN, ribbon
tri J(t)
sin J(t)
0.3
sin V(t)
tri J(t)
tri V(t)
sin V(t) tri V(t)
0.1
tri H(t)
0.2
tri H(t) -0.006 + 0.025
-0.013 + 0.05 -0.002 + 0.047
0
10
20
0.1
f - 4.1% f - 5.7%
30
40
f
50
mag
f - 0.9%, R=0.998
-0.018 + 0.041 f
0.4
, R = 0.999
, Hz
f
60
0
100
200
300
400
mag
, Hz
500
Figure 3: Dependence of the rms value Urms of BN on the magnetizing frequency fmag for all magnetizing waveforms and two filtering bandwidths: (a) 2–40 kHz; (b) 10–40 kHz. The BN signal from the tested Hitperm ribbon is detected by the surface-mounted coil. Representative relations are fitted by the same loss-separation function with the linear coefficients showed in the labels as the percentage ratio b/a. In (b) the relation is additionally fitted by a power function.
10
169
R = 0.9998 give the negative linear coefficients b/a ∼ −5%. The rms rela-
170
tions divide into two similar groups with different dependence on the mag-
171
netizing waveform shape. However, the group with the sinusoidal/triangular
172
J(t) demonstrates higher rms values at fmag > 10 Hz in contrast to the re-
173
sults obtained with the sample-wrapping coil (compare Figs. 2(b) and 3(a)).
174
This waveform-induced difference between the rms dependence vanishes at
175
the higher cut-off frequency of the filter (see Fig. 3(b)). The loss-separation
176
fitting results in a negative linear coefficient again, but of a smaller negligible
177
178
179
180
181
level b/a ∼ −1%. An alternative power-law fitting gives a similar curve with the similar correlation coefficient R ≃ 0.999, but the resulting power term 0.4 0.5 fmag is rather far from the expected fmag [11, 12]. Constant terms of the fits
Udc can be again higher than the background noise, whose level is ∼ 3 µV for both filtering bandwidths.
182
Figure 4 presents the discrete Fourier spectra of the BN signals de-
183
tected by both coils at different magnetizing conditions [9, 13]. For bet-
184
ter visualization, the spectra obtained at the higher magnetizing frequencies
185
fmag = 5 − 50 Hz in Fig. 4(a) are normalized to a level of the original 2 Hz
186
spectrum on the assumption that the rms magnitude increases according to
187
the square root of the magnetizing frequency, i.e. the spectra are divided by
188
Urms / fmag /2. Such fmag -normalized spectra differ in a low-frequency region
189
q
up to f ≤ 20 Hz. This deviation of the spectra from the Urms ∼
q
fmag behav-
190
ior at low frequencies results in the negative linear term of the loss-separation
191
fitting in Fig. 3(a). Moreover, only this low-frequency spectral region is sen-
192
sitive to variations of the magnetizing waveform (see Fig. 4(b)) [6]. The same
193
fmag -normalization of the spectra recorded by the sample-wrapping coil (not
11
(a)
U
rms
1
(f
mag
/2),
(b)
V
U f
mag
BN, ribbon
2 Hz
surface-mounted coil
5 Hz
sin
J(t),
filter 2-40 kHz
rms
1
=
,
V
f
mag
BN, ribbon surface-mounted coil
10 Hz
tri J(t)
tri V(t)
50 Hz 0.5
tri H(t)
0.5
sample-wrapping coil /10
f, kHz 20
sin J(t)
sin V(t)
20 Hz
0
= 2 Hz
filter 2-40 kHz
40
0
10
f, kHz 20
Figure 4: Fourier power spectra of the BN signals from the Hitperm ribbon recorded by the surface-mounted coil at: (a) the sinusoidal polarization J(t) and different magnetizing frequencies fmag = 2 − 50 Hz; (b) different magnetizing waveforms and fixed fmag = 2 Hz. The filtering bandwidth is 2–40 kHz. In (a) the spectra for fmag = 5−50 Hz are normalized to the 2 Hz spectrum on the assumption of the square root rise with the magnetizing p frequency Urms / fmag /2. In (b) the similar spectra recorded by the sample-wrapping coil are shown by the corresponding dashed lines. They are reduced by an order of magnitude to fit the same scale.
