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6b8aaa3a16daf1881ecfc19fc8c7d5b8ac4bdd8c
subsection
15
21
Non-isoplanatism and large field imaging
The image is clipped so that only the central disk of radius Ma remains (see Fig. REF ). The simulations of Fig. REF show that, for rapidely varying object fields, light is observed outside the central disk of radius Ma. More complex effects are exhibited, but clipping do not occur anymore. In many applications of cohe...
{ "cite_spans": [] }
10.1016/j.optcom.2008.10.058
0807.1718
Coherent imaging of extended objects
[ "E. Brainis", "C. Muldoon", "L. Brandt", "A. Kuhn" ]
[ "physics.optics" ]
2,008
en
Physics
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23f182b5ef24fbc3ee85c5cbd34cd68b5bd14ddb
subsection
16
21
Isoplanatic imaging through a thin lens
In Sec. , we claimed that isoplanatic imaging is possible with a thin lens when the object lies on the spherical surface \mathcal {S}_o and the image is observed on the spherical surface \mathcal {S}_i. Let's examine this statement more closely.Referring to Fig. REF , simple Gaussian Optics arguments suggest that if th...
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10.1016/j.optcom.2008.10.058
0807.1718
Coherent imaging of extended objects
[ "E. Brainis", "C. Muldoon", "L. Brandt", "A. Kuhn" ]
[ "physics.optics" ]
2,008
en
Physics
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87a52fb5b38759038e6f672be6091a29e4110b24
subsection
17
21
Isoplanatic imaging through a thin lens
This lens must act as a pure phase-correction transparency. Similarly, on the image side, a thin lens of focal length z_i placed just after (or before) the image plane can be used to project the image from S_i onto \mathcal {I}. From a broader point of view, any spherical field distribution in the object space of a cen...
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10.1016/j.optcom.2008.10.058
0807.1718
Coherent imaging of extended objects
[ "E. Brainis", "C. Muldoon", "L. Brandt", "A. Kuhn" ]
[ "physics.optics" ]
2,008
en
Physics
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3c30158098059df151118e7a48ce448457f85b64
subsection
18
21
Experimental investigation
The theoretical discussion of Secs.  and relies on two strong approximations: the paraxial approximation and the thin lens approximation. One may wonder whether our analysis is robust enough to be applied to systems containing powerful lenses, which are usually thick and have a high numerical aperture. The following e...
{ "cite_spans": [] }
10.1016/j.optcom.2008.10.058
0807.1718
Coherent imaging of extended objects
[ "E. Brainis", "C. Muldoon", "L. Brandt", "A. Kuhn" ]
[ "physics.optics" ]
2,008
en
Physics
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22a486ac73235c70087c1221acda7fff5d29de54
subsection
19
21
Experimental investigation
REF , the lens size was varied while the object size was kept constant. Here, the lens is always the same, but the square size is varied instead. For this reason, the ring pattern is the same for every picture in the left column of Fig. REF . When the SLM is illuminated with a spherical wave converging on L_{1} (isopla...
{ "cite_spans": [] }
10.1016/j.optcom.2008.10.058
0807.1718
Coherent imaging of extended objects
[ "E. Brainis", "C. Muldoon", "L. Brandt", "A. Kuhn" ]
[ "physics.optics" ]
2,008
en
Physics
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1b89100cc67efafacd776e4057df36daa57a072f
subsection
20
21
Conclusion
In general, even diffraction-limited imaging systems distort the phase of the processed fields. This is of no relevence when used with incoherent light, but has a tremendous effect on coherent imaging. In combination with Fraunhofer diffraction from the finite instrumental aperture, the phase distortion leads to a seve...
{ "cite_spans": [] }
10.1016/j.optcom.2008.10.058
0807.1718
Coherent imaging of extended objects
[ "E. Brainis", "C. Muldoon", "L. Brandt", "A. Kuhn" ]
[ "physics.optics" ]
2,008
en
Physics
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ea1611bd18f99a82da5233fb27938a8d390b906c
abstract
0
10
Abstract
This note is an appendix to a preprint by E. Hellmann. We give a complete classification of simple objects of the category of vector spaces D over K = Fpbar((u)) equipped with an endomorphism phi whose image generates D and that are semi-linear with respect to the ring morphism sending u to u^b (b > 1 is an integer) an...
{ "cite_spans": [] }
0807.1719
Sur la classification de quelques phi-modules simples
[ "Xavier Caruso" ]
[ "math.NT" ]
2,008
en
Mathematics
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278db8d4a7a081747061dc785219c81a7a316aea
subsection
1
10
Body
Sur la classification de quelques \phi -modules simples Xavier CarusoDans cet appendice, on détermine les \phi -modules étales simples sur \bar{F}_p((u)) dans une situation légèrement plus générale que celle étudiée dans l'article (). On fixe p un nombre premier et on pose k = \bar{\mathbb {F}}_p et pour tout q, puissa...
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0807.1719
Sur la classification de quelques phi-modules simples
[ "Xavier Caruso" ]
[ "math.NT" ]
2,008
en
Mathematics
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71c17f5d2f80a22449fc1cc90a311e3781a15b15
subsection
2
10
Body
\bullet \phi (e_{d-1}) = a u^n e_0.D(d,n) = K e_0 \oplus K e_1 \oplus \cdots \oplus K e_{d-1} ;\phi (e_i) = e_{i+1} pour i \in \lbrace 0, \ldots , d-2\rbrace .\phi (e_{d-1}) = a u^n e_0.On définit également D(d,n) = D(d,n,1).On commence par déterminer des familles d'isomorphismes entre les différents D(d,n,a).Lemme 1 ...
{ "cite_spans": [] }
0807.1719
Sur la classification de quelques phi-modules simples
[ "Xavier Caruso" ]
[ "math.NT" ]
2,008
en
Mathematics
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b32646a24dc7f21a930ea00a1cb5867f56e698e1
subsection
3
10
Body
(ii) Si \sigma est l'identité et si t est premier avec p, on a : D(d,n,a) \simeq D(d^{\prime },n^{\prime },a^{\prime }_1) \oplus D(d^{\prime },n^{\prime },a^{\prime }_2) \oplus \cdots \oplus \simeq D(d^{\prime },n^{\prime },a^{\prime }_t) où les a^{\prime }_i sont les racines t-ièmes de a. (iii) Si \sigma est l'identit...
{ "cite_spans": [] }
0807.1719
Sur la classification de quelques phi-modules simples
[ "Xavier Caruso" ]
[ "math.NT" ]
2,008
en
Mathematics
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adfcfb51ee2338a1024791bec67611d941f8e958
subsection
4
10
Body
Comme par ailleurs, il est clair que à \alpha fixé, la famille des f_i(\alpha ) est libre, on en déduit que les sous-objets F(\alpha ) = K f_0(\alpha ) \oplus \cdots \oplus K f_{d-1}(\alpha ) sont tous isomorphes à D(d^{\prime },n^{\prime }). Il suffit donc pour conclure de montrer que t d'entre eux sont en somme direc...
