[PDF] Top 20 Solar Wind Charge Exchange Emission from the Helium Focusing Cone: Model to Data Comparison
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Solar Wind Charge Exchange Emission from the Helium Focusing Cone: Model to Data Comparison
... panel: model and data 1 4 keV surface brightnesses for the ...SEP. The plain curves are the total (upper) and LTE-corrected (lower) RASS 1 4 keV ...fluxes. The diamonds are ... Voir le document complet
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Solar Wind Charge Exchange Emission in the Chandra Deep Field North
... of the Sun resulting in a substantially enhanced region of SWCX emission on the downwind side of the Sun known as the He focusing cone (see Figure 1 ...). The ... Voir le document complet
13
Solar wind charge exchange X-ray emission from Mars.
... wish to thank our referee Thomas Cravens for his per- tinent remarks and our editor Tristan Guillot for stimulating the discussion on ...grateful to the ACE SWICS and SWEPAM instrument teams ... Voir le document complet
11
The Solar Wind Charge-eXchange Contribution to the Local Soft X-ray Background. Model to Data Comparison in the 0.1–1.0 keV Band
... on the SWCX soft X-ray emission in the heliosphere in the ...compared to data from past and present observing ...ranges: the 3/4 keV, dominated by the oxygen ... Voir le document complet
16
The Helium Focusing Cone of the Local Interstellar Medium Close to the Sun
... Finally, the third group of observations gathers data from when the UVCS line of sight deviates substantially from the direction of the interstellar ...of model ... Voir le document complet
12
WIND observations of coherent electrostatic waves in the solar wind
... On the other hand, the TDS provides simultaneous measurements Ex and Ey of the electric ®eld amplitude on the two orthogonal x and y ...used to obtain the polarisation of ... Voir le document complet
15
Response of Jupiter's and Saturn's auroral activity to the solar wind
... with solar wind con- ...with solar wind pressure values measured by the Ulysses spacecraft, and a correlation reported between the log of changes in solar wind ... Voir le document complet
20
Marine productivity response to Heinrich events: a model-data comparison
... In the SEP area, EXP decrease by 17 % in the model (Ta- ble 2), in contrast to the NZL ...Our model simulates increasing Austral winter sea ice that isolates the surface ... Voir le document complet
19
The origin of slow Alfvénic solar wind at solar minimum
... Although the origins of slow solar wind are unclear, there is increasing evidence that at least some of it is released in a steady state on overexpanded coronal hole magnetic field ...slow ... Voir le document complet
7
Isotopic Composition of the Solar Wind Inferred from In-Situ Spacecraft Measurements
... Abstract The Sun is the largest reservoir of matter in the solar system, which formed ...ago from the protosolar nebula. Data from space missions and theoretical ... Voir le document complet
10
Minor ions in the solar wind
... in the solar ...on the dynamics of the interplanetary ...of the formation, on the acceleration and on the transfer of solar plasma from the corona ... Voir le document complet
40
Polar ionospheric responses to solar wind IMF changes
... optical data have been complementory; while the DMSP particle data provide good spatial resolution and details of electron spectral in¯ux, the optical data provide the temporal ... Voir le document complet
12
EISCAT measurements of the solar wind
... used to measure the velocity of the solar wind at distances between 15 and 130 R x (solar radii) from the ...Sun. The results show that the ... Voir le document complet
12
Cone-Enriched Cultures from the Retina of Chicken Embryos to Study Rod to Cone Cellular Interactions
... genetic model of the disease led to the concept of cell interactions between rods and cones and of non-cell autonomous degeneration of cones in all genetic forms of retinitis ...in the ... Voir le document complet
17
Solar wind energy flux observations in the inner heliosphere: first results from Parker Solar Probe
... Normalizing the solar wind energy flux as 1/r 2 assumes a radial expansion of solar wind, which does not hold true for individual flux tubes, especially close to the ... Voir le document complet
8
Modelling the solar wind interaction with Mercury by a quasi-neutral hybrid model
... fluid. The approach has received an in- creasing interest in space plasma physics research because it makes it possible to study several plasma physical processes that are difficult or impossible to ... Voir le document complet
14
Estimating the contribution from different ionospheric regions to the TEC response to the solar flares using data from the international GPS network
... grateful to E. A. Kosogorov and O. S. Lesuta for preparing the input ...due to V. G. Mikhalkosky for his assistance in preparing the English version of the ...Finally, the ... Voir le document complet
8
Multifractality and intermittency in the solar wind
... illustration the results for D q + 3 and f (α), fitted to the experimental values of the generalized dimensions with ...and the de- gree of multifractality should be stronger for ... Voir le document complet
7
The magnetosphere under weak solar wind forcing
... electron data acquired by the DMSP-F13 spacecraft during a 14-min-long pass over the Northern Hemisphere at high ...latitudes. From top to bottom: ion density, magnetic field ... Voir le document complet
16
Developing a Universal Exchange Format for Integrated Circuit Emission Model – Conducted Emissions
... emissions, Data Exchange, XML, Standarization ...1) The starting point is an appreciation and acceptation that EMC modeling of components is no longer a fringe activity; it is reached a state that it ... Voir le document complet
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