Created visit 54 as a repeat of failed visit 04
Removed ORIENT from visit 54 to maximize scheduling.
1976692101
----- Attempting Submission 3 (Mon May 20 14:45:44 GMT 2013) -----
----- Attempting Submission 4 (Fri May 24 17:17:38 GMT 2013) -----
Will process in house
Optical Line Emission Impact Polarization: SN1006
We propose to probe the physics of shocks and transport processes by seeking the intrinsic line emission polarization predicted to be present in the classical non-radiative fast-shock remnant of SN1006. The prediction, Laming (1990), is that the narrow Balmer line core of the 2000 km/s shock in SN1006 will be polarized in the range 5-10% and that the broad wings will be unpolarized. The polarization is sensitive to shock velocity and ionization equilibrium. By measuring polarization for SN1006 we validate and enable a completely new diagnostic that has important applications in a wide variety of astrophysical situations involving anisotropic excitation mechanisms in general, such as shocks, intense radiation fields, high energy particle streams and conductive interfaces along with a substantial body of theoretical work that cuts across disciplines in this area. We also apply this diagnostic directly to the case of SN1006 and determine if our current theoretical expecations based on inferences on the shock velocity and structure are fullfilled. The observations will yield a spectacularly precise measurement of the proper motion distribution in the filaments of SN1006 and allow a direct estimate of its deceleration.
We will image the emission filaments of SN 1006 using the ACS Halpha filter together with the ACS polarizers. In parallel we will obtain WFC3 images. Each orbit is at a slightly different pointing to achieve effective dithering between similar images.
ISM AND CIRCUMSTELLAR MATTER
12
false
false
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false
false
false
AVAILABLE
CLUSTER OF GALAXIES
CONDUCTION FRONT
COOLING FLOW
EMISSION LINE NEBULA
FILAMENT
Proper motion for Region E of WInkler et al 2003 ApJ 585, 324.
J2000
J2000
Halpha surface brightness 5.3e-16 erg/s/cm2/arcsec
ACS/WFC
Imaging
No
Yes
F658N
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