on the source of the solar wind
DESCRIPTION
On the Source of the solar wind. by Uri Feldman Artep Inc. The source of an underground river. Lakes. 1. Underground River. 2. 3. The Source of an under ground river. The solar wind composition is not always the same as the composition of the photosphere . - PowerPoint PPT PresentationTRANSCRIPT
On the Source of the solar wind
by
Uri Feldman
Artep Inc.
The source of an underground river
• Lakes
1
2
3
Underground River
The Source of an under ground river
•The solar wind composition is not always the same as the composition of the photosphere.
•In the Solar wind at times elements with first ionization potential (FIP) <10 eV are enriched.
Definition
FIP bias
coronal abundance/Photospheric abundance
In the fast SW elemental abundances are photospheric in nature , I.e. FIP bias~1
In the slow SW low-FIP elements are enriched by a factor of ~4. I.e., FIP bias~4
So where in the Solar Upper Atmosphere such conditions
exist?
The Sun at 106 K.
The Sun at 105 K
The Sun at 106 and 105 K
FIP-bias
Photosphere 1
105 K 1.5-2
106 K Coronal hole ~1
106 K Quiet Sun ~4
Elemental settling in the corona
1.00E+10
1.00E+11
1.00E+12
1.00E+13
1 1.1 1.2 1.3 1.4 1.5
Height (R)
Intensity (ph cm-2 s-1 sr-1)
Ne VIII
Mg X
Si XI
Si XII
Fe X
Fe XI
Fe XII
Atomic weights:
High-FIP Ne=20; Low-FIP Mg=24; Si=28; Low FIP Fe=56
Location of observations
-800
-600
-400
-200
0
200
400
600
800
1000 1100 1200 1300 1400 1500
East West coordinates (arcsec)
North south coordinates (arcsec)
Elemental settling in the western hemisphere
0.1
1
1 1.1 1.2 1.3 1.4 1.5 1.6
Height (R)
S XI/Fe XII Relative Intensity
450" N
450" S
150" N
150" S
750" N
750" S
Conclusions
1) The SW originates from ~106 K SUA plasmas
2) Slow SW originates in the quiet Sun corona close to the solar surface
3) Fast solar wind originates from the corona in coronal hole regions
C III at Sun Center
A Polar Region
An active region at different temperatures