on the source of the solar wind

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On the Source of the solar wind by Uri Feldman Artep Inc.

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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 Presentation

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Page 1: On the Source of the solar wind

On the Source of the solar wind

by

Uri Feldman

Artep Inc.

Page 2: On the Source of the solar wind

The source of an underground river

• Lakes

1

2

3

Underground River

Page 3: On the Source of the solar wind

The Source of an under ground river

Page 4: On the Source of the solar wind

•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

Page 5: On the Source of the solar wind

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

Page 6: On the Source of the solar wind

So where in the Solar Upper Atmosphere such conditions

exist?

Page 7: On the Source of the solar wind

The Sun at 106 K.

Page 8: On the Source of the solar wind

The Sun at 105 K

Page 9: On the Source of the solar wind

The Sun at 106 and 105 K

Page 10: On the Source of the solar wind

FIP-bias

Photosphere 1

105 K 1.5-2

106 K Coronal hole ~1

106 K Quiet Sun ~4

Page 11: On the Source of the solar wind
Page 12: On the Source of the solar wind
Page 13: On the Source of the solar wind

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

Page 14: On the Source of the solar wind

Atomic weights:

High-FIP Ne=20; Low-FIP Mg=24; Si=28; Low FIP Fe=56

Page 15: On the Source of the solar wind

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)

Page 16: On the Source of the solar wind

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

Page 17: On the Source of the solar wind

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

Page 18: On the Source of the solar wind

C III at Sun Center

Page 19: On the Source of the solar wind

A Polar Region

Page 20: On the Source of the solar wind

An active region at different temperatures

Page 21: On the Source of the solar wind