HAL Id: hal-00532181
https://hal.archives-ouvertes.fr/hal-00532181
Submitted on 4 Nov 2010
HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.
L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.
Reply to Comments on “ Separation of Qi, Qs from 1 passive data at Mt. Vesuvius: A reappraisal of the
seismic attenuation estimates” by Ugalde, A. and Carcole, E
Edoardo del Pezzo, Francesca Bianco, Lucia Zaccarelli
To cite this version:
Edoardo del Pezzo, Francesca Bianco, Lucia Zaccarelli. Reply to Comments on “ Separation of Qi, Qs from 1 passive data at Mt. Vesuvius: A reappraisal of the seismic attenuation estimates” by Ugalde, A. and Carcole, E. Physics of the Earth and Planetary Interiors, Elsevier, 2009, 173 (1-2), pp.195.
�10.1016/j.pepi.2008.10.002�. �hal-00532181�
Accepted Manuscript
Title: Reply to Comments on “ Separation of Qi, Qs from 1 passive data at Mt. Vesuvius: A reappraisal of the seismic attenuation estimates” by Ugalde, A. and Carcole, E Authors: Edoardo Del Pezzo, Francesca Bianco, Lucia Zaccarelli
PII: S0031-9201(08)00295-1
DOI: doi:10.1016/j.pepi.2008.10.002 Reference: PEPI 5079
To appear in: Physics of the Earth and Planetary Interiors Received date: 10-9-2008
Accepted date: 1-10-2008
Please cite this article as: Del Pezzo, E., Bianco, F., Zaccarelli, L., Reply to Comments on “ Separation of Qi, Qs from 1 passive data at Mt. Vesuvius: A reappraisal of the seismic attenuation estimates” by Ugalde, A. and Carcole, E, Physics of the Earth and Planetary Interiors (2008), doi:10.1016/j.pepi.2008.10.002
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.
Page 1 of 5
Accepted Manuscript
Reply to Comments on " Separation of Qi and
1
Qs from 1 passive data at Mt. Vesuvius: A
2
reappraisal of the seismic attenuation
3
estimates" by Ugalde, A. and Carcolé , E.
4
Edoardo Del Pezzo, Francesca Bianco and Lucia Zaccarelli
5
INGV sezione di Napoli Osservatorio Vesuviano
6 7
Key words: seismic scattering, elastic attenuation
8
1 Introduction
9
The paper by Del Pezzo et al. (2006) , hereafter named DPBZ, deals with the
10
estimate of the seismic attenuation in the high frequency range for the volcanic
11
area of Mt. Vesuvius. In particular DPBZ use a method based on the …t of the
12
observed local earthquake coda envelopes to the radiative transfer classical
13
equation (see Sato and Fehler, 1998 for a wide and exhaustive review on this
14
argument) in terms of the intrinsic attenuation and the scattering attenuation
15
coe¢ cients.
16
Ugalde and Carcolé in their comment (hereafter named UC) discuss two points
17
of DPBZ that we summarize here in their essence:
18
a) Two approximations of the exact solution of the 3-D radiative transfer
19
model have been calculated, that discussed by Zeng (1991) - hereafter Z91 -
20
expressed by Formula (5) of UC, and that by Paaschens (1997) - hereafter P97
21
- expressed by Formula (6) of UC. UC show that P97 is more accurate than
22
Z91, which is instead used in DPBZ.
23
b) DPBZ obtain the separated estimates of intrinsic- and scattering-attenuation
24
coe¢ cients, respectively i and s, …rst stacking the normalized energy en-
25
velopes (starting at 2T s lapse time) and then …tting the experimental data
26
with the normalized (in the same way) theoretical curve. UC disagree with
27
this procedure. Their opinion is that DPBZ should have inverted the single
28
energy envelopes and then have averaged the results obtained.
29
Preprint submitted to Elsevier 10 September 2008
Testo
Page 2 of 5
Accepted Manuscript
In the following we reply to points a) and b) in two separate sections.
