Wilcox Solar Observatory, Stanford - PowerPoint PPT Presentation

1 / 21
About This Presentation
Title:

Wilcox Solar Observatory, Stanford

Description:

Wilcox Solar Observatory, Stanford – PowerPoint PPT presentation

Number of Views:25
Avg rating:3.0/5.0
Slides: 22
Provided by: SarahG64
Category:

less

Transcript and Presenter's Notes

Title: Wilcox Solar Observatory, Stanford


1
  • Wilcox Solar Observatory, Stanford

2
Solar eclipse HawaiiJuly 1989
3
The Sun!
4
(No Transcript)
5
(No Transcript)
6
(No Transcript)
7
(No Transcript)
8
(No Transcript)
9
(No Transcript)
10
(No Transcript)
11
(No Transcript)
12
(No Transcript)
13
Coronal Mass Ejections
14
Coronal Mass Ejections
White light (SOHO/LASCO) solar limb coronagraph
image of CME. Inner corona and solar disk seen
in extreme ultraviolet (SOHO/EIT).
15
The view from Earth
16
3D and twisted.
17
CME Onset Due to Loss of Confinement of Twisted
Magnetic Flux Ropes
  • What triggers coronal mass ejections (CMEs)?
    This is a fundamental question in solar
    astrophysics that must be answered for space
    weather prediction.
  • Magnetic twist can drive eruption. A 3D
    numerical simulation demonstrates that given
    enough twist, a magnetic flux rope can no longer
    be confined by the surrounding coronal magnetic
    field and will erupt in a CME.
  • Twist in eruptions is observed. Twisted
    internal structure and motion consistent with the
    model has been observed in CMEs.

Observation of a CME by HAO Mauna Loa Solar
Observatory Mk4 white-light coronagraph
MHD Simulation from Fan (2005)
18
Soft-X ray sigmoid brightening and associated
dimming
Fan and Gibson (in preparation)
Line-of-sight column integration of
Line-of-sight
  • Looking down on flux rope we see it as it would
    appear on the solar disk
  • Model predicts current sheets forming forward or
    backwards S shapes (depending on direction of
    flux rope twist)
  • X-ray observations show such S shapes
  • Model predicts twin density depletions within
    the S-shape (owl-eyes)
  • Observations sometimes show such twin dimmings
    during eruptions

Line-of-sight column integration of
Soft-X ray image from Yohkoh satellite during the
onset of a CME
19
Sigmoids
Sigmoids are generally visible in three ways
(Pevtsov, 2002)
persistent (long-lived)
transient (short-lived)
eruptive (transient sigmoid --gt cusp)
(Gibson et al., 2002)
20
Magnetic flux rope observables X-ray sigmoids
  • Sigmoid evolution -- evidence for flux rope
    before, during and after eruption (Gibson et al.,
    2004 2005)

eruptive (transient sigmoid --gt cusp)
persistent (long-lived)
transient (short-lived)
21
(No Transcript)
Write a Comment
User Comments (0)
About PowerShow.com