倒转
发表于 2025-3-28 15:46:42
Three-Dimensional Solar Modulation of Cosmic Rays and Anomalous Components in the Inner Heliospheretures in the solar wind and magnetic field; e) the surface of symmetry of the modulation in 1994–95 was offset about 10. south of the heliographic equator; f) the intensity of electrons and of low energy (< ~100 MeV) protons showed essentially no dependence on heliographic latitude.
Obedient
发表于 2025-3-28 22:28:39
Cosmic-Ray Modulation in the Heliospheree energy spectra of anomalous cosmic rays as a function of heliocentric distance..From solar minimum to solar maximum the long term modulation is principally a combination of two solar related phenomena, the cumulative effect of long-lived global merged interaction regions (GMIRs) and gradient and c
心神不宁
发表于 2025-3-29 00:34:12
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NAV
发表于 2025-3-29 05:18:27
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讨厌
发表于 2025-3-29 09:13:27
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Suppository
发表于 2025-3-29 15:22:07
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听写
发表于 2025-3-29 17:59:46
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Contracture
发表于 2025-3-29 23:04:49
https://doi.org/10.1007/978-3-319-94367-1e energy spectra of anomalous cosmic rays as a function of heliocentric distance..From solar minimum to solar maximum the long term modulation is principally a combination of two solar related phenomena, the cumulative effect of long-lived global merged interaction regions (GMIRs) and gradient and c
产生
发表于 2025-3-30 01:43:07
Human Resource Development and Work Analysiso mid-latitudes; the polar regions of the heliosphere are dominated by uniform fast solar wind streams and large amplitude, long wavelength, mostly transverse magnetic fluctuations. Coronal Mass Ejections (CMEs) introduce transient variability into the large scale heliospheric structure and may domi
Alopecia-Areata
发表于 2025-3-30 05:24:50
National Occupational Standardsthe magnetic field and solar wind particles and largely controls the dynamical processes. During 1983 and 1994, corotating streams and corotating interaction regions were observed at 1 AU. Merged interaction regions were observed at ≈15 AU in 1983, but not at ≈45 AU during 1994. This result suggests