Results 231 to 240 of about 35,714 (290)

The Need for Near-Earth Multi-Spacecraft Heliospheric Measurements and an Explorer Mission to Investigate Interplanetary Structures and Transients in the Near-Earth Heliosphere. [PDF]

Space Sci Rev
Lugaz N, Lee CO, Al-Haddad N, Lillis RJ, Jian LK, Curtis DW, Galvin AB, Whittlesey PL, Rahmati A, Zesta E, Moldwin M, Summerlin EJ, Larson DE, Courtade S, French R, Hunter R, Covitti F, Cosgrove D, Prall JD, Allen RC, Zhuang B, Winslow RM, Scolini C, Lynch BJ, Filwett RJ, Palmerio E, Farrugia CJ, Smith CW, Möstl C, Weiler E, Janvier M, Regnault F, Livi R, Nieves-Chinchilla T.   +33 more
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Exploring the Potential Observations Between Geomagnetic Activity and Cardiovascular Events: A Scoping Review. [PDF]

Cureus
Belenko J, Cancel G, Mayrovitz HN.
europepmc   +1 more source

A Holistic Approach to the SMILE Mission and SMILE Public Engagement. [PDF]

Space Sci Rev
Carter JA, Sembay S, Nitti S, Walach MT, Milan S, Soobiah Y, Oksavik K, Forsyth C, Taylor MGGT.   +8 more
europepmc   +1 more source

Chaotic, rational and irrational oscillations of nonlinear waves in the Earth's magnetosheath featuring bi-regularized κ -distributed electrons. [PDF]

Sci Rep
Sarkar J, Saha A.
europepmc   +1 more source

Irreversibility and Energy Transfer at Non-MHD Scales in a Magnetospheric Current Disruption Event. [PDF]

Entropy (Basel)
Consolini G, De Michelis P.
europepmc   +1 more source

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Interplanetary Magnetic Fields

Science, 1962
Preliminary analysis of Mariner II magnetometer data indicates a persistent interplanetary field varying between a least 2 and 10 gamma (1γ = 10 -5 gauss). The interplanetary field appears to lie mainly in the ecliptic plane, although there is a substantial, fluctuating, transverse component.
Coleman, P. J., Jr., Davis, Leverett, Jr., Smith, E. J., Sonett, C. P.   +3 more
openaire   +3 more sources

Interplanetary magnetic fields

Reviews of Geophysics, 1979
Within the past four years, significant scientific progress has been possible as a result of improvements in observations of the interplanetary field. First, the range of radial distances over which observations are available has been greatly extended; measurements have been made as near the Sun as 0.3 AU and as far away as 8.5 AU. Second, the range of
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Interplanetary magnetic field and magnetospheric substorms

Planetary and Space Science, 1977
The interplanetary magnetic field (IMF) changes and the associated responses of the magnetosphere on November 1, 1972, are examined. IMF Bz changes consisted of a sudden southward turning, a slow northward turning, and a subsequent steady northward sense. Magnetospheric substorms occurred throughout this period.
S.-I. Akasofu, R.P. Lepping
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Counterelectrojet and interplanetary magnetic field

Journal of Geophysical Research: Space Physics, 1978
About a dozen counterelectrojet events both in the afternoon and in the morning hours were compared with interplanetary magnetic field data. It was noticed that in three to four cases there was an association between counterelectrojets and an excursion of Bz from southward to northward.
openaire   +1 more source