Detection of 55-80 keV hydrogen atoms of heliospheric origin by CELIAS/HSTOF on Soho

被引：83

作者：

Hilchenbach, M ^{[1
]}

Hsieh, KC

Hovestadt, D

Klecker, B

Grünwaldt, H

Bochsler, P

Ipavich, FM

Bürgi, A

Möbius, E

Gliem, F

Axford, WI

Balsiger, H

Bornemann, W

Coplan, MA

Galvin, AB

Geiss, J

Gloeckler, G

Hefti, S

Judge, DL

Kallenbach, R

Laeverenz, P

Lee, MA

Livi, S

Managadze, GG

Marsch, E

Neugebauer, M

Ogawa, HS

Reiche, KU

Scholer, M

Verigin, MI

Wilken, B

Wurz, P

机构：

[1] Max Planck Inst Aeron, D-37189 Katlenburg Lindau, Germany

[2] Univ Arizona, Dept Phys, Tucson, AZ 85721 USA

[3] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany

[4] Univ Bern, Inst Phys, CH-3012 Bern, Switzerland

[5] Univ Maryland, Dept Phys & Astron, College Pk, MD 20742 USA

[6] ARIAS, CH-3012 Bern, Switzerland

[7] Univ New Hampshire, EOS, Durham, NH 03824 USA

[8] Tech Univ Carolo Wilhelmina Braunschweig, Inst Datenverarbeitungsanlagen, D-38023 Braunschweig, Germany

[9] Int Space Sci Inst, CH-3012 Bern, Switzerland

[10] Univ So Calif, Ctr Space Sci, Los Angeles, CA 90089 USA

[11] Inst Space Phys, Moscow, Russia

[12] Jet Prop Lab, Pasadena, CA 91103 USA

来源：

ASTROPHYSICAL JOURNAL | 1998年 / 503卷 / 02期

关键词：

cosmic rays; ISM : atoms; solar wind;

D O I：

10.1086/306022

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The High-Energy Suprathermal Time-of-Flight sensor (HSTOF) of the Charge, Element, and Isotope Analysis System (CELIAS) on the Solar and Heliospheric Observatory (SOHO) near the Lagrangian point L1 is capable of identifying energetic hydrogen atoms (EHAs) between 55 and 80 keV. Between 1996 February 13 and 1997 August 31, near solar minimum, there were 285 "quiet" days when the interplanetary charged-particle flux was low. During these quiet times, HSTOF scanned the apex of the heliosphere once and the antiapex twice. The flux level and time profile, and hence the arrival direction, of the EHAs accumulated during these quiet times are best interpreted as fluxes of EHAs coming from the heliosheath.

引用

页码：916 / 922

页数：7

共 27 条

[1] The heliosphere [J].

Axford, WI .

SPACE SCIENCE REVIEWS, 1996, 78 (1-2) :9-14

[2]

AXFORD WI, 1972, NASA PUBL, V308, P609

[3] OBSERVATIONS OF ANOMALOUS COSMIC-RAY HYDROGEN FROM THE VOYAGER SPACECRAFT [J].

CHRISTIAN, ER ;

CUMMINGS, AC ;

STONE, EC .

ASTROPHYSICAL JOURNAL, 1995, 446 (02) :L105-L108

[4] Composition of anomalous cosmic rays and implications for the heliosphere [J].

Cummings, AC ;

Stone, EC .

SPACE SCIENCE REVIEWS, 1996, 78 (1-2) :117-128

[5]

CZECHOWSKI A, 1995, ASTRON ASTROPHYS, V297, P892

[6] INTERPRETATION OF OBSERVED OXYGEN AND NITROGEN ENHANCEMENTS IN LOW-ENERGY COSMIC-RAYS [J].

FISK, LA ;

KOZLOVSK.B ;

RAMATY, R .

ASTROPHYSICAL JOURNAL, 1974, 190 (01) :L35-L37

[7]

Fleck B., 1995, SOHO MISSION

[8] NEW TEST FOR SOLAR MODULATION THEORY - 1972 MAY-JULY LOW-ENERGY GALACTIC COSMIC-RAY PROTON AND HELIUM SPECTRA [J].

GARCIAMUNOZ, M ;

MASON, GM ;

SIMPSON, JA .

ASTROPHYSICAL JOURNAL, 1973, 182 (02) :L81-L84

[9] Properties of the interstellar gas inside the heliosphere [J].

Geiss, J ;

Witte, M .

SPACE SCIENCE REVIEWS, 1996, 78 (1-2) :229-238

[10]

HO GC, 1997, UNPUB NIM B

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