Reconstruction of the magnetic connection from Mercury to the solar corona during enhancements in the solar proton fluxes at Mercury

Author(s):  
A. Ippolito ◽  
C. Plainaki ◽  
G. Zimbardo ◽  
T. Alberti ◽  
S. Massetti ◽  
...  
2021 ◽  
Author(s):  
Alessandro Ippolito ◽  
Christina Plainaki ◽  
Gaetano Zimbardo ◽  
Tommaso Alberti ◽  
Stefano Massetti ◽  
...  

<p>We present a study conducted on a number of selected events characterised by a significant increase in the solar proton fluxes measured by FIPS-MESSENGER during the period 2011-2013. For each of them, the magnetic connection between Mercury and the solar corona (Source Surface Field @2.5 R<sub>S</sub>) has been reconstructed, in order to identify the possible source of the accelerated particles on the solar surface. The transport of the magnetic field lines in the heliosphere is here evaluated with a Monte Carlo code that computes a random displacement at each step of the integration along the Parker magnetic field model. Such displacement is proportional to a “local” diffusion coefficient, which is a function of the fluctuation level and magnetic turbulence correlation lengths. The simulation is tailored to the specific events by using the observed values of solar wind velocity and magnetic fluctuation levels.</p>


2004 ◽  
Vol 42 (3) ◽  
pp. 203-209 ◽  
Author(s):  
N. V. Kuznetsov ◽  
R. A. Nymmik ◽  
M. I. Panasyuk ◽  
E. N. Sosnovets ◽  
M. V. Teltsov

1968 ◽  
Vol 46 (10) ◽  
pp. S812-S818 ◽  
Author(s):  
S. N. Vernov ◽  
E. V. Gortchakov ◽  
Yu. I. Logatchov ◽  
G. P. Lyubimov ◽  
N. V. Pereslegina ◽  
...  

This work studies the structure of interplanetary space between the orbits of Venus and Mars on the basis of solar proton streaming and cosmic-ray variations measured from Soviet and U.S. spacecraft. Solar proton fluxes measured from spacecraft at various distances from the sun and in various solar activity phases are intercompared. The problem of the large radial gradient of protons with energies of 1–5 MeV is discussed.


1972 ◽  
Vol 77 (34) ◽  
pp. 6656-6664 ◽  
Author(s):  
J. G. Greenhill ◽  
K. B. Fenton ◽  
A. G. Fenton ◽  
K. S. White
Keyword(s):  

2006 ◽  
Vol 6 (12) ◽  
pp. 5307-5314 ◽  
Author(s):  
C. M. Hall ◽  
A. H. Manson ◽  
C. E. Meek ◽  
S. Nozawa

Abstract. We have noted sporadic instances of strong isolated reflections of medium frequency (MF) radar waves from the mesosphere from as low as 50 km altitude and have devised a set of criteria for isolating these apparently anomalous echoes from those normally occurring from progressive partial reflections in the D-region. The object of this study is to map the occurrences of such echoes facilitating comparisons with other observations. For example, the similarity and simultaneity of the echo structure for the 20 January 2005 with VHF radar results presented by Lübken et al. (2006) are particularly striking. In presenting a number of such echo events since 2001 selected from the MF radar dataset (which spans 1997 to present), we find that virtually all echo occurrences coincide with enhanced solar proton fluxes suggesting that substantial ionisation of the mesosphere is a necessary condition. Strong partial reflections of the radio wave in the lower mesosphere combined with seasonally varying total absorption higher up, thus giving false impressions of lower mesospheric layers preferentially in winter, constitute a scenario consistent with our observations.


1975 ◽  
Vol 12 (2) ◽  
pp. 122-124 ◽  
Author(s):  
J. H. King ◽  
E. G. Stassinopoulos
Keyword(s):  

Author(s):  
Michael A. Xapsos ◽  
Craig A. Stauffer ◽  
Thomas M. Jordan ◽  
James H. Adams ◽  
William F. Dietrich

1966 ◽  
Vol 71 (13) ◽  
pp. 3289-3296 ◽  
Author(s):  
C. Y. Fan ◽  
J. E. Lamport ◽  
J. A. Simpson ◽  
D. R. Smith

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