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Title: OBSERVATIONS OF THE INTERPLANETARY HYDROGEN DURING SOLAR CYCLES 23 AND 24. WHAT CAN WE DEDUCE ABOUT THE LOCAL INTERSTELLAR MEDIUM?

Abstract

Observations of interstellar helium atoms by the Interstellar Boundary Explorer (IBEX) spacecraft in 2009 reported a local interstellar medium (LISM) velocity vector different from the results of the Ulysses spacecraft between 1991 and 2002. The interplanetary hydrogen (IPH), a population of neutrals that fills the space between planets inside the heliosphere, carries the signatures of the LISM and its interaction with the solar wind. More than 40 yr of space-based studies of the backscattered solar Lyα emission from the IPH provided limited access to the velocity distribution, with the first temporal evolution map of the IPH line-shift during solar cycle 23. This work presents the results of the latest IPH observations made by the Hubble Space Telescope's Space Telescope Imaging Spectrograph during solar cycle 24. These results have been compiled with previous measurements, including data from the Solar Wind Anisotropies instrument on the Solar and Heliospheric Observatory. The whole set has been compared to physically realistic models to test both sets of LISM physical parameters as measured by Ulysses and IBEX, respectively. This comparison shows that the LISM velocity vector has not changed significantly since Ulysses measurements.

Authors:
; ;  [1]; ;  [2];  [3];  [4];  [5]
  1. Université Versailles St.-Quentin, Sorbonne Universités, UPMC Univ. Paris 06, CRNS/INSU, LATMOS-IPSL, 11 boulevard d'Alembert, 78280 Guyancourt (France)
  2. Space Research Institute of Russian Academy of Sciences, Moscow (Russian Federation)
  3. UPMC Univ. Paris 06, UMR7095, Institut d'Astrophysique de Paris, F-75014, Paris (France)
  4. University of Arizona, Lunar and Planetary Laboratory, 1629 E. University Blvd., Tucson, AZ 85721 (United States)
  5. Center for Space Physics, Boston University, 725 Commonwealth Avenue, Boston, MA 02215 (United States)
Publication Date:
OSTI Identifier:
22365779
Resource Type:
Journal Article
Journal Name:
Astrophysical Journal Letters
Additional Journal Information:
Journal Volume: 788; Journal Issue: 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 2041-8205
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ANISOTROPY; ATOMS; COMPARATIVE EVALUATIONS; HELIOSPHERE; HELIUM; HYDROGEN; INTERSTELLAR SPACE; LYMAN LINES; PLANETS; SOLAR CYCLE; SOLAR WIND; SPACE; SUN; TELESCOPES; ULTRAVIOLET RADIATION; VELOCITY

Citation Formats

Vincent, Frédéric E., Quémerais, Eric, Koutroumpa, Dimitra, Katushkina, Olga, Izmodenov, Vladislav, Ben-Jaffel, Lotfi, Harris, Walter M., and Clarke, John. OBSERVATIONS OF THE INTERPLANETARY HYDROGEN DURING SOLAR CYCLES 23 AND 24. WHAT CAN WE DEDUCE ABOUT THE LOCAL INTERSTELLAR MEDIUM?. United States: N. p., 2014. Web. doi:10.1088/2041-8205/788/2/L25.
Vincent, Frédéric E., Quémerais, Eric, Koutroumpa, Dimitra, Katushkina, Olga, Izmodenov, Vladislav, Ben-Jaffel, Lotfi, Harris, Walter M., & Clarke, John. OBSERVATIONS OF THE INTERPLANETARY HYDROGEN DURING SOLAR CYCLES 23 AND 24. WHAT CAN WE DEDUCE ABOUT THE LOCAL INTERSTELLAR MEDIUM?. United States. doi:10.1088/2041-8205/788/2/L25.
Vincent, Frédéric E., Quémerais, Eric, Koutroumpa, Dimitra, Katushkina, Olga, Izmodenov, Vladislav, Ben-Jaffel, Lotfi, Harris, Walter M., and Clarke, John. Fri . "OBSERVATIONS OF THE INTERPLANETARY HYDROGEN DURING SOLAR CYCLES 23 AND 24. WHAT CAN WE DEDUCE ABOUT THE LOCAL INTERSTELLAR MEDIUM?". United States. doi:10.1088/2041-8205/788/2/L25.
@article{osti_22365779,
title = {OBSERVATIONS OF THE INTERPLANETARY HYDROGEN DURING SOLAR CYCLES 23 AND 24. WHAT CAN WE DEDUCE ABOUT THE LOCAL INTERSTELLAR MEDIUM?},
author = {Vincent, Frédéric E. and Quémerais, Eric and Koutroumpa, Dimitra and Katushkina, Olga and Izmodenov, Vladislav and Ben-Jaffel, Lotfi and Harris, Walter M. and Clarke, John},
abstractNote = {Observations of interstellar helium atoms by the Interstellar Boundary Explorer (IBEX) spacecraft in 2009 reported a local interstellar medium (LISM) velocity vector different from the results of the Ulysses spacecraft between 1991 and 2002. The interplanetary hydrogen (IPH), a population of neutrals that fills the space between planets inside the heliosphere, carries the signatures of the LISM and its interaction with the solar wind. More than 40 yr of space-based studies of the backscattered solar Lyα emission from the IPH provided limited access to the velocity distribution, with the first temporal evolution map of the IPH line-shift during solar cycle 23. This work presents the results of the latest IPH observations made by the Hubble Space Telescope's Space Telescope Imaging Spectrograph during solar cycle 24. These results have been compiled with previous measurements, including data from the Solar Wind Anisotropies instrument on the Solar and Heliospheric Observatory. The whole set has been compared to physically realistic models to test both sets of LISM physical parameters as measured by Ulysses and IBEX, respectively. This comparison shows that the LISM velocity vector has not changed significantly since Ulysses measurements.},
doi = {10.1088/2041-8205/788/2/L25},
journal = {Astrophysical Journal Letters},
issn = {2041-8205},
number = 2,
volume = 788,
place = {United States},
year = {2014},
month = {6}
}