12
194
shown in the graph) gives similar spectra deviation in the low-frequency re-
195
gion, but of the opposite sign. This logically leads to the positive linear
196
term of the loss-separation fitting in Fig. 2(a). This low-frequency region up
197
to f ≤ 20 kHz is also sensitive to variations of the magnetizing waveform,
198
however, the spectra obtained with and without the J(t) control are clearly
199
detached for the sample-wrapping data. Next difference between the spectra
200
for both coils is that the spectral magnitudes for the sinusoidal/triangular
201
J(t) are smaller than those obtained without the J(t) control in accordance
202
with the rms dependence in Fig. 2(b).
203
Figure 5(a) demonstrates a nearly linear correlation between the BN rms
204
values and the hysteresis losses at ac magnetizing frequencies fmag > 10 Hz.
205
Number of the individual BN pulses over a magnetization cycle hyperbolically
206
drops with magnetizing frequency (see Fig. 5(b)) [4, 10]. Qualitatively same
207
results are obtained for other magnetizing-sensing conditions.
208
One-cycle rms values of MAE demonstrate qualitatively similar depen-
209
dence on the magnetizing frequency as compared with the hysteresis loss (see
210
Figs. 1(b) and 6(a)). Therefore, there are similar nearly linear correlations
211
between the MAE rms values and the hysteresis losses at fmag > 10 Hz (see
212
Figs. 5(a) and 6(b)). However, a low signal-to-noise ratio leads to a higher
213
scattering of the MAE data. Correlation coefficients of the loss-separation
214
215
fits are of the same level, R = 0.991 − 0.996; but the linear coefficients of the fits are higher b/a ≃ ±1%. It is difficult to perform a detailed spec-
216
tral analysis of the weak MAE signal; the reasonable signal-to-noise ratio
217
is achieved by amplification within the resonance bandwidth of the MAE
218
transducer. Number of the individual MAE pulses also drops hyperbolically
13
(a) U
rms
(b)
, mV
2
f
1
mag
10
3
sin J(t)
ribbon sin
pulse count,
50
BN
40
J(t)
surface-mounted coil
sin V(t)
filter 2 - 40 kHz
tri V(t)
30
= 10 Hz
tri J(t)
BN, ribbon
tri H(t) sample-wrapping coil
20
surface-mounted coil
-0.19 + 52.2
10
f
3
0
W, J/m
36
39
42
f
45
0
10
20
30
40
mag
50
, Hz
60
Figure 5: (a) Correlations between the BN rms values and the hysteresis losses under the sinusoidal J(t) fitted by the linear curves for fmag > 10 Hz. The BN signal from the Hitperm ribbon is filtered within the 10–40 kHz bandwidth. (b) Number of the BN individual pulses over a magnetization cycle versus fmag fitted by the hyperbolical function with R = 0.9998.
14
(a)
2
(b) 2
Urms , µV
sin V(t):-0.04+0.073⋅√f+0.5% tri V(t):-0.03+0.063⋅√f +0.6% tri H(t):-0.15+0.083⋅√f -0.3%
U
rms
,
V
MAE ribbon
MAE ribbon
1
1
sin J(t) f
mag
= 10 Hz
tri J(t) sin V(t) tri V(t)
sin J(t): -0.09+0.065⋅√f -0.9% tri J(t): -0.04+0.048⋅√f -1.7% 0
100
200
300
400
tri H(t)
0
500
fmag , Hz
36
39
42
3
45
48
51
W, J/m
Figure 6: Dependence of the MAE rms value Urms from the Hitperm ribbon on (a) the magnetizing frequency fmag and (b) the hysteresis losses W for the different magnetizing waveforms. In (a) the relations are fitted by the loss-separation function with the linear coefficients showed in the labels as the percentage ratio b/a. In (b) the relations for the sinusoidal J(t) and the triangular H(t) are fitted by the linear curves for fmag > 10 Hz.
219
with magnetizing frequency [4].
