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Estimation of Reconnection Rate From Soft X‐Ray Emission at the Earth's Dayside Magnetopause

Geophysical Research Letters, Volume 52, Issue 12, 28 June 2025.
Abstract We propose an approach to estimating the reconnection rate by utilizing soft X‐rays emitted during the solar wind charge exchange (SWCX) process at the Earth's magnetopause. Employing a high‐resolution global magnetohydrodynamic (MHD) simulation model of the magnetosphere, we investigated the SWCX emission around the magnetopause during a ...
Ryota Momose, Yosuke Matsumoto, Yoshizumi Miyoshi +2 more
wiley +1 more source

Solar Flare Phenomena [PDF]

Nature, 1964
Solar Flares By Henry J. Smith and Elske van Panhuys Smith. Pp. xii + 322. (New York: The Macmillan Company; London: Collier-Macmillan, 1963.) 100s.
openaire +2 more sources

Measurements on a shock wave generated by a solar flare [PDF]

, 1983
Richard Woo, J. W. Armstrong
openalex +3 more sources

6. Flare-Associated Phenomena in the Solar Corona [PDF]

, 1960
Walter Orr Roberts
openalex +1 more source

Uncovering the heterogeneity of a solar flare mechanism with mixture models

Frontiers in Astronomy and Space Sciences
The physics of solar flares occurring on the Sun is highly complex and far from fully understood. However, observations show that solar eruptions are associated with the intense kilogauss fields of active regions, where free energies are stored with ...
Bach Viet Do +4 more
doaj +1 more source

The 1859 space weather event revisited: limits of extreme activity

Journal of Space Weather and Space Climate, 2013
The solar flare on 1 September 1859 and its associated geomagnetic storm remain the standard for an extreme solar-terrestrial event. The most recent estimates of the flare soft X-ray (SXR) peak intensity and Dst magnetic storm index for this event are ...
Cliver Edward W., Dietrich William F.
doaj +1 more source

The isotopic composition of solar flare accelerated neon [PDF]