{ "cite_spans": [] }
0807.1719
Sur la classification de quelques phi-modules simples
[ "Xavier Caruso" ]
[ "math.NT" ]
2,008
en
Mathematics
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7e48e6a1be0de53787517cfd7c01fe625ccedc25
subsection
5
10
Body
Pour tous entiers i \in \lbrace 0, \ldots , d^{\prime }-1\rbrace et j \in \lbrace 0, \ldots , p-1\rbrace , on pose :et on définit D_m comme le sous-K-espace vectoriel de D(d,n) engendré par les f_{i,j} avec 0 \leqslant i < d^{\prime } et 0 \leqslant j < m. À nouveau l'utilisation des déterminants de Vandermonde assure ...
{ "cite_spans": [] }
0807.1719
Sur la classification de quelques phi-modules simples
[ "Xavier Caruso" ]
[ "math.NT" ]
2,008
en
Mathematics
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32b699b7eebe1dc868b013df37670d79dd53018d
subsection
6
10
Body
De plus, ils sont deux à deux non isomorphes.Pour simplifier la preuve, on suppose dans la suite a=1, laissant au lecteur l'exercice (facile) d'adapter les arguments au cas général.Notons \ell = \ell (r) et considérons n tel que \frac{n}{p^\ell -1} représente r. Soit D un sous-objet non nul de D(r), et soit x = \lambda...
{ "cite_spans": [] }
0807.1719
Sur la classification de quelques phi-modules simples
[ "Xavier Caruso" ]
[ "math.NT" ]
2,008
en
Mathematics
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2b56c13754d9f8164db0c4a09e4c801427c6ecd3
subsection
7
10
Body
Pour cela, nous considérons D un objet simple de \text{\rm Mod}^\phi _{/K}, (e_1, \ldots , e_d) une base de D et G la matrice de \phi dans cette base, i.e. l'unique matrice vérifiant l'égalité :On rappelle, à ce propos, la formule de changement de base qui interviendra plusieurs fois dans la suite : si \mathcal {B}^{\p...
{ "cite_spans": [] }
0807.1719
Sur la classification de quelques phi-modules simples
[ "Xavier Caruso" ]
[ "math.NT" ]
2,008
en
Mathematics
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87cbbae453989b97f7e02e6fd7cb53a74351f2e7
subsection
8
10
Body
En particulier, on peut supposer que G a tous ses coefficients dans \mathbb {F}_q[[u]] pour un certain q. C'est ce que nous ferons par la suite.Soit M le sous-\mathbb {F}_q[[u]]-module de D engendré par les e_i ; il est libre de rang d. On définit deux suites récurrentes (x_i) et (n_i) comme suit. On pose en premier li...
{ "cite_spans": [] }
0807.1719
Sur la classification de quelques phi-modules simples
[ "Xavier Caruso" ]
[ "math.NT" ]
2,008
en
Mathematics
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f2e62c72e35b96e95b2e0cef3acf142536ec8be2
subsection
9
10
Body
Ainsi la suite (z_i) converge vers un élément z \in M (car tous les v_i sont positifs) vérifiant \phi ^\delta (z) = z. Par ailleurs, on a z \equiv x \pmod {u}, ce qui assure qu'il est non nul. On a donc montré le résultat intermédiaire important suivant :Théorème 7 Soit D un objet simple de \text{\rm Mod}^\phi _{/K}. ...
{ "cite_spans": [] }
0807.1719
Sur la classification de quelques phi-modules simples
[ "Xavier Caruso" ]
[ "math.NT" ]
2,008
en
Mathematics
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de299db6b0647bdbbe4807feca6c6f7a47eb17f0
abstract
0
51
Abstract
In this paper we consider the operator mapping problem for in-network stream processing applications. In-network stream processing consists in applying a tree of operators in steady-state to multiple data objects that are continually updated at various locations on a network. Examples of in-network stream processing in...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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f137db2fe838b4b9d3720e51cc0088c05e226674
subsection
1
51
Introduction
In this paper we consider the execution of applications structured as trees of operators. The leaves of the tree correspond to basic data objects that are spread over different servers in a distributed network. Each internal node in the tree denotes the aggregation and combination of the data from its children, which i...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 791, "openalex_id": "", "raw": "B. Badcock, S. Babu, M. Datar, R. Motwani, and J. Widom, “Models and issues in data stream systems,” in Proceedings of the Intl. Conf. on Very Large Data Bases, 2004, pp. 456–467.", "source_re...
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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6010c5fa27069727e2148587b17e0a526ccebcc3
subsection
2
51
Introduction
Our objective is to meet this constraint while minimizing the “overall cost”, that is the amount of resources used to achieve the throughput. For instance, the cost could be simply the total number of compute servers, in the case when all servers are identical and network bandwidth is assumed to be free.We study severa...
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0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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0e8eb705e800a8ee4e02f2c31a6ade583143a665
subsection
3
51
Application model
We consider an application that can be represented as a set of operators, \mathcal {N}. These operators are organized as a binary tree, as shown in Figure REF . Operations are initially performed on basic objects, which are made available and continuously updated at given locations in a distributed network. We denote t...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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c2ac95eeddb4751c526a58eb8534fff6a4d2476e
subsection
4
51
Application model
In this paper we sometimes consider left-deep trees, i.e., binary trees in which the right child of an operator is always a leaf. These trees arise in practical settings , , and we show an example of left-deep tree in Figure REF . Here \mathit {Child}(i) and \mathit {Leaf}(i) have cardinal 1 for every operator n_i but ...
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0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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c5c94d6ec2f314b0ef9981c921be3a4b2243db69
subsection
5
51
Application model
The time required by each activity must be summed for all operators to determine the processor's computation time. We assume that a basic object can be duplicated, and thus be available and updated at multiple servers. We assume that duplication of basic objects is achieved in some out-of-band manner specific to the ta...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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7c11cdf1b04fbd0b853c810df7148b65d1bd3a13
subsection
6
51
Application model
This is expressed by the following constraint, in which the first term corresponds to basic object downloads, the second term corresponds to inter-node communications when a tree node is assigned to P_u and its parent node is assigned to another processor, and the third term corresponds to inter-node communications whe...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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471cf135b2bbe3676be3ce7353f7495b047a5c39
subsection
7
51
Application model
The goal is then to use a subset of this platform so that the prescribed throughput is achieved while minimizing a cost function. Several cost functions can be envisioned, including the compute capacity or the bandwidth capacity used by the application in steady state, or a combination of the two. In the following, we ...
