Joule Heating and Anomalous Resistivity in the Solar Corona - PowerPoint PPT Presentation

1 / 13
About This Presentation
Title:

Joule Heating and Anomalous Resistivity in the Solar Corona

Description:

Main unknown is the resistivity: can calculate heating rate with Spitzer resistivity ... Conclusion: Joule heating rate with Spitzer conductivity is too low by ... – PowerPoint PPT presentation

Number of Views:60
Avg rating:3.0/5.0
Slides: 14
Provided by: StevenS49
Category:

less

Transcript and Presenter's Notes

Title: Joule Heating and Anomalous Resistivity in the Solar Corona


1
Joule Heating and Anomalous Resistivity in the
Solar Corona
  • Steven R. Spangler
  • University of Iowa

2
Invocation to the Muse
  • Coronal Heating is one of the major problems in
    astrophysics

3
Coronal heating theories AC and DC
  • Evaluation of DC (Joule heating) theories
    requires measurements of coronal currents

4
Radioastronomical measurement consistent with
coronal currents within a coronal Amperian Loop
  • Spangler, Astrophysical Journal 670, 841, 2007
  • Strongest case is for I2.5 GA

5
The implication for Joule heating of the corona
dependence on distribution of currents
2D MHD turbulence (e.g. Spangler ApJ 522, 879,
1999)
6
Development of strong current sheets is a generic
feature of 2D MHD turbulence
7
The Mr. Donut theory of coronal heating
Use this model to calculate The volumetric
heating rate
8
Two models for thin current sheets
  • Random distribution of positive and negative
    current sheets
  • Statistical preference for one sign of current

9
Expression for heating rate from model 1
resistivity
Properties of Current sheets
Observational properties
10
Main unknown is the resistivity can calculate
heating rate with Spitzer resistivity
suitable for observers form
Ohm-m
For coronal conditions
Ohm-m (35 times Resistivity of silver)
Calculated heating rates
11
The significance of Joule heating rate
comparison with inferred heating rates
Cranmer and Van Ballegooijen, ApJS 156, 265, 2005
12
Conclusion Joule heating rate with Spitzer
conductivity is too low by 6 orders of magnitude
  • Conclusion 1 currents detected by radio
    astronomy are irrelevant for coronal heating
    (strengthened by more common upper limits)
  • Conclusion 2 currents are relevant, and
    resistivity is enhanced by many orders of
    magnitude

13
Postscript current sheet model allows expression
for electron drift speed
  • Calculation is consistent with (or not
    inconsistent with)

It is plausible that the electron drift speeds
are sufficiently high To excite instabilities
which would enhance resistivity
Thanks
Write a Comment
User Comments (0)
About PowerShow.com