Energetic particles near and beyond the solar-wind termination

J. R. Jokipii

doi:10.1063/1.2359319

Energetic particles near and beyond the solar-wind termination

J. R. Jokipii

Lunar and Planetary Lab

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

9 Scopus citations

Abstract

A global picture of the transport and acceleration of energetic particles in the heliosphere has evolved over the last few decades, which has successfully explained many features of the modulation of galactic cosmic rays and the transport of anomalous cosmic rays and their acceleration by the solar-wind termination shock. Recent Voyager observations near and beyond the termination shock have revealed new and in some cases unexpected phenomena which have led to questions concerning the established paradigm. The physical interpretation of the observations requires a blunt termination shock, rapid inward motion of the shock and temporal variations over time scales ranging from hours to 22 years. Incorporation of these into the physics has promise of explaining most if not all of the observed phenomena while retaining the advantages of the termination shock paradigm for both galactic and anomalous cosmic rays.

Original language	English (US)
Title of host publication	PHYSICS OF THE INNER HELIOSHEATH
Subtitle of host publication	Voyager Observations, Theory, and Future Prospects; 5th Annual IGPP International Astrophysics Conference
Publisher	American Institute of Physics Inc.
Pages	143-152
Number of pages	10
ISBN (Print)	0735403554, 9780735403550
DOIs	https://doi.org/10.1063/1.2359319
State	Published - 2006
Event	PHYSICS OF THE INNER HELIOSHEATH: Voyager Observations, Theory, and Future Prospects; 5th Annual IGPP International Astrophysics Conference - Oahu, HI, United States Duration: Mar 3 2006 → Mar 9 2006

Publication series

Name	AIP Conference Proceedings
Volume	858
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	PHYSICS OF THE INNER HELIOSHEATH: Voyager Observations, Theory, and Future Prospects; 5th Annual IGPP International Astrophysics Conference
Country/Territory	United States
City	Oahu, HI
Period	3/3/06 → 3/9/06

Keywords

Cosmic rays
Heliopause and solar wind termination
Interplanetary magnetic fields
Particle acceleration

ASJC Scopus subject areas

General Physics and Astronomy

Access to Document

10.1063/1.2359319

Cite this

Energetic particles near and beyond the solar-wind termination. / Jokipii, J. R.
PHYSICS OF THE INNER HELIOSHEATH: Voyager Observations, Theory, and Future Prospects; 5th Annual IGPP International Astrophysics Conference. American Institute of Physics Inc., 2006. p. 143-152 (AIP Conference Proceedings; Vol. 858).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Jokipii, JR 2006, Energetic particles near and beyond the solar-wind termination. in PHYSICS OF THE INNER HELIOSHEATH: Voyager Observations, Theory, and Future Prospects; 5th Annual IGPP International Astrophysics Conference. AIP Conference Proceedings, vol. 858, American Institute of Physics Inc., pp. 143-152, PHYSICS OF THE INNER HELIOSHEATH: Voyager Observations, Theory, and Future Prospects; 5th Annual IGPP International Astrophysics Conference, Oahu, HI, United States, 3/3/06. https://doi.org/10.1063/1.2359319

@inproceedings{e243adf6f7a440929ecb22dcce505318,

title = "Energetic particles near and beyond the solar-wind termination",

abstract = "A global picture of the transport and acceleration of energetic particles in the heliosphere has evolved over the last few decades, which has successfully explained many features of the modulation of galactic cosmic rays and the transport of anomalous cosmic rays and their acceleration by the solar-wind termination shock. Recent Voyager observations near and beyond the termination shock have revealed new and in some cases unexpected phenomena which have led to questions concerning the established paradigm. The physical interpretation of the observations requires a blunt termination shock, rapid inward motion of the shock and temporal variations over time scales ranging from hours to 22 years. Incorporation of these into the physics has promise of explaining most if not all of the observed phenomena while retaining the advantages of the termination shock paradigm for both galactic and anomalous cosmic rays.",

keywords = "Cosmic rays, Heliopause and solar wind termination, Interplanetary magnetic fields, Particle acceleration",

author = "Jokipii, {J. R.}",

year = "2006",

doi = "10.1063/1.2359319",

language = "English (US)",

isbn = "0735403554",

series = "AIP Conference Proceedings",

publisher = "American Institute of Physics Inc.",

pages = "143--152",

booktitle = "PHYSICS OF THE INNER HELIOSHEATH",

note = "PHYSICS OF THE INNER HELIOSHEATH: Voyager Observations, Theory, and Future Prospects; 5th Annual IGPP International Astrophysics Conference ; Conference date: 03-03-2006 Through 09-03-2006",

}

TY - GEN

T1 - Energetic particles near and beyond the solar-wind termination

AU - Jokipii, J. R.

PY - 2006

Y1 - 2006

N2 - A global picture of the transport and acceleration of energetic particles in the heliosphere has evolved over the last few decades, which has successfully explained many features of the modulation of galactic cosmic rays and the transport of anomalous cosmic rays and their acceleration by the solar-wind termination shock. Recent Voyager observations near and beyond the termination shock have revealed new and in some cases unexpected phenomena which have led to questions concerning the established paradigm. The physical interpretation of the observations requires a blunt termination shock, rapid inward motion of the shock and temporal variations over time scales ranging from hours to 22 years. Incorporation of these into the physics has promise of explaining most if not all of the observed phenomena while retaining the advantages of the termination shock paradigm for both galactic and anomalous cosmic rays.

AB - A global picture of the transport and acceleration of energetic particles in the heliosphere has evolved over the last few decades, which has successfully explained many features of the modulation of galactic cosmic rays and the transport of anomalous cosmic rays and their acceleration by the solar-wind termination shock. Recent Voyager observations near and beyond the termination shock have revealed new and in some cases unexpected phenomena which have led to questions concerning the established paradigm. The physical interpretation of the observations requires a blunt termination shock, rapid inward motion of the shock and temporal variations over time scales ranging from hours to 22 years. Incorporation of these into the physics has promise of explaining most if not all of the observed phenomena while retaining the advantages of the termination shock paradigm for both galactic and anomalous cosmic rays.

KW - Cosmic rays

KW - Heliopause and solar wind termination

KW - Interplanetary magnetic fields

KW - Particle acceleration

UR - http://www.scopus.com/inward/record.url?scp=33846483589&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=33846483589&partnerID=8YFLogxK

U2 - 10.1063/1.2359319

DO - 10.1063/1.2359319

M3 - Conference contribution

AN - SCOPUS:33846483589

SN - 0735403554

SN - 9780735403550

T3 - AIP Conference Proceedings

SP - 143

EP - 152

BT - PHYSICS OF THE INNER HELIOSHEATH

PB - American Institute of Physics Inc.

T2 - PHYSICS OF THE INNER HELIOSHEATH: Voyager Observations, Theory, and Future Prospects; 5th Annual IGPP International Astrophysics Conference

Y2 - 3 March 2006 through 9 March 2006

ER -

Energetic particles near and beyond the solar-wind termination

Abstract

Publication series

Other

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this