220
3.2. Electrical steels
221
Hysteresis loops for the tested electrical steels measured under the sinu-
222
soidal waveform of the magnetic induction B(t) at the magnetizing frequency
223
fmag = 50 Hz are shown in Fig. 7(a) together with the quasi-static loop for
224
the hardest NO steel. The loops are of typical sizes and shapes for this class
225
of ferromagnetic materials [2]. The first GO steel with the dc coercive field
226
Hc ≃ 8 A/m belongs to the softest transformer steels. Figure 7(b) presents
227
dependence of the hysteresis loss on the magnetizing frequency obtained at
228
the sinusoidal B(t). The dependence are well fitted by the above-discussed 15
(a)
(b) 3
450
B, T
W, J/m
400
1
NO, sin V(t): 138+15⋅√f +7.6%
350
NO, sin B(t): 144+8.43⋅√f +17% NO, tri B(t): 150+3.7⋅√f + 41%
300 250
H, A/m
200
-50
50
100
150
150 100
-1
sin B(t), fmag= 50 Hz GO1 NO
sin B(t)
50
GO2 1 Hz
0
20
40
GO1: 50+3.35⋅√f+21% GO2: 47+11⋅√f + 3.8%
60
80
100
120
fmag , Hz
Figure 7: (a) Hysteresis loops B(H) for the tested electrical steels at the sinusoidal induction waveforms B(t) and the magnetizing frequency fmag = 50 Hz. Nearly quasi-static loop obtained at fmag = 1 Hz for the NO steel is shown for comparison. (b) Dependence of the hysteresis loss W on the magnetizing frequency fmag for the tested steels at the sinusoidal B(t). For the NO steel, similar dependence for the triangular B(t) and the sinusoidal V (t) are additionally shown. Relations are fitted by the loss-separation function. Linear coefficients of the fits are shown in the labels as the percentage ratio to the square root coefficients b/a.
16
(a)
U
rms
,
V
(b) 60
BN, filter 20 - 100 kHz
U
rms
sample-wrapping coil
80
,
V
GO2
sin B(t)
tri B(t)
NO
sin B(t)
tri B(t)
40
60 GO1
40
GO2
sin B(t)
tri B(t)
sin B(t)
tri B(t)
f 2 k
sin B(t)
tri B(t)
20
BN, filter 70 - 170 kHz
20
sample-wrapping coil
f +3.5%
3.3+7.36
f +6.1%
2.6+ 5.01
f +4.2%
1.9 + 8.9
f +1%
1.7 + 4.9
f + 3.2%
4.4 + 19.6
0
sin V(t)
NO
2.6+7.37
20
sin B(t)
40
f
f -2%
60
mag
, Hz
f
80
0
20
mag
40
, Hz
60
Figure 8: Dependence of the rms value Urms of BN on the magnetizing frequency fmag for the tested electrical steels and the different magnetizing waveforms. The BN signal is detected by the sample-wrapping coil and filtered within (a) the medium bandwidth 20– 100 kHz and (b) the high bandwidth 70–170 kHz. In (a) the dependence obtained at the low filtering bandwidth 2–70 kHz is additionally shown for the NO steel (the highest green line). Relations are fitted by the same loss-separation function with the linear coefficients showed in the labels as the percentage ratio b/a; correlation coefficients of the fits are R ≃ 0.9998. 229
230
q
loss-separation formula W = Wdc + a · fmag + b · fmag as shown in the graph labels. Pearson correlation coefficients of the fits are R ≃ 0.998. Ratio be-
231
tween the fitting coefficients b/a is on a level of 20 % for the first GO and the
232
NO steels, but is only 4 % for the second GO steel. Variations of the mag-
233
netizing waveform can significantly influence the slope of the loss-frequency
234
dependence as shown in Fig. 7(b) for the NO steel. However, the slope dif-
235
ferences are smaller for the GO steels. For the softest GO steel, there are the
236
same loss-frequency relations for the triangular and the sinusoidal B(t).
17
237
Figure 8 presents the dynamic rms dependence of BN detected by the
238
sample-wrapping coil under different magnetizing waveforms and filtering
239
bandwidths. The linear coefficients of the loss-separation fits for the two
240
highest filtering bandwidths are on a level of b/a ≃ 4%, which is several
241
times higher than those for the tested ribbon (compare with Fig. 2). There
242
is no evident correlation between magnitudes of the linear coefficient b for
243
the hysteresis loss and the BN rms values. Moreover, the coefficient b is
244
negative for the NO steel and the lowest filtering bandwidth. Influence of
245
the magnetizing waveform shape on the BN rms value is practically negligible.
246
247
248
249
250
251
Figure 9 presents similar dynamic dependence of the BN rms value recorded by the surface-mounting coil. The low filtering bandwidths give small negative values of the linear coefficients of the loss-separation fitting, b/a ≃ −1%, which is several times lower than those for the tested ribbon (compare Figs. 3(a) and 9(a)). However, the fittings for the GO steels and the high filtering bandwidth 70–170 kHz give b/a ≃ +4% (see Fig. 9(b)). There is
252
again no evident correlation between the linear coefficients of the BN rms
253
and the loss dependence as well as there is no noticeable influence of the
254
magnetizing waveform shape on the BN rms values.
