scholarly journals Composition of quasi-stationary solar wind flows from Ulysses/Solar Wind Ion Composition Spectrometer

2000 ◽  
Vol 105 (A12) ◽  
pp. 27217-27238 ◽  
Author(s):  
R. von Steiger ◽  
N. A. Schwadron ◽  
L. A. Fisk ◽  
J. Geiss ◽  
G. Gloeckler ◽  
...  
Keyword(s):  
Solar Wind ◽  
Ion Composition ◽  
Wind Flows

The solar wind interaction with Mars: Consideration of Phobos 2 mission observations of an ion composition boundary on the dayside

1991 ◽  
Vol 96 (A7) ◽  
pp. 11165 ◽  
Author(s):  
T. K. Breus ◽  
A. M. Krymskii ◽  
R. Lundin ◽  
E. M. Dubinin ◽  
J. G. Luhmann ◽  
...  
Keyword(s):  
Solar Wind ◽  
Ion Composition ◽  
Solar Wind Interaction

Solar Wind Ion Composition

1968 ◽  
Vol 20 (8) ◽  
pp. 393-395 ◽  
Author(s):  
S. J. Bame ◽  
A. J. Hundhausen ◽  
J. R. Asbridge ◽  
I. B. Strong
Keyword(s):  
Solar Wind ◽  
Ion Composition

scholarly journals Observations of Interplanetary Scintillation and a Theory of High-Speed Solar Wind

1980 ◽  
Vol 91 ◽  
pp. 499-502
Author(s):  
H. Washimi ◽  
T. Kakinuma ◽  
M. Kojima
Keyword(s):  
Solar Wind ◽  
High Speed ◽  
Coronal Holes ◽  
Polar Regions ◽  
Interplanetary Scintillation ◽  
Speed Flow ◽  
Low Latitudes ◽  
Speed Solar Wind ◽  
Wind Flows ◽  
High Speed Solar Wind

It has been confirmed that the high-speed solar wind flows out of the coronal holes at low latitudes, where the magnetic fields open and the temperature is low (e.g., Krieger et al. 1973). But there has not been direct observation of the solar wind out of the polar regions of corona. We report here that the observations of interplanetary scintillation (IPS) show the existence of the high-speed flow of 800 km/s out of the polar coronal regions and the well-coincidence to the model of the coronal holes extending from the polar regions.

Implantation of ions escaping the atmosphere of Mars within the regolith of Phobos, and Phobos’ surface ion weathering

2020 ◽  
Author(s):  
Quentin Nénon ◽  
Andrew R Poppe ◽  
Ali Rahmati ◽  
James P McFadden
Keyword(s):  
Solar Wind ◽  
Atomic Oxygen ◽  
The Moon ◽  
Ion Composition ◽  
Atmospheric Escape ◽  
The Past ◽  
Lunar Samples ◽  
Singly Charged

<p>Mars has lost and is losing its atmosphere into space. Strong evidences of this come from the observation of planetary singly charged heavy ions (atomic oxygen, molecular oxygen, carbon dioxide ions) by Mars Express and MAVEN. Phobos, the closest moon of Mars, orbits only 6,000 kilometers above the red planet’s surface and is therefore a unique vantage point of the planetary atmospheric escape, with the escaping ions being implanted within the regolith of Phobos and altering the properties of the moon’s surface.</p> <p>In this presentation, we aggregate all ion observations gathered in-situ close to the orbit of Phobos by three ion instruments onboard MAVEN, from 2015 to 2019, to constrain the long-term averaged ion environment seen by the Martian moon at all longitudes along its orbit. In particular, the SupraThermal and Thermal Ion Composition (STATIC) instrument onboard MAVEN distinguishes between solar wind and planetary ions. The newly constrained long-term ion environment seen by Phobos is combined with numerical simulations of ion transport and effects in matter.</p> <p>This way, we find that planetary ions are implanted on the near side of Phobos (pointing towards Mars) inside the uppermost tens of nanometers of regolith grains. The composition of near-side grains that may be sampled by future Phobos sample return missions is therefore not only contaminated by planetary ions, as seen in lunar samples with the terrestrial atmosphere, but may show a unique record of the past atmosphere of Mars.</p> <p>The long-term fluxes of planetary ions precipitating onto Phobos are so intense that these ions weather the moon’s surface as much as or more than solar wind ions. In particular, Martian ions accelerate the long-term sputtering and amorphization of the near side regolith by a factor of 2. Another implication is that ion weathering is highly asymmetric between the near side and far side of Phobos.</p>

Solar Wind Ion Composition

1970 ◽  
Vol 75 (31) ◽  
pp. 6354-6359 ◽  
Author(s):  
T. E. Holzer ◽  
W. I. Axford
Keyword(s):  
Solar Wind ◽  
Ion Composition

Solar wind composition measurements by the Ulysses SWICS experiment during transient solar wind flows

1993 ◽  
Vol 13 (6) ◽  
pp. 75-78 ◽  
Author(s):  
A.B. Galvin ◽  
G. Gloeckler ◽  
F.M. Ipavich ◽  
C.M. Shafer ◽  
J. Geiss ◽  
...  
Keyword(s):  
Solar Wind ◽  
Wind Flows ◽  
Solar Wind Composition ◽  
Composition Measurements

Evidence of an ion composition boundary (protonopause) in bi-ion fluid simulations of solar wind mass loading

1994 ◽  
Vol 21 (20) ◽  
pp. 2255-2258 ◽  
Author(s):  
Konard Sauer ◽  
Alexander Bogdanov ◽  
Klaus Baumgärtel
Keyword(s):  
Solar Wind ◽  
Mass Loading ◽  
Ion Composition

Relationships of quasi-stationary solar wind flows with their sources on the Sun

Solar Physics ◽  
1992 ◽  
Vol 137 (1) ◽  
pp. 179-197 ◽  
Author(s):  
V. G. Eselevich
Keyword(s):  
Solar Wind ◽  
The Sun ◽  
Wind Flows
Sign in / Sign up

Export Citation Format

Share Document