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Streamer disconnection events observed with the LASCO coronagraph
DOI: 10.1029/1999GL900177 Bibcode: 1999GeoRL..26.1349W

Lamy, P. L.; Howard, R. A.; Sheeley, N. R., Jr. +2 more

We present Large Angle Spectrometric Coronagraph (LASCO) observations of two events that suggest magnetic disconnection in coronal streamers. During the 1-2 days preceding each event, successions of narrow looptops are seen rising slowly through the 2-6 RS field of view, forming a bright streamer stalk which continues to elongate with t…

1999 Geophysical Research Letters
SOHO 42
Evidence of a solar origin for pressure balance structures in the high-latitude solar wind
DOI: 10.1029/1999GL900368 Bibcode: 1999GeoRL..26.1805R

Reisenfeld, D. B.; McComas, D. J.; Steinberg, J. T.

Ulysses observations of the high-latitude solar wind have shown that on time scales of < 1 day, the polar wind is dominated by pressure balance structures (PBSs). Fluctuations of the plasma beta within PBSs appear to be strongly correlated with fluctuations in the helium abundance. The correlation occurs in both the northern and southern hemisp…

1999 Geophysical Research Letters
Ulysses 41
Differences in the temporal variations of galactic cosmic ray electrons and protons: Implications from Ulysses at solar minimum
DOI: 10.1029/1999GL900482 Bibcode: 1999GeoRL..26.2133H

Sierks, H.; Kunow, H.; Bothmer, V. +8 more

According to standard drift dominated modulation models the intensity variations of galactic cosmic ray protons and electrons respond differently to the latitudinal extension of the heliospheric current sheet α. In an A>0 solar cycle intensities of protons should vary weakly with the latitudinal extension, whereas electrons should show a strong…

1999 Geophysical Research Letters
Ulysses 33
The global nature of solar cycle variations of the solar wind dynamic pressure
DOI: 10.1029/1999GL900052 Bibcode: 1999GeoRL..26..561R

Wang, Chi; Richardson, John

The solar wind dynamic pressure measured near the ecliptic varies over the solar cycle. A major unanswered question has been whether this variation is a global feature or restricted to low latitudes and thus perhaps a consequence of the changing heliospheric current sheet configuration. We use plasma data from IMP-8, Ulysses and Voyager 2 to show …

1999 Geophysical Research Letters
Ulysses 28
Direct evidence of the interstellar gas flow velocity in the pickup ion cut-off as observed with SOHO CELIAS CTOF
DOI: 10.1029/1999GL003644 Bibcode: 1999GeoRL..26.3181M

Bochsler, P.; Klecker, B.; Möbius, E. +9 more

He+ pickup ions as observed with SOHO CELIAS CTOF have been analyzed for the time period DOY 160-190, 1996. During this time of the year the Earth is on the upwind side of the interstellar gas flow with respect to the sun. The high-speed cut-off in the frame of the sun is significantly higher v/Vsw = 2, predicted for pickup i…

1999 Geophysical Research Letters
SOHO 27
Ion-cyclotron wave dissipation channel for Alfvén waves
DOI: 10.1029/1999GL900343 Bibcode: 1999GeoRL..26.1817K

Kaghashvili, Edisher Kh.

The effect of inhomogeneous velocity flow on Alfvén wave dynamics in the solar wind is investigated. Unlike existing studies in this field that model energy deposition from high-frequency waves to solar wind particles, we consider here the possibility of obtaining high-frequency waves (in this case fast magnetosonic waves) from the ordinary Alfvén…

1999 Geophysical Research Letters
SOHO 24
Ulysses measurements of variations in the solar wind-interstellar hydrogen charge exchange rate
DOI: 10.1029/1999GL900519 Bibcode: 1999GeoRL..26.2701M

McComas, D. J.; Gosling, J. T.; Pryor, W. R. +1 more

Charge exchange with solar wind protons is the primary ionization process for interstellar hydrogen traveling through the heliosphere. In this study we use Ulysses solar wind observations to examine and quantify variations in charge exchange. We find that these variations are largest within stream interaction regions where the charge exchange rate…

1999 Geophysical Research Letters
Ulysses 24
Radial evolution of density structure in the solar corona
DOI: 10.1029/1999GL900366 Bibcode: 1999GeoRL..26.1793W

Habbal, Shadia Rifai; Woo, Richard

White-light measurements made by the SOHO coronagraphs (LASCO for Large Angle Spectrometric Coronagraph) and the HAO Mauna Loa Mk III K-coronameter are combined to follow the evolution of path-integrated density structure in the solar corona overlying both coronal hole and quiet Sun regions from 1.15 to 5.5 Ro. The global imaging provid…

1999 Geophysical Research Letters
SOHO 23
Observations of heliospheric planar and offset-planar magnetic structures
DOI: 10.1029/1998GL900258 Bibcode: 1999GeoRL..26...13J

Balogh, A.; Jones, G. H.; Horbury, T. S.

Planar magnetic structures are regions of solar wind plasma where the magnetic field orientation is constrained within a fixed plane for durations of several hours. Within these structures, magnetic field discontinuities are seen, with the discontinuity surfaces being almost co-planar. The results of a survey of planar magnetic strutures detected …

1999 Geophysical Research Letters
Ulysses 21
The electron heat flux in the polar solar wind: Ulysses observations
DOI: 10.1029/1999GL900503 Bibcode: 1999GeoRL..26.2129S

Scime, Earl E.; Littleton, J. E.; Badeau, Allen E., Jr.

Ulysses measurements of the solar wind electron heat flux as a function of heliographic latitude are presented. Contamination from a light leak at the highest latitudes has been removed from the data by interpolating between uncontaminated pixels. After normalization by the radial gradient in the electron heat flux obtained during the inecliptic p…

1999 Geophysical Research Letters
Ulysses 19