255
The Fourier power spectra of the BN signal behave correspondingly to
256
the above-shown dynamic dependence of the rms value. There is a simi-
257
lar suppression of the
258
leading to the negative linear coefficient of the loss-separation fits at the
259
low filtering bandwidths (see Figs. 4(a), 9(a) and 10(a)). However, the last
260
power spectrum for fmag = 50 Hz in Fig. 10(a) does not already demon-
261
strate such a suppression in the low-frequency region, but on the contrary, it
q
fmag -normalized spectra in the low-frequency region
18
(a)
U
rms
,
V
150
(b)
GO1
sin B(t)
tri B(t)
sin V(t)
GO2
sin B(t)
tri B(t)
sin V(t)
NO
sin B(t)
tri B(t)
sin V(t)
f20k
sin B(t)
tri B(t)
sin V(t)
U
rms
250
150
BN, filter
V
GO1
200
100
,
sin B(t)
GO2
sin B(t)
NO
sin B(t)
NO
tri B(t)
NO
sin V(t)
BN, filter
2-70 kHz,
70-170 kHz,
100
surface-
50
2 + 12.2
f - 1.1%
1.1+13.7
f -1.3%
2.2+14.8
f -1.8%
3 + 15.1
0
20
40
60
mounted
50
coil f
f -0.5%
80
surface-
mounted
100
mag
, Hz
120
0
20
20+11.
f + 4.2%
18+15.7
f +4.7%
6.3+23.4
f -0.5%
40
60
coil f
80
mag
, Hz
100
Figure 9: Dependence of the rms value Urms of BN on the magnetizing frequency fmag for the tested electrical steels and the different magnetizing waveforms. The BN signal is detected by the surface-mounted coil and filtered within (a) the low filtering bandwidth 2– 70 kHz and (b) the high filtering bandwidth 70–170 kHz. In (a) the dependence obtained at the medium filtering bandwidth 20–100 kHz is additionally shown for the NO steel (the highest green line). Relations are fitted by the loss-separation function with the linear coefficients showed in the labels as the percentage ratio b/a; correlation coefficients of the fits are R ≃ 0.9996.
19
(a)
U
rms
(f
mag
/2),
(b)
V
f
mag
U
=
rms
(f
mag
/2),
V
f
mag
=
2 Hz 0.2
BN, GO2, sin
surface-mounted coil filter 2 - 70 kHz
2 Hz 0.2
5 Hz
B(t)
5 Hz
10 Hz
10 Hz
20 Hz
20 Hz
50 Hz
50 Hz
0.1
0.1
BN, GO2, sin
B(t)
surface-mounted coil filter 70 - 170 kHz f, kHz
0
20
40
f, kHz 60
60
80
100
120
140
160
Figure 10: Fourier power spectra of the BN signals recorded by the surface-mounted coil at different filtering bandwidths: (a) 2–70 kHz; (b) 70–170 kHz. The measurements are performed for the second GO steel at the sinusoidal B(t) waveform. Similar to Fig. 4(a), p the spectra for fmag = 5 − 50 Hz are normalized to Urms / fmag /2. 262
263
shows a small rise as compared with the 20 Hz spectrum at higher frequencies f ≃ 20 − 60 kHz. This rise becomes apparent at frequencies ∼ 100 kHz lead-
264
ing to the positive coefficient of the loss-separation fits at the high filtering
265
bandwidth (see Figs. 9(b) and 10(b)). Peaks of the spectra near 120 kHz is
266
determined by the resonance of the surface-mounted coil [9]. For such high
267
frequencies, the signal-to-noise ratio is worse; the spectra are noisier with
268
clear spikes of disturbing harmonics [13]. Dynamic dependence of the BN
269
pulse count for the electrical steels are similar to that for the ribbon (see
270
Fig. 5(b)).