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0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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79ed4059a84442a46cd157c5c545b27230081895
subsection
8
51
Application model
Definition 1 The problem C-LDT-Hom (Constr-Hom-HomS-LDTree-HomA-NoComA) consists in minimizing the number of processors used in the application execution. K is the prescribed throughput that should not be violated. C-LDT-Hom-Dec is the associated decision problem: given a number of processors N, is there a mapping that...
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0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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62a2e9a4ce8118ce4af5c0b904d5396c410cdf5b
subsection
9
51
Application model
The size of \mathfrak {I}_2 is clearly polynomial in the size of \mathfrak {I}_1, since the size of the tree is bounded by 3nM. We now show that instance \mathfrak {I}_1 has a solution if and only if instance \mathfrak {I}_2 does. Suppose first that \mathfrak {I}_1 has a solution. We map all operators corresponding to ...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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9ca29cf1663fa5d982417277221f84f617aa7891
subsection
10
51
Application model
We denote the cost of a processor in class c by cost_c. Each processor of class c has computing speed s_c and network card bandwidth Bp_c. The link bandwidth between processors is a constant bp, while the link between a server S_l and a processor is bs_{l}. For each class, processors are numbered from 1 to |\mathcal {N...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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8f293f103ae11baf85c0285d8ddcd5b7a0759458
subsection
11
51
Application model
\forall i~~ \sum _{c,u} x_{i,c,u}=1: each operator is placed on exactly one processor; \forall c,u,k,l~~ d_{c,u,k,l} \le obj(k,l): object o_k can be downloaded from S_l only if S_l holds o_k; \forall c,u,k,l~~ d_{c,u,k,l} \le \sum _i x_{i,c,u}.leaf(i,k): if there is no operaotr assigned to P_{c,u} that requires objec...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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672b8f10b61cc5c447abb3d786c54379ea77bbf7
subsection
12
51
Application model
Finally, we have to ensure that the required throughput is achieved and that the various bandwidth capacities are not exceeded, following equations (REF )-(REF ). \forall c,u~~ \sum _{i} x_{i,c,u}.\rho \frac{w_i}{s_c} \le 1: the computation of each processor must be fast enough so that the throughput is at least equal...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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5f53993a67b48d054e304544e4275b9475874b41
subsection
13
51
Application model
We can further generalize the linear program to Non-Constr-Het, by adding links of different bandwidths between processors. We just need to replace bp by bp_{c,c^{\prime }} and bs_l by bs_{l,c} every time they appear in the linear program in the previous section. Altogether, we have provided integer linear program form...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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fcd6e78ba62e5cd0b4c922f1ecc7c6beb4374bf2
subsection
14
51
Application model
It picks the two operators that have the largest communication requirements. These two operators are grouped and assigned to the same processor, thus saving the costly communication between both processors. There are three cases to consider for this assignment: (i) both operators were unassigned, in which case the heur...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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fe7f99297e94e7e47b2715bddbbe4e168b53880e
subsection
15
51
Application model
The remaining internal operators are assigned in the same mechanism as Comp-Greedy proceeds, i.e., in decreasing order of w_i of the operators. Object Download Heuristics Once an operator placement heuristic has been executed, each al-operator is mapped on a processor, which needs to download basic objects required by...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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29feee103432daf5a06b207389eba633db8aa677
subsection
16
51
Application model
Note that we do not consider configurations designed for low power consumption, which achieve possibly lower performance at higher costs. [Table: Incremental costs for increases in processor performance ornetwork card bandwidth relative to a $7,548 base configuration (based on datafrom the Dell Inc. web site, as of ear...
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0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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db6678e9a17a3b7db81e51d63c2f2feb84ef9f68
subsection
17
51
Application model
This experiment uses the same parameters as the previous one. Up to a threshold the \alpha parameter has no influence on the heuristics' performance and the solution cost is linear. When \alpha reaches the threshold, the solution cost of each heuristic increases until \alpha exceeds a second threshold and no solution c...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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80839ba39664d2e3221b77432bf104256df42d46
subsection
18
51
Application model
Here once again, the solution found by the heuristic for the operator mapping leads to the failure in the server association process. [Figure: Simulation with big basic objects and high downloadrates, increasing \alpha .] Low download rates - small object sizes The behavior of the heuristics when download rates are low...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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20e4bfce635f262317077b3a9a6cde5f328d8482
subsection
19
51
Application model
We use Cplex 11 to solve our linear program. Unfortunately, the LP is so enormous that, even when using only 5 possible groups of processors and using tress with 30 operators, the LP file could not be opened in Cplex. For trees with 20 operators, Cplex produces the optimal solution, which consists in all cases in buyin...
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0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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72ee7a686e70050b64b3256f8414b2977e5d52da
subsection
20
51
Application model
Such situations arise for instance in relational database applications .
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0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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0bcaafe1b9dcad63131fe49691275a75dab14284
subsection
21
51
Problem Definitions
The overall objective of the operator-mapping problem is to ensure that a prescribed throughput is achieved while minimizing a cost function. We consider two broad cases. In the first case, the user must buy processors (with various computing speed and network card bandwidth specifications) and build the distributed ne...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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0387f721d6a51d91ec40efa0aadd581d02416d2c
subsection
22
51
Complexity
Without surprise, most problem instances are NP-hard, because downloading objects with different rates on two identical servers is the same problem as 2-Partition . But from a theoretical point of view, it is important to assess the complexity of the simplest instance of the problem, i.e., mapping a fully homogeneous l...
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0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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57070c178a5f6f54a7b6b34e6bdd0ff7f5536d25
subsection
23
51
Complexity
Because 3-Partition is NP-complete in the strong sense, we can encode the 3n numbers in unary and assume that the size of \mathfrak {I}_1 is O(n + M), where M = \max _i \lbrace a_i\rbrace .We build the following instance \mathfrak {I}_2 of C-LDT-Hom-Dec:The object set is \mathcal {O}= \lbrace o_1,...,o_{3n}\rbrace , an...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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6fda158e3ec8f8e4f3d34a51dc85eac4ca68f61b
subsection
24
51
Linear Programming Formulations
In this section, we formulate the Constr optimization problem as an integer linear program (ILP). We deal with the most general instance of the problem Constr-LAN. Then we explain how to transform this integer linear program to formulate the Non-Constr-Het problem.
