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Coronal magnetic field observations

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J.R. Kuhn, R. Coulter, H. Lin, D. Mickey. Are images enough? ... Roy Coulter, Jeff Kuhn, Haosheng Lin, Don Mickey. 100nm spectrograph. filter bandpass ... – PowerPoint PPT presentation

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Title: Coronal magnetic field observations


1
Coronal magnetic field observations
J.R. Kuhn, R. Coulter, H. Lin, D. Mickey
  • Useful coronal field model constraints can be
    obtained from IR observations
  • This is a vigorous activity, with three serious
    ongoing efforts (plus important solar radio
    measurements proposed)

2
Are images enough?
(from Chen et al., Low, Gibson, Roussev et al.)
3
Magnetic linear polarization sensitivity
B
QU
Q
E
4
Coronal Hanle measurements
  • Raouafi, Sahal-Bréchot, Lemaire, AA 396, 1019,
    2002.
  • OVI 103.2nm polarization measurement using CDS in
    a coronal hole (9, 9 degree from limb tangent)
  • Analysis non-unique solution requires both B of
    a few gauss and velocity of few 10s km/s

5
QU forbidden line observations
  • Habbal, Woo, Arnaud, Ap.J. 558, 825, 2001
  • FeXIII HAO/NSO KELP project 1980s

6
Coronal forbidden line Zeeman Observations
  • Lin, Penn, Tomczyk, ApJ, 541, L83 (2000)
  • FeXIII V polarimetry

7
Why IR Atmospheric backgrounds
8
IR expectations
  • Judge, Casini, Tomczyk, Burkepile... (http//comp.
    hao.ucar.edu/how.html)?

9
The IR corona
Kuhn et al. 1995, 1999
Also Judge et al., 2002
10
Ideal B measurement sensitivity
5 min observation, 10 pixel
11
Ongoing Coronal B efforts
  • COMP, Ground-Based Coronal Research Project (HAO
    lead)
  • ATST (NSO)
  • SOLARC (IfA)

12
SOLARCRoy Coulter, Jeff Kuhn, Haosheng Lin, Don
Mickey
3.93 micron
100nm spectrograph filter bandpass
13
Magnetic field measurements...
  • ...will be achieved in the quiet corona with a
    sensitivity of better than 1 G
  • ...from IR coronal observations obtained by
    several research groups using sensitive
    polarimetry techniques
  • ...on a timescale of one year

14
Vector Inversions
  • FF and potential model from Low (1993)
  • External potential fieldFF at rltR dipole
  • Radon transform using Algebraic Reconstruction
    Technique

z
y
Q
s
15
The projection problem
16
The inversion
10 iterations over 12 projections spaced 15
degrees...
17
Another inversion
6 projections, 0-90 degrees...
18
Potential field...
19
(No Transcript)
20
Long Wavelengths
Prime or Gregorian Focus
SOLARC
Fast 1-5mu IR Camera
chop
Warm IR Spectrograph
Cold Narrow-band filter
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