271
For the softest GO steel, good linear correlations between the BN rms
272
values and the hysteresis loss are observed for different measurement condi-
273
tions in an ac magnetization range fmag > 5 Hz (see Fig. 11(a)). For the
20
(a) 200
U
rms
,
(b) U
V
rms
250
GO1, sample coil, 20-100 kHz 3
W, J/m
150
GO2, surface coil, 2-70 kHz
100
BN sin
surface coil, 20-100 kHz
200
B(t)
surface coil, 70-170 kHz
150 f
mag
f
= 5 Hz
mag
= 2 Hz
100
50
BN, NO sin
50 -138+22.6
0
V
surface coil, 2-70 kHz
GO1, surface coil, 2-70 kHz GO1, surface coil, 70-170 kHz
,
sample coil, 20-100 kHz
W -1.5%
-31.6 + 0.84 W
60
80
100
120
3
0 150
W, J/m
140
200
-270+28.7
W -1.3%
-581+64.9
W -1.9%
250
300
350
B(t) 3
W, J/m
400
Figure 11: Correlations between the BN rms values and the hysteresis loss for the tested electrical steels. The measurements are made by both coils at the sinusoidal B(t) and different filtering bandwidths. The data for the GO steels are fitted by the linear curves for fmag > 5 Hz. The data for the second GO and the NO steels are fitted by the loss-separation function for fmag > 2 Hz; correlation coefficients of the fits are R ≃ 0.998.
21
(a)
U
rms
15
,
(b)
V
U
rms
15
sin B(t)
sin V(t)
10
10 4.7+0.63 5 + 0.44 f
40
60
MAE GO1 sin B(t) tri B(t)
0.72
sin V(t)
, R = 0.9999
f
20
-0.8 + 0.12 W, R =0.9965
f + 9.4%, R =0.9995
5 0
V
-1.2 + 0.11 W, R =0.9968
MAE GO1
tri B(t)
,
80
mag
5
, Hz
100
3
W, J/m
60
80
100
120
140
Figure 12: (a) Dependence of the rms value Urms of MAE on the magnetizing frequency fmag for the softest GO steel and the different magnetizing waveforms. The dependence is fitted by the loss-separation and the power functions with the comparable correlation coefficients R. (b) Linear correlations between the MAE rms values and the hysteresis loss for the same GO steel.
274
second GO steel, this correlation bends down to the loss scale and is bet-
275
ter fitted by the same loss-separation function with a small linear coefficient
276
277
b/a = −1.5%; the correlation coefficient of this fit is R = 0.9977 versus the linear fit R = 0.993. For the NO steel, the correlations should be also fitted
279
by the loss-separation function with the similar ratio b/a (see Fig. 11(b)). √ The observed W -like relations are consistent with our previous results for
280
other electrical steels with similar magnetic properties [14].
278
281
Figure 12 presents dependence of the MAE rms value on the magnetizing
282
frequency and the hysteresis loss for the softest GO steel. There is again
283
no evident influence of the magnetizing waveform shape on the rms value.
284
The linear coefficient of the loss-separation fit Urms (fmag ) is relatively high,
285
b/a = 9.4%, but it is still twice lower than that for the corresponding depen22
286
287
dence of the hysteresis loss (compare Figs. 7(b) and 12(a)). The constant term Udc ≃ 5 µV is much higher than that for the ribbon measurements
288
because of the wider filtering bandwidth (compare with Fig. 6(a)). The cor-
289
relations between the MAE rms values and the hysteresis loss demonstrate
290
the same linear trend, but in the whole fmag range in contrast to the BN data
291
(compare Figs. 11(a) and 12(b)). For the second GO steel, very similar results
292
293
294
q
are obtained: Urms = 4.5 µV+0.98· fmag +11% and Urms = −1.44+0.121·W for the sinusoidal B(t) (see Fig. 4 in our recent work [4]). First, there are comparable ratios b/a ≃ 10% for the MAE dependence Urms (fmag ) for both
295
GO steels despite of quite different ratios b/a = 21 and 3.8% for the corre-
296
sponding loss data. Second, a good linear correlation of the MAE rms values
297
with the hysteresis loss for the second GO steel contradicts the corresponding
298
BN data (see Fig. 11(a)).
299
4. Discussion
300
Hysteresis losses of magnetic ribbons are known to increase nearly proq
301
portional to
302
it is a consequence of their tiny thickness, high resistivity or specific DW
303
structure [1, 5]. The studied nanocrystalline ribbon follows the same trend
304
and the thickness is expected to be an important factor determining such
305
a loss behavior (see Fig. 1(b)). Anyway, this factor is definitely important
306
for investigation of the BN response: the tiny thickness ensures homogeneous
307
magnetization and detection. But even under these measurement conditions,
308
intensity of the BN signal behaves differently from the hysteresis loss. For the
309
case of the sample-wrapping coil, a considerable positive level of the linear
fmag , although there is still no a clear explanation whether
23
310
coefficient b can be explained by influence of the high-frequency harmonics of
311
the hysteresis induction signal since the high-frequency filtering decreases the
312
linear term of the loss-separation fits to a negligible level (see Fig. 2). How-
313
ever, a negligible negative level of b for the case of the sample-mounted coil
314
is evidently caused by a suppression of large BN pulses in the low-frequency
315
part of the power spectra (see Figs. 3 and 4). These largest pulses are only
316
sensitive to variations of the magnetizing waveform and are logically assigned
317
to the magnetization reversal at the coercive field region, where considerable
318
jumps of the 180◦ DW occur (see Fig. 1(a)). With increasing magnetizing
319
frequency, number of the BN pulses is significantly reduced due to a pulse
320
overlapping (see Fig. 5(b)). Such an overlapping is assumed to occur with a
321
small loss in the total BN intensity, just as a peak of the differential magnetic
322
permeability loses in its height with fmag increase [6, 15].