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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09bcb2af7183b258e200593fbcb9c16e8a4ff9e4
subsection
25
51
ILP for
Constants – We first define the set of constant values that define our problem. The application tree is defined via parameters par and leaf, and the location of objects on servers is defined via parameter obj. Other parameters are defined with the same notations as previously introduced: \mathsf {\delta }_i, w_i for op...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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95f58997ef03c26308d50c280d2ad78dc3b5a59a
subsection
26
51
ILP for
There are |\mathcal {N}|^4.|\mathcal {C}|^2 such variables. used_{c,u} is a boolean variable equal to 1 if processor P_{c,u} is used in the final mapping, i.e., there is at least one operator mapped on this processor, and 0 otherwise. There are |\mathcal {C}|.|\mathcal {N}| such variables.Constraints – Finally, we mus...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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4731360f0cd2738f62276fd1128fdf9d4a0f5d5c
subsection
27
51
ILP for
Instead, for all i,c,u,i^{\prime },c^{\prime },u^{\prime }, we write:y_{i,c,u,i^{\prime },c^{\prime },u^{\prime }} \le par(i,j); ~y_{i,c,u,i^{\prime },c^{\prime },u^{\prime }} \le x_{i,c,u}; ~y_{i,c,u,i^{\prime },c^{\prime },u^{\prime }} \le x_{i^{\prime },c^{\prime },u^{\prime }}: y is forced to 0 if one of the condit...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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f5cc8ac26c784c1265d49d9d936c01fd28719245
subsection
28
51
ILP for
Furthermore, we no longer consider processor classes. However, we can simply assume that there is only one processor of each class, and define |\mathcal {C}|=|\mathcal {P}|, the set of processors of the platform. The number of processors of class c is then limited to 1. As a result, all indices u in the previous linear...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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ab339d7ee54e9c6acb65b3773a37cea254d17768
subsection
29
51
Heuristics
In this section we propose several heuristics to solve the Constr operator-placement problem. Due to lack of space, we leave the development of heuristics for the Non-Constr problem outside the scope of this paper. We choose to focus on constructive scenarios because such scenarios are relevant to practice and, to the ...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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78dc8b2b251cb7083af24a486ba83539f40f6521
subsection
30
51
Random
While there are some unassigned operators, the Random heuristic picks one of these unassigned operators randomly, called op. It then purchases the cheapest possible processor that is able to handle op while achieving the required application throughput. If there is no such processor, then the heuristic considers op alo...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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77d0714ee97715286ebf498162e1e489172875af
subsection
31
51
Comp-Greedy
The Comp-Greedy heuristic first sorts operators in non-increasing order of w_i, i.e., most computationally demanding operators first. While there are unassigned operators, the heuristic purchases the most expensive processor available and assigns the most computationally demanding unassigned operator to it. If this ope...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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84eeb2ebc7181a908c1dbe56df854d711351adba
subsection
32
51
Comm-Greedy
The Comm-Greedy heuristic attempts to group operators to reduce communication costs. It picks the two operators that have the largest communication requirements. These two operators are grouped and assigned to the same processor, thus saving the costly communication between both processors. There are three cases to con...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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89d70d79a7ab8e0b73145b0a0cefc0c61a5d8ab0
subsection
33
51
Object-Greedy
The Object-Greedy heuristic attempts to group operators that need the same basic objects. Recall that an al-operator is an operator that requires at least one basic object. The heuristic sorts all al-operators by the maximum required download frequency of the basic objects they require, i.e., in non-increasing order of...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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7bcdeb9e94d30d341faab2ea934974cc92fadab9
subsection
34
51
Subtree-Bottom-Up
The Subtree-Bottom-Up heuristic first purchases as many most expensive processors as there are al-operators and assigns each al-operator to a distinct processor. The heuristic then tries to merge the operators with their father on a single machine, in a bottom-up fashion (possibly leading to the selling back of some pr...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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0a82bf03830fc82947fa286af0c211af7b0616ad
subsection
35
51
Object-Grouping
For each basic object, this heuristic counts how many operators need this basic object. This count is called the “popularity” of the basic object. The al-operators are then sorted by non-increasing sum of the popularities of the basic object they need. The heuristic starts by purchasing the most expensive processor and...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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897bd68015dfcb52851bc657597abc6c1b1da678
subsection
36
51
Object-Availability
This heuristic takes into account the distribution of basic objects on the servers. For each object k the number av_k of servers handling object o_k is calculated. Al-operators in turn are treated in increasing order of av_k of the basic objects they need to download. The heuristic tries to assign as many al-operators ...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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30991dd0aeae37aa766c2693c016214ed7b9cdb6
subsection
37
51
Object Download Heuristics
Once an operator placement heuristic has been executed, each al-operator is mapped on a processor, which needs to download basic objects required by the operator. Thus, we need to specify from which server this download should occur. Two server selection heuristics are proposed in order to define, for each processor, t...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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94cdfc5241f915c526203ff74d682b2be0f2adff
subsection
38
51
Server-Selection-Random
This heuristic is only used in combination with Random. Once Random has decided about the mapping of operators onto processors, Server-Selection-Random associates randomly a server to each basic object a processor has to download.
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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ea723aaf93b87f51848f81e2eff81bb3f9baa3c7
subsection
39
51
Server-Selection-Intelligent
This server selection heuristic is more sophisticated and is used in combination with all operator placement heuristics except Random. Server-Selection-Intelligent uses three loops: the first loop assigns objects that are held in exclusivity, i.e., objects that have to be downloaded from a specific server. If not all d...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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a56bbd37599ea0b8678f11df4c134999f133a680
subsection
40
51
Resource Cost Model
In order to instantiate our simulations with realistic models for resource costs, we use information available from the Dell Inc. Web site. More specifically, we use the prices for configurations of Intel's latest, high-end, rack-mountable server (PowerEdge R900), as advertised on the Web site as of early March 2008. D...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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5a333b56298bb422550adc3db3fd22b1e1089d2e
subsection
41
51
Simulation Methodology
All our simulations use randomly generated binary operator trees with at most N operators, which can be specified. All leaves correspond to basic objects, and each basic object is chosen randomly among 15 different types. For each of these 15 basic object types, we randomly choose a fixed size. In simulations with smal...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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fcbdeb86c9c4767de3384d96fb46bc449ac04e59
subsection
42
51
Results
We present hereafter results for several sets of experiments. Due to lack of space we will only present the most significant figures, but the entire set of figures can be found on the web .
