2011ApJ...738..100H


Query : 2011ApJ...738..100H

2011ApJ...738..100H - Astrophys. J., 738, 100 (2011/September-1)

The adjoint method applied to time-distance helioseismology.

HANASOGE S.M., BIRCH A., GIZON L. and TROMP J.

Abstract (from CDS):

For a given misfit function, a specified optimality measure of a model, its gradient describes the manner in which one may alter properties of the system to march toward a stationary point. The adjoint method, arising from partial-differential-equation-constrained optimization, describes a means of extracting derivatives of a misfit function with respect to model parameters through finite computation. It relies on the accurate calculation of wavefields that are driven by two types of sources, namely, the average wave-excitation spectrum, resulting in the forward wavefield, and differences between predictions and observations, resulting in an adjoint wavefield. All sensitivity kernels relevant to a given measurement emerge directly from the evaluation of an interaction integral involving these wavefields. The technique facilitates computation of sensitivity kernels (Fréchet derivatives) relative to three-dimensional heterogeneous background models, thereby paving the way for nonlinear iterative inversions. An algorithm to perform such inversions using as many observations as desired is discussed.

Abstract Copyright: ∼

Journal keyword(s): magnetohydrodynamics, MHD - Sun: dynamo - Sun: helioseismology - Sun: interior - Sun: oscillations - waves

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Antennae IG 12 01 53.170 -18 52 37.92           ~ 1749 0

Query : 2011ApJ...738..100H

Basic data :
NAME Antennae -- Interacting Galaxies
Other object types:
otypes_help
PaG (), X (1E,2E,...), G (APG,2MASX), UV (FAUST,[DBA2001]), IR (IRAS,PSCz), GiG ([CHM2007]), IG (VV)
ICRS coord. (ep=J2000) :
12 01 53.170 -18 52 37.92 (Infrared) [ ] C 2006AJ....131.1163S
FK4 coord. (ep=B1950 eq=1950) :
11 59 19.356 -18 35 55.59 [ ]
Gal coord. (ep=J2000) :
286.962889 +42.452849 [ ]
Radial velocity / Redshift / cz :
V(km/s) 1574 [~] / z(emission) 0.005265 [~] / cz 1578.41 [~]
   (IR) C 2016ApJS..226...11S
Fluxes (3) :
J 8.110 [0.018] C 2006AJ....131.1163S
H 7.399 [0.019] C 2006AJ....131.1163S
K 7.177 [0.024] C 2006AJ....131.1163S
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 3
: 632
: 19 Display criteria :

Identifiers (20) :
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NAME NGC 4038/9 FAUST 2987 NAME Ring Tail [CHM2007] HDC 684 J120153.17-1852379
APG 244 IRAS F11593-1836 NAME the Antennae [CHM2007] LDC 856 J120153.17-1852379
1E 1159.3-1835 IRAS 11593-1835 PSCz Q11593-1835 [DBA2001] FA33
2E 2573 2MASX J12015317-1852379 1RXS J120151.5-185214
2E 1159.3-1835 NAME Antennae VV 245

References (1749 between 1850 and 2026) (Total 1749)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 2    Distance : 4   

   

Observing logs
Herschel : 50    ISO : 37    XMM : 2   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : NAME Antennae

Link by name to the catalogue in VizieR :

APG 244 2E 2573 FAUST 2987 IRAS F11593-1836 IRAS 11593-1835
2MASX J12015317-1852379 1RXS J120151.5-185214 [DBA2001] FA33

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