323
For the electrical steels, the BN dynamic behavior is qualitatively similar
324
to the above-discussed ribbon case despite the quite different dependence of
325
the hysteresis loss [10]. There is no any correlation between the parameters
326
of the loss-separation fits for the hysteresis losses and the BN rms values.
327
There is much weaker influence of the magnetizing waveform shape on the
328
BN rms value as compared with the hysteresis loss. Moreover, the dynamic
329
rms dependence for three tested steels are very close to each other, which
330
indicates a comparable level of the BN activity. For the low filtering band-
331
width, the BN spectra demonstrate similar suppression of the low-frequency
332
333
334
BN signal at f ≤ 20 kHz giving the negative linear term of the loss-separation fits (see Figs. 8(a), 9(a) and 10(a)). Qualitatively similar results with higher b/a ≃ −7% are obtained in our previous work [6] for a harder microalloyed 24
335
336
steel with dc Hc = 210 A/m. There is only one significant distinction from the ribbon data. This is the high-frequency BN activity at f ∼ 100 kHz lead-
337
ing to the positive b coefficient at the high filtering bandwidth, which can not
338
be already explained by the high-frequency harmonics of the hysteresis signal
339
(see Figs. 8(b) and 9(b)). This high-f BN activity is determined by short BN
340
pulses and can be logically assigned to the hysteresis loop knees, where the
341
90◦ DW reorganization mostly occurs. These are prior and completion phases
342
of the magnetization reversal, where nucleation, growth and subsequent an-
343
nihilation of the 90◦ domains on the grain boundaries and the sheet surface
344
take place. These domains are needed to close the internal magnetic flux
345
of the rapidly moving 180◦ domains, thereby minimizing the magneto-static
346
energy [16]. With increase of the magnetizing frequency, these knee-regions
347
of the hysteresis loops do not significantly change, only the magnetization
348
reversal occurs at higher magnetic fields producing wider B(H) loops (see
349
Figs. 1(a) and 7(a)). However, a number of the magnetic domains is known
350
351
352
353
to rise at high fmag ≥ 40 Hz for this class of materials [17]. Increasing number of the 90◦ DWs can cause this additional BN activity at f ∼ 100 kHz giving the positive linear coefficient b for the high filtering bandwidth. The principal issues under discussion are validity and physical grounds q
354
of the observed dynamic dependence with the
355
use the loss-separation formula to fit the micro-magnetic signals simply by
356
analogy with the hysteresis data. There is still no suitable theory for de-
357
scribing the obtained dynamical properties of BN/MAE, which we can rely
358
on [18, 19, 20]. We also try to use the power function proposed in [11, 12] as
359
a fitting alternative. It provides a similar accurate fitting of the experimental
25
fmag dominant term. We
360
data, but the power coefficient can significantly deviate from the expected
361
value 0.5, even if the corresponding loss-separation fitting gives a small ra-
362
tio b/a (see Fig. 3(b) and 12(a)). Analysing the BN spectra in Figs. 4 and
363
10, we are inclined to stick with the opinion about the dominating role of
364
365
the a ·
q
fmag component with the above-discussed deviations, which can be
introduced by the linear term ±b · fmag . Physical background should be of
366
similar origin as proposed to explain the excess loss Wex component. Rapid
367
irreversible changes of local magnet moments caused by the DW motion are
368
detected by the induction coils with an unknown transfer coefficient [19]. Af-
369
ter the filtering (it should be mentioned that a coil with many turns of wind-
370
ing has a self-capacitance and is a LC filtering circuit in fact), the detected
371
packet of the electrical impulses is symmetrical in polarity, so evaluation of
372
the rms value is a routine method to estimate the intensity of the micro-
373
magnetic signals [9]. These sensing-evaluation procedures could also have
374
an influence on the resulting dynamic dependence, but we again stick with
375
the opinion about the micro-magnetic origin of the observed Urms ∼
q
fmag
376
behavior. The local DW motion does not only give rise to the BN activity,
377
but also to micro eddy-currents, which are considered to define the excess
378
379
loss Wex ∼
q
fmag term [1, 2].