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0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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8d3df7effbb45b9fd25f5555c9b35502348c0602
subsection
43
51
High download rates - small object sizes
In a first set of simulations, we study the behavior of the heuristics when download rates are high and object sizes small (5-30MB). Figure REF shows the results, when the number of nodes N in the tree varies, but the computation factor \alpha is fixed. As expected, Random performs poorly and the platform chosen for an...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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80f4ee84b1034c8bca8aecf337da46f6082bee03
subsection
44
51
High download rates - big object sizes
The second set of experiments analyzes the heuristics' performance under high download rates and big object sizes (450-530MB). As for small object sizes, we plot two types of figures. Figure REF shows results for a fixed \alpha and increasing number of operators. We see that for trees bigger than 45 nodes, almost no fe...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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4b2cbf9887d6bc1ad2a6b9c22dd9d9469db61b03
subsection
45
51
Low download rates - small object sizes
The behavior of the heuristics when download rates are low, i.e., frequency = 1/50s, is almost the same as for high download rates. In general the heuristics lead to the same operator mapping, but in some cases the purchased processors have less powerful network cards (Cf. Table REF ). [Table: Influence of the download...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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subsection
46
51
Low download rates - big object sizes
In this case, low download rates slightly improve the success rate of the heuristics (see Figure REF ). Indeed, because of the lower download rates the links between servers and processors are less congested, and hence the server association is feasible in more scenarios. [Figure: Comparison between the simulations wit...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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subsection
47
51
Influence of download rates (frequency) on the solution
The third set of experiments studies the influence of download rates on the solution. Remember the download rate of a basic object k is computed by rate_k = frequency \times \delta _k. A first results is that frequencies smaller than 1/10s has no further influence on the solution. All heuristics will find the same solu...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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2a2257ca54c0ec804e3044d775036d8ad8750967
subsection
48
51
Comparison of the heuristics to a LP solution on a homogeneous platform
This last set of experiments is dedicated to the evaluation of our heuristics via a lower bound given by the solution of our integer linear program. We use Cplex 11 to solve our linear program. Unfortunately, the LP is so enormous that, even when using only 5 possible groups of processors and using tress with 30 operat...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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84aada2b6b845e05e902dc626d96a1a6638a8467
subsection
49
51
Summary
Our results show that all our more sophisticated heuristics perform better than the simple random approach. Unfortunately, the object sensitive heuristics, Object-Grouping and Object-Availability, do not show the desired performance. We think that in some situations these heuristics could lead to good performance, but ...
{ "cite_spans": [] }
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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5fb8b0a6ac0851620b7d6bad95046080fb6fe183
subsection
50
51
Conclusion
In this paper we have studied the problem of resource allocation for in-network stream processing. We formalized several operator-placement problems. We have focused more particularly on a “constructive” scenario in which one aims at minimizing the cost of a platform that satisfies an application throughput requirement...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1327, "openalex_id": "", "raw": "V. Pandit and H. Ji, “Efficient in-network evaluation of multiple queries,” in HiPC, 2006, pp. 205–216.", "source_ref_id": "bf483f445199aaa17a360fa4f7f7dfea6a401662", "start": 1196 ...
0807.1720
Resource Allocation Strategies for In-Network Stream Processing
[ "Anne Benoit", "Henri Casanova", "Veronika Rehn-Sonigo", "Yves Robert" ]
[ "cs.DC" ]
2,008
en
Computer Science
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83e6878a4ed0a4d58aaea20b09c06d7f0f19642e
abstract
0
12
Abstract
After launch, the Advanced CCD Imaging Spectrometer (ACIS), a focal plane instrument on the Chandra X-ray Observatory, suffered radiation damage from exposure to soft protons during passages through the Earth's radiation belts. An effect of the damage was to increase the charge transfer inefficiency (CTI) of the front ...
{ "cite_spans": [] }
10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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593561b44b1a72ef446cceae58d52c244ba6d317
subsection
1
12
INTRODUCTION
The Advanced CCD Imaging Spectrometer (ACIS), one of two focal plane science instruments on the Chandra X-ray Observatory, utilizes frame-transfer charge-coupled devices (CCDs) of two types, front- and back-illuminated (FI and BI). Soon after launch it was discovered that the FI CCDs had suffered radiation damage from ...
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10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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1b2ee559da091de5a718b2f917c9e551e9f7247a
subsection
2
12
EXPERIMENTAL DETAILS
The ACIS CCDs are buried channel devices made of high-resistivity float zone silicon with a depletion depth of 50–75 \mu m. Each CCD is a framestore-transfer device with 1024 by 1026 pixels in the imaging and framestore arrays. The pixels in the imaging array are 24 \mu m square. The image-to-framestore transfer rate i...
{ "cite_spans": [] }
10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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2be9d56307de1657be0228aeb358924d6e9752c2
subsection
3
12
EXPERIMENTAL DETAILS
Parallel CTI was measured by fitting a linear function to the center pixel pulseheight as a function of row. Serial CTI is unaffected by the low-energy protons used here and was not measured.Three different irradiation/annealing profiles were used. In all cases, the CCDs were powered off during both irradiation and ann...
{ "cite_spans": [] }
10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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2265881f93436a3945c374bab6ade4a09f53fdcc
subsection
4
12
RESULTS
We then use our measured CTI to examine the properties of the reverse annealing. Before we can understand our results, however, we need to confront two sources of systematic error and either correct the CTI data or increase the error associated with each measurement to compensate. These error sources are due to variabl...
{ "cite_spans": [] }
10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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a4a10a251fbf74fdf49466997f944b5f3c0809d4
subsection
5
12
Temperature Variation Corrections
Measured CTI is a function of temperature. Detrapping time constants decrease as the temperature increases so that different populations of traps can become more or less important. If the detrapping time constant drops below the pixel-to-pixel transfer time (40 \mu s for the ACIS imaging array) or becomes much longer t...
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10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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83d95820604f558a435fc33cb304676caef9e879
subsection
6
12
Post-Irradiation CTI Relaxation
An additional unexpected source of systematic error is that repeated CTI measurements immediately after irradiation, but before annealing, show clear “relaxation” or reduction of CTI during the first hour after irradiation. For most CCD quadrants, annealing took place many hours after irradiation, and multiple pre-anne...
{ "cite_spans": [] }
10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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f457bf061780456fd9a610001cb3207f2362172b
subsection
7
12
Anomalous Annealing Results
In this experiment, as in our previous experiment and the flight experience, room-temperature annealing increases the CTI of the CCDs. If we assume that the CTI increase due to annealing should be proportional to the CTI increase from the pre-anneal irradiation independent of dose, then we can define the ratio, R, such...
{ "cite_spans": [] }
10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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354f3354af93d3242813e5e3a361d1d8da26b2ef
subsection
8
12
Long Duration Annealing
A long duration anneal was done at the conclusion of the isochronal annealing (which will be discussed in Section REF ). The CCDs were annealed at a temperature of +30^\circ  C for intervals of one hour, one hour again, six hours and finally over a hundred hours. Between each annealing interval, the temperature was low...