30
2 Reply to point a)
31
UC show that P97 is more accurate than Z91. This is true, with no doubts at
32
all. At the time DPBZ was written (2005) the authors were not informed of
33
P97, being P97 published on a General Physics Journal in a sector di¤erent
34
from that of Seismology. The authors of DPBZ are grateful to A. Ugalde and
35
E. Carcolè for having informed that the approximation described in P97 is
36
better than that in Z91; accordingly they already changed the formula in Z91
37
with that in P97 in their Matlab …les for a possible use in their future works.
38
However, due to the assumptions that are at the base of DPBZ as well as
39
to the data scatter produced by the high level of background seismic noise
40
in their study, the separated estimates of intrinsic- and scattering-attenuation
41
coe¢ cients, respectively i and s, are a¤ected by an uncertainty (see Figure 7
42
of DPBZ) that results so high that the use of P97 instead of Z91 is practically
43
ine¤ective. In addition, but only for the sake of precision (or in other words
44
to be scholastic), in DPBZ the authors use theoretical curves normalized at
45
12 seconds lapse time to …t their data. In the plot of Figures 1 and 2 of UC
46
the percent ratio between the absolute P97 and Z91 instead of the normalized
47
values used in DPBZ is reported. In the present reply we plot in Fig. 1 the
48
percent ratio between the normalized P97 and Z91, estimated for the values
49
of i and s estimated by DPBZ for Mt. Vesuvius. Due to the normalization,
50
the bias is much lower than that calculated by UC.
51
3 Reply to point b)
52
We generate two vectors of normally distributed values ik and sk in the
53
error range determined in DPBZ for the estimate of i and s (at 3 Hz, see
54
Fig. 7 of DPBZ) and a vector of uniformly distributed (between 0.5 and 5
55
km) synthetic values of source station distances, rk, k 2 [0; 1000] ; roughly
56
corresponding to the real distribution of measured source-BKE distances for
57
the seismicity at Mt. Vesuvius. Then, for each value of k we calculated the
58
theoretical energy envelopes using Formula (6) of UC for ik , sk and rk. For
59
these synthetical envelopes we eventually calculate the stack in the same way
60
as described in DPBZ. Indicating the average of ik , sk and rk respectively
61
with i , s and r we plot in Fig. 2 the energy envelope calculated using
62
Formula (7) of UC for i , s and r and the stacked envelope of the synthetic
63
traces. The two quantity are practically coincident in the range of lapse time
64
used for the analysis done at Mt. Vesuvius by DPBZ.
65
2
Page 3 of 5
Accepted Manuscript
4 Figure Captions
66
Figure 1 - Percent ratio between Z91 and P97 ( 100 (1 (EZeng/ EP aasschens);
67
continuous line) and between Z91-normalized and P91-normalized (100 (1
68
(EZengN/ EP aasschensN), dashed line) as a function of lapse time, in the lapse
69
time interval between 3.6 and 12 s, used by DPBZ.
70
Figure 2 - Normalized energy envelope calculated for the average (dashed) and
71
stack of the energy envelopes (continuous). The vertical bar mark the lapse
72
time at which DPBZ start their analysis.
73
5 References
74
References
75
Del Pezzo, E., Bianco, F., Zaccarelli, L. (2006) Separation of Qi and Qs
76
from passive data at Mt. Vesuvius: a reappraisal of the sismic attenuation
77
estimates, Physics of the Earth and Pl. Int., 159, 202-212
78
Paasschens, J.C.J. (1997) Solution of the time dependent Boltzmann equation,
79
Phys. Rev. E. 56, 1135-1141
80
Sato, H. and Fehler, M. (1998) Seismic wave propagation and scattering in
81
the heterogeneous earth. Springer and Verlag, New York.
82
Zeng, Y. (1991) Compact solutions for multiple scattered wave energy in time
83
domain, Bull. Seism. Soc. Am 81, 1022-1029
84
3
Page 4 of 5
Accepted Manuscript
2 4 6 8 10 12
Lapse time (s)
0 1 2 3 4 5
Percen t ratio
100*[1-(EZeng / EPaasschens)]
100*[1-(EZengN / EPaasschensN)]
Figure 1
Figure 1
Page 5 of 5
Accepted Manuscript
4 6 8 10 12 14
Lapse time (s) 1
10 100
Normalized energy envelope
Energy Envelope for the average parameters Average (Stack) of the energy envelopes
Figure 2
Figure 2