Small negative ratios b/a ≃ −1% for the MAE J(t)-controlled dependence
380
of the ribbon in Fig. 6(a) can be similarly explained by the overlapping of
381
the largest MAE pulses because the magnetization rates near Hc are min-
382
imal under the J(t) adjusted waveforms [6]. Much higher positive ratios
383
384
b/a ≃ 10% for the MAE dependence of the GO steels as compared with the corresponding BN relations (see Figs. 8, 9(b) and 12(a)) can be explained
26
385
by a more intensive MAE response to the 90◦ DW activity. As mentioned in
386
Introduction, theoretically MAE should not be sensitive to the motion of the
387
180◦ DWs at all [3, 4]. The next factor, which can be responsible for higher
388
MAE ratios b/a, is the fact that the MAE waves freely propagate through
389
the whole material, whereas the surface-mounted coil picks up the BN signal
390
from the steel surface only [4, 9]. However, the thickness of the GO steel
391
sheets is still small enough to ensure relatively homogeneous magnetization
392
and BN detection.
393
Finally, let us discuss the observed correlations between the micro-magnetic
394
rms values and the hysteresis losses. A main difference between these pa-
395
rameters is caused by the reversible component of the magnetization reversal
396
describing by the loss-separation terms Wdc and Wcl ∼ fmag . The constant
397
terms Wdc /Udc and different near-dc magnetization dynamics on the macro-
398
and the micro-scales are probably responsible for a lack of the correlation at
399
400
401
low fmag ≤ 2 − 10 Hz. At higher dynamic range, the correlations actually proves the physical coupling of the micro-magnetic signals (local DW motions causing the detected magnetic pulses) with the exchange losses Wex ∼
q
fmag
402
assigned to the micro eddy currents [1]. This assumption is experimentally
403
confirmed by the linear correlations in case of all MAE data and the BN
404
data for the two softest and thinnest materials, the ribbon and the first GO
405
steel (see Figs. 5(a), 6(b), 11(a) and 12(b)). The square-root correlations for
406
the two harder and thicker materials, the second GO and the NO steels, are
407
408
defined by a near-linear dependence W ∼ fmag at high fmag > 20 Hz (see Figs. 7(b) and 11).
27
409
410
5. Conclusion The dynamic behavior of magnetic Barkhausen noise and magneto-acoustic
411
emission for the typical soft ferromagnetic materials is primarily determined
412
by a square root of the magnetizing frequency. However, a supplementary
413
linear term could be added to fit the experimental dependence of the rms
414
intensities of these micro-magnetic signals (by analogy with the hysteresis
415
loss separation). For the Barkhausen noise data, this linear term is mostly
416
negligible. Its sign, however, is opposite for different regions of the Fourier
417
spectrum. It is negative for the largest impulses at the frequencies up to
418
f ≤ 20 kHz, but seems to be positive for the short impulses at f ∼ 100 kHz.
419
For the magneto-acoustic emission, the linear terms of the fits become con-
420
siderable and comparable with the classical hysteresis loss components. This
421
gives a good linear correlation between the hysteresis loss and the rms inten-
422
sity of the magneto-acoustic emission. No direct correlation is found between
423
the fitting parameters for the micro-magnetic and the macro-hysteresis re-
424
sponses, however, related physical factors (local domain wall motion and
425
attendant micro eddy currents) are assumed to be responsible for the square
426
root rise of the dynamic dependence. Influence of the magnetizing waveform
427
shape on the micro-magnetic rms intensities is nearly negligible as compared
428
with that on the hysteresis loss.
429
Acknowledgment
430
The authors appreciate the financial support of the Czech Science Founda-
431
ˇ tion (GA CR) under projects 13-18993S and 14-36566G. The authors thank
28
432
ˇ Dr. P. Svec from Institute of Physics SAS in Bratislava and Dr. P. Anderson
433
from Cardiff University for sample provision.
434
435
[1] A.J. Moses, Energy efficient electrical steels: Magnetic performance prediction and optimization, Scripta Mater. 67 (2012) 560–565.