{ "cite_spans": [] }
10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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a2b5eb148f2aaf1762b8c242bac5f4daff67a029
subsection
9
12
Multi-Temperature Isochronal Annealing
A multi-temperature isochronal annealing cycle was done to test the sensitivity of the annealing rate to temperature. After irradiation, the CCD was annealed for one hour intervals each at 0^\circ  C, +10^\circ  C, +20^\circ  C, and +30^\circ  C. The temperature was returned to –100^\circ  C between each annealing inte...
{ "cite_spans": [] }
10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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01c1589933584977c307533511e57092ec038fc3
subsection
10
12
DISCUSSION
In our initial experiment reported in Paper I, we found a substantial difference in the magnitude of the annealing-induced CTI between the ground and flight devices. Several explanations were proposed, such as differences in impurity concentrations between CCDs and in the energy spectrum of the irradiating particles. T...
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10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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4b3f7aba77fe9c5d5777915109a0767bbfdb3af7
subsection
11
12
CONCLUSION
We report the results of laboratory experiments of cold irradiation and room-temperature annealing on ACIS CCDs. Six CCDs were irradiated cold, at –100^\circ  C, by low-energy protons with energies from 100 to 400 keV. The CCDs were then annealed at +30^\circ  C in one of three annealing cycles. We used the fractional ...
{ "cite_spans": [] }
10.1117/12.789750
0807.1721
Physics of reverse annealing in high-resistivity Chandra ACIS CCDs
[ "C. E. Grant", "B. LaMarr", "G. Y. Prigozhin", "S. E. Kissel", "S. K. Brown", "M. W. Bautz" ]
[ "astro-ph", "physics.ins-det" ]
2,008
en
Physics
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c3ace64ba6b703af279d7343ce4fffd605386cf9
abstract
0
19
Abstract
We study the stability and the modes of non -- isothermal coronal loop models with different intensity values of the equilibrium twisted magnetic field.We use an energy principle obtained via non -- equilibrium thermodynamic arguments. The principle is expressed in terms of Hermitian operators and allows to consider to...
{ "cite_spans": [] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
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414cfc6d92e893046b12dc5a19910967a0fbe46f
subsection
1
19
Variational principle
A crucial requirement for any theoretical model of coronal structures is to give account of the stability and evolution of far–from–equilibrium states which are responsible of the characteristic rich topology and dynamics of the solar corona. This implies to consider the coupling of thermal and mechanical equations. Di...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 680, "openalex_id": "", "raw": "Bernstein I. B., 1958, PhRv, 109, 10", "source_ref_id": "0a8bead6c4fb6cd508f87a94bb8347ba054521e9", "start": 487 }, { "arxiv_id": "", "doi": "", "end": 1363, ...
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
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99164f6864e2c2db106b93fc5f9c1dbb6426ba6a
subsection
2
19
Solar coronal loops
MHD loop oscillations in the corona are known to be strongly damped, mostly having decaying times of few periods N_{p}\approx 2 - 7 \ periods. While thermal conduction, with the contribution of radiative cooling mechanisms, could be the main cause of the damping of pure MHD slow magnetoacoustic mode oscillations they a...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 565, "openalex_id": "", "raw": "Halberstadt G., Goedbloed J. P., 1994, A&A, 286, 275", "source_ref_id": "287cb96458620aa75810584342f24aaf85713e85", "start": 359 }, { "arxiv_id": "", "doi": "", ...
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
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555874b6a8291c1466fe259e98590484e3f1c52d
subsection
3
19
Solar coronal loops
They found that pure Alfvén and pure slow modes are obtained as singular limiting cases of cluster spectra of Alfvén–fast or slow–fast modes, where the fast components are localized in a photospheric boundary associated to the line–tied condition: the coronal part of the loop acting as a resonant cavity of large Alfvén...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 931, "openalex_id": "", "raw": "Goedbloed J. P., Halberstadt G., 1993, A&A, 280, 647", "source_ref_id": "c86caa7121588da28b07ad17a02de073647a5ff2", "start": 751 } ] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
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e560a0448f05659dfdd94d99499b058e8b02e4d7
subsection
4
19
The MHD stability criterion for coronal structures
Solar coronal conditions with large Reynolds numbers are well fitted by ideal MHD plasma models (i.e. infinite electrical conductivity \sigma \gg 1 leading to vanishing viscosity and ohmic dissipation). Thus, the fundamental equations considered are the mass conservation equation, the perfect gas law or state equation ...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 2327, "openalex_id": "", "raw": "Costa A., González R., Sicardi Schifino A. C., 2004, A&A, 427, 353", "source_ref_id": "22285ed112a822a561880f14b3b1613a2d7ce7af", "start": 1209 } ] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.016068022698163986, 0.06176957115530968, -0.035706717520952225, -0.009460754692554474, -0.015594985336065292, -0.0678732842206955, 0.010795941576361656, 0.0373242013156414, 0.012955130077898502, 0.016754690557718277, -0.03077797032892704, -0.015236392617225647, -0.00857571605592966, 0.0...
63228d3a588e01bd8013a0598a4afb7c2354bec4
subsection
5
19
Application to an inhomogeneous loop model with non–vanishing helicity
On one hand, the azimuthal component of the loop perturbation is believed to be one of the principle responsible of resonant absorption and damping of ideal oscillations; on the other, this component is associated to the storage of magnetic energy in systems with non–vanishing helicity which eventually is released by i...
{ "cite_spans": [] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.011464671231806278, 0.012250341475009918, -0.012235085479915142, 0.017116915434598923, -0.027490802109241486, -0.05077102780342102, 0.007105350494384766, -0.024226078763604164, 0.016552453860640526, 0.025538070127367973, -0.03328797593712807, -0.016033759340643883, -0.000451473897555843, ...
a1f443603a3bb642caa2baf26c40ecc4a29ba0f9
subsection
6
19
Mechanical equilibrium
To determine an equilibrium configuration we assume force–free equations. This assumption is justified for coronal conditions due to the fact that in plasmas with low \mathcal {\beta } (gas pressure over the magnetic pressure) the pressure gradient can be neglected in comparison to the Lorentz force. For the chromosphe...
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10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.03469327837228775, 0.028117727488279343, -0.03853791579604149, -0.016568558290600777, 0.009016591124236584, -0.0177738219499588, 0.03936176747083664, 0.0354866161942482, -0.010748203843832016, 0.0185824166983366, 0.005355031229555607, 0.010465958155691624, -0.0031542812939733267, 0.0071...