436
[2] S.E. Zirka, Y.I. Moroz, R.G. Harrison, K. Chwastek, On physical as-
437
pects of the Jiles-Atherton hysteresis models, J. Appl. Phys. 112 (2012)
438
043916.
439
440
[3] M. Guyot, V. Cagan, The magneto-acoustic emission (invited), J. Appl. Phys. 73 (1993) 5348–5353.
441
[4] A. Stupakov, O. Perevertov, M. Landa, Dynamic behaviour of magneto-
442
acoustic emission in a grain-oriented steel, J. Magn. Magn. Mater. 426
443
(2017) 685-690.
444
445
[5] C.D. Graham Jr, Physical origin of losses in conducting ferromagnetic materials (invited), J. Appl. Phys. 53 (1982) 8276–8280.
446
[6] A. Stupakov, O. Perevertov, V. Zablotskii, Dynamical properties of mag-
447
netic Barkhausen noise in a soft microalloyed steel, IEEE Trans. Magn.
448
51 (2015) 6100204.
449
450
ˇ [7] O. Stupakov, P. Svec, Three-parameter feedback control of amorphous ribbon magnetization, J. Electr. Eng. 64 (2013) 166–172.
451
[8] A. Stupakov, O. Perevertov, V. Zablotskii, A system for controllable
452
magnetic measurements of hysteresis and Barkhausen noise, IEEE
453
Trans. Instrum. Measur. 65 (2016) 1087–1097. 29
454
[9] O. Stupakov, J. Pal’a, T. Takagi, T. Uchimoto, Governing conditions
455
of repeatable Barkhausen noise response, J. Magn. Magn. Mater. 321
456
(2009) 2956-2962.
457
[10] O. Stupakov, Y. Melikhov, Influence of magnetizing and filtering fre-
458
quencies on Barkhausen noise response, IEEE Trans. Magn. 50 (2014)
459
6100104.
460
[11] A. Zhukov, M. V´azquez, J. Vel´azquez, C. Garc´ıa, R. Valenzuela,
461
B. Ponomarev, Frequency dependence of coercivity in rapidly quenched
462
amorphous materials, Mater. Sci. Eng. A A226–228 (1997) 753–756.
463
[12] R. Gr¨ossinger, N. Mehboob, D. Suess, R. Sato Turtelli, M. Kriegisch, An
464
eddy-current model describing the frequency dependence of the coerciv-
465
ity of polycrystalline galfenol, IEEE Trans. Magn. 48 (2012) 3076–3079.
466
[13] M. Vashista, V. Moorthy, Influence of applied magnetic field strength
467
and frequency response of pick-up coil on the magnetic Barkhausen noise
468
profile, J. Magn. Magn. Mater. 345 (2013) 208-214.
469
[14] O. Stupakov, Local non-contact evaluation of the ac magnetic hysteresis
470
parameters of electrical steels by the Barkhausen noise technique, J.
471
Nondestruct. Eval. 32 (2013) 405–412.
472
473
[15] O.V. Perevertov, Application of the Preisach model to the magnetization process in steels, J. Phys. D: Appl. Phys. 35 (2002) 2467–2471.
474
[16] O. Perevertov, J. Thielsch, R. Sch¨afer, Effect of applied tensile stress
475
on the hysteresis curve and magnetic domain structure of grain-oriented
476
transverse Fe-3%Si steel, J. Magn. Magn. Mater. 385 (2015) 358-367. 30
477
478
479
480
[17] T.R. Haller, J.J. Kramer, Observation of dynamic domain size variation in a silicon-iron alloy, J. Appl. Phys. 41 (1970) 1034–1035. [18] G. Biorci, D. Pescetti, Frequency spectrum of the Barkhausen noise, J. Appl. Phys. 28 (1957) 777–780.
481
[19] G. Bertotti, F. Fiorillo, M.P. Sassi, Barkhausen noise and domain struc-
482
ture dynamics in Si-Fe at different points of the magnetization curve, J.
483
Magn. Magn. Mater. 23 (1981) 136-148.
484
[20] R.G. Harrison, Accurate mean-field modeling of the Barkhausen noise
485
power in ferromagnetic materials, using a positive-feedback theory of
486
ferromagnetism, J. Appl. Phys. 118 (2015) 023904.
31
Highlights Intensity of Barkhausen noise rises as a square root function of the magnetizing frequency Level of magneto-acoustic emission is proportional to the hysteresis loss Magnetizing waveform has small influence on intensities of these micro-magnetic signals