18ff6ed502e9e9b647bd5a0ede5c3c0027dab5b7
subsection
7
19
Thermal equilibrium
The thermal equilibrium is obtained, as in Paper I, assuming L=0 in the balance energy equation (eq. REF ) . The procedure developed consists in obtaining the function of the temperature along the arc element s by integrating eq. REF with the constraint L=0 and replacing border conditions: the temperature at the bottom...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1041, "openalex_id": "", "raw": "Priest E. R., 1982, ”Solar Magneto-hydrodynamics” (Boston:Publishing Company)", "source_ref_id": "2a806f170c2470c287008ed3d8a4f938aa74c100", "start": 382 }, { "arxiv_id": ...
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ 0.0482279509305954, 0.009332719258964062, -0.06843485683202744, 0.03589624911546707, -0.0038841816131025553, -0.03385113924741745, 0.03916231915354729, -0.01032475009560585, 0.01629982702434063, 0.014353920705616474, -0.0030276014003902674, -0.002651774324476719, -0.022053604945540428, 0.0...
970bdc69d332536c077b2e29a0227b453d864c15
subsection
8
19
The perturbation
To calculate the stability and the structure of the modes the general perturbation along the equilibrium magnetic field is written\vec{\xi }=[\zeta _{r}(r,z) \mathbf {e}_{t}+i \zeta _{\phi }(r,z) \mathbf {e}_{\phi }+\zeta _{z}(r,z) \mathbf {e}_{z}]e^{im\phi } \ \ T_{1}=T_{1}(r,z)e^{im\phi }with r=R. The \phi dependence...
{ "cite_spans": [] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ 0.002174515277147293, 0.014107645489275455, -0.015099529176950455, -0.020799048244953156, 0.00020707966177724302, -0.04117082431912422, 0.04455849155783653, -0.014145794324576855, 0.02704028971493244, 0.01294790394604206, -0.010361375287175179, -0.030870487913489342, -0.000649016525130719, ...
39eab1cef2907870cb5d8b94255d3fc94e6aa766
subsection
9
19
Results and discussion
Convective motion of the photosphere is believed to provide the energy that is storage in twisted magnetic coronal fields allowing the presence of long–lived coronal structures until it is released by instabilities (; ). On the other hand, continuous spectra are generally associated to stability. An accepted conjecture...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 220, "openalex_id": "", "raw": "Raadu M.A., Schmieder B., Mein N., Geesztelyi L., 1988, A&A, 197, 289", "source_ref_id": "aeba585fb1a40c22966f909f7ad1f5914705738b", "start": 0 }, { "arxiv_id": "", "...
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.04587950184941292, -0.012774830684065819, -0.017811503261327744, -0.009020221419632435, 0.009684146381914616, -0.03656928986310959, 0.007192519959062338, -0.011729340068995953, 0.027671169489622116, 0.00906600896269083, -0.00810446310788393, -0.003764149034395814, -0.02982320263981819, ...
83c3f399bd987683500eaef436ccd038f47f28ea
subsection
10
19
Results and discussion
A matrix discrete eigenvalue problem subject to a normalization constraint was obtained. From the resulting modes and the generalized potential energy (eq. REF ): \delta ^{2}W_{p}\ge 0 the stability of each mode was determined.The coronal loop parameters used were: L=10^{10}cm (or L=100Mm), T_{b}=10^{4}K T_{t}=10^{6}K ...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 926, "openalex_id": "", "raw": "Aschwanden, M. J. 2004, \"Physics of the Solar Corona\", (New York:Springer-Verlag).", "source_ref_id": "b37502a7eb7bcec88345c1701ef697937c69a500", "start": 789 }, { "arxiv...
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.0023491918109357357, 0.010769671760499477, -0.03810572251677513, -0.03102763742208481, -0.004179731011390686, -0.021691886708140373, 0.04033287614583969, 0.000019783168681897223, 0.011936640366911888, 0.0197698213160038, -0.023064792156219482, -0.007017066236585379, -0.004633551929146051,...
eb3286d1d5da35011df445ca5ca222f66b8b67bb
subsection
11
19
Results and discussion
For B_{0}=10G and weak and moderate helicity cases there are five different groups of periods (P_{1}-P_{6};P_{7}-P_{10};P_{11}-P_{12};P_{13}-P_{14};P_{15}- P_{18}) (see also Table 2). The clustering is more difficult to establish i.e., the differences are less pronounced, with increasing magnetic field intensity and la...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1348, "openalex_id": "", "raw": "Freidberg, J.P, 1982, Reviews of Modern Physics, 54, 3", "source_ref_id": "8c00192a504a96bd54c8e254a9bd5563c2fba31f", "start": 1113 }, { "arxiv_id": "", "doi": "", ...
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.0132380286231637, -0.0071340384893119335, -0.025713058188557625, -0.019776927307248116, 0.0218065045773983, -0.02182176522910595, 0.04016425460577011, 0.025102658197283745, 0.035952500998973846, 0.02026524767279625, -0.025713058188557625, -0.021638644859194756, -0.013077798299491405, -0...
b593464058e2a4eb64179b51234c6c6969b51b67
subsection
12
19
Results and discussion
Table 2 (Second Panel) also shows the intensity relationship between the cylindrical components. In order to classify the modes and to compare with the slow and fast magnetoacoustic modes obtained in Paper I, we calculated the cylindrical mode components and also the tangential and normal to the field components (\xi _...
{ "cite_spans": [] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.01861167512834072, 0.033470503985881805, -0.018764231353998184, -0.0178183913230896, -0.007765035144984722, -0.017803136259317398, 0.03807765617966652, 0.017070872709155083, 0.04399678111076355, 0.01624707691371441, -0.028039557859301567, -0.057085976004600525, -0.00813116692006588, -0....
83fb5866310c9d4c06a2ca0d49b39870e7b4c308
subsection
13
19
Results and discussion
The \xi _{\parallel } and \xi _{\perp } components are in an inverted phase for real eigenvector modes and in phase for imaginary eigenvector modes.For moderate helicity the overall description is similar but all the cases having non vanishing \xi _{\phi } component and all the periods in the resonant line-tied continu...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 2703, "openalex_id": "", "raw": "Ruderman M.S., 2007, SoPh, 246, 119", "source_ref_id": "c23414b1b67a967995f634e19b35fbe71da8bcac", "start": 2354 }, { "arxiv_id": "", "doi": "", "end": 2855, ...
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.029367493465542793, -0.0006669663125649095, -0.013646350242197514, -0.012441138736903667, -0.011136763729155064, 0.0012481184676289558, 0.03283056989312172, 0.040550027042627335, 0.0021625154186040163, 0.01166309043765068, -0.030496425926685333, -0.04396733269095421, 0.0011203507892787457...
c6968508594c6d72f9f92eacf453721d8e747373
subsection
14
19
Results and discussion
However, when the helicity is incremented to b=0.5 even for the radius of R=0.01 the loop structure is unstable, thus, instability can be associated with the presence of helicity values larger than a critical one.Figure REF shows the general potential energy for P_{6} and P_{7} in the weak and moderate cases. Note the ...
{ "cite_spans": [] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.009706689044833183, 0.010866607539355755, -0.024251459166407585, -0.017215637490153313, -0.006318504922091961, -0.034095507115125656, 0.02249632030725479, 0.042153891175985336, 0.007734064012765884, 0.004326802212744951, -0.011957847513258457, -0.023045755922794342, -0.0009844048181548715...
e0990dbad8aa09182c424aa483428c054c17fc69
subsection
15
19
Results and discussion
Meanwhile all the "zoo" of the coronal seismology can be active and accessible to observations. [Figure: Energy content of the sixth and seventh mode for B_{0}=10G. a) Total potential energy and b) magnetic potential energy respectively for the sixth mode P_{6}=1.23 \ min and for weak helicity. c) Total potential energ...
{ "cite_spans": [] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ 0.00947654340416193, 0.019365111365914345, -0.02553020417690277, -0.03464050590991974, -0.008431224152445793, -0.06015545129776001, 0.0356781929731369, 0.0521286204457283, -0.004192722029983997, 0.014481867663562298, -0.0010796545539051294, -0.003925669472664595, 0.02774292416870594, -0.01...
7741ea3141331e60aff0c22cd7210f0bb6622a28
subsection
16
19
Appendix: Generalized potential energy terms
From the procedure described above and extensively exemplified in Paper I we can obtain -laboriously but in a straightforward way- the explicit terms for the energy principle given in eq. REF :\delta ^{2} W_{p}= \delta ^{2} W_{c}+\delta ^{2} W_{m}+\delta ^{2} W_{hc}+\delta ^{2} W_{r}where the right side of the equation...
{ "cite_spans": [] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.0023218169808387756, 0.03183769807219505, -0.01775035634636879, -0.030860895290970802, -0.033760782331228256, -0.07735065370798111, 0.044841401278972626, 0.024145370349287987, 0.03550071269273758, 0.010950886644423008, -0.004647449590265751, -0.023580655455589294, -0.023412765935063362, ...
69a834a27c85686d8a459a97c0667721b597ba75
subsection
17
19
Appendix: Generalized potential energy terms
\Delta \frac{d\rho _{0}}{ds}(\frac{\xi _{r}\xi _{\phi }}{R} -\frac{m}{R} \xi _{\phi }\xi _{z}+\xi _{z}\frac{d\xi _{z}}{dz}) \right)The magnetic contribution is:\delta ^{2} W_{m}=C_{1}\left\lbrace \beta \Delta \left(\frac{m}{R}B_{\phi }B_{z}\xi _{r} \xi _{\phi }-B_{\phi }B_{z}\frac{d\xi _{r}}{dz}\xi _{z}\right. \right.-...
{ "cite_spans": [] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.03024897538125515, 0.0013824071502313018, -0.036823514848947525, 0.006620300468057394, -0.04368788003921509, -0.028464240953326225, 0.027182891964912415, 0.005060563795268536, 0.0541217178106308, 0.002482612617313862, -0.013797377236187458, 0.022896476089954376, 0.0013881274498999119, 0...
285152d08b21b0d70db6fff94bb863f7835ee45f
subsection
18
19
Appendix: Generalized potential energy terms
\left. +\frac{5}{2}T_{0}^{3/2}\frac{d^{2}T_{0}}{ds^{2}}\right) +\frac{1}{\Delta ^{2}}T_{0}^{5/2}T_{1}\frac{d^{2}T_{1}}{dz^{2}}\right\rbraceThe new compressional contribution is expressed as:\delta ^{2} W_{c2}=-\beta \left(\frac{m}{R} \rho _{0}\xi _{\phi }T_{1}+\Delta \frac{d \rho _{0}}{ds} \xi _{z}T_{1}+\rho _{0}\xi _{...
{ "cite_spans": [] }
10.1051/0004-6361:20079052
0807.1722
Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles II. Modes in twisted non--isothermal magnetic field configurations
[ "A. Costa", "R. Gonzalez" ]
[ "astro-ph" ]
2,008
en
Physics
[ -0.025999154895544052, 0.0018604882061481476, -0.04287419095635414, 0.027555441483855247, -0.011283083818852901, -0.025419360026717186, 0.01280885562300682, 0.049190886318683624, 0.038205329328775406, 0.01830926351249218, -0.038083266466856, -0.019209468737244606, 0.002233348786830902, 0.0...
b1732164e2d6b083dfb2d2309d252ff660115e2a
abstract
0
20
Abstract
We investigate experimentally the mixing dynamics in a channel flow with a finite stirring region undergoing chaotic advection. We study the homogenization of dye in two variants of an eggbeater stirring protocol that differ in the extent of their mixing region. In the first case, the mixing region is separated from th...
{ "cite_spans": [] }
10.1063/1.3080680
0807.1723
Open-flow mixing: Experimental evidence for strange eigenmodes
[ "Emmanuelle Gouillart", "Olivier Dauchot", "Jean-Luc Thiffeault", "Stéphane Roux" ]
[ "nlin.CD" ]
2,008
en
Physics
[ -0.01677114889025688, -0.03595343604683876, -0.01965535804629326, 0.01748838648200035, -0.009400389157235622, -0.020036868751049042, -0.025271175429224968, 0.005051183048635721, -0.003458381863310933, 0.053350258618593216, -0.018602393567562103, -0.011353716254234314, 0.013940349221229553, ...
65101e7401e2c6e218da741151641447518461be
subsection
1
20
Introduction
Many industrial situations require the mixing of very viscous fluids, and involve mechanical stirring in order to achieve sufficient homogeneity. We investigate here the mixing scenario of a low-diffusivity dye in a free-surface open flow that crosses a localized stirring region. Relevant applications concern continuou...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 738, "openalex_id": "", "raw": "H. Aref, “Stirring by chaotic advection,” J. Fluid Mech. 143, 1 (1984).", "source_ref_id": "8940730c2dd56c7bc9f8c183e06ee1d2fc05b842", "start": 601 }, { "arxiv_id": "", ...
10.1063/1.3080680
0807.1723
Open-flow mixing: Experimental evidence for strange eigenmodes
[ "Emmanuelle Gouillart", "Olivier Dauchot", "Jean-Luc Thiffeault", "Stéphane Roux" ]
[ "nlin.CD" ]
2,008
en
Physics
[ -0.0034942219499498606, -0.026397395879030228, -0.050719622522592545, 0.0103300791233778, 0.018218781799077988, 0.02243015728890896, -0.0411372147500515, -0.00179574778303504, 0.001323684467934072, 0.03237877041101456, -0.0064009870402514935, -0.01664714515209198, 0.0407710075378418, 0.003...