Storm time evolution of the outer radiation belt: Transport and losses

By A. Y. Ukhorskiy, Brian J. Anderson, P. Brandt, N. Tsyganenko. 2006

157 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/9ba08de57178f8e6999e87af4861069c8dbb2977

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

1. Wen Li
2. R. Thorne
3. Nigel P. Meredith
4. Jacob Bortnik
5. R. Horne
6. Y. Shprits
7. Binbin Ni
8. S. Glauert

Citations in the corpus

• Radiation Belt Environment model: Application to space weather nowcasting (2008, methodology): “Using a test particle approach, Ukhorskiy et al. [2006] simulated the evolution of outer belt electrons during the magnetic storm of 7 September 2002.”
• Global distributions of suprathermal electrons observed on THEMIS and potential mechanisms for access into the plasmasphere (2010, background): “…possibly due to pitch angle scattering by chorus waves and electrostatic Electron Cyclotron Harmonic (ECH) waves [e.g., Horne et al., 2003; Ni, et al., 2008; Su et al., 2009; Thorne et al., 2010] and magnetopause shadowing [e.g., Li et al., 1997; Desorgher et al., 2000; Ukhorskiy et al., 2006].”
• Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) (2013, background): “This effect can explain rapid depletion of electron fluxes over a broad region of the outer electron belt during storm main phase (e.g., Ukhorskiy et al. 2006; Turner et al. 2012).”
• Space Weather Effects in the Earth’s Radiation Belts (2018, background): “…(Gkioulidou et al. 2014), thereby diamagnetically expanding electron drift orbits to a point where magnetopause shadowing (West et al. 1972) can have a greater effect on the core population (Ukhorskiy et al. 2006) and lead to dramatic dropout features in the observations (Shprits et al. 2006).”
• Use of POES SEM-2 observations to examine radiation belt dynamics and energetic electron precipitation into the atmosphere (2010, background): “…fraction of all of the particles lost are precipitated into the atmosphere [Lorentzen et al., 2001; Horne, 2002; Friedel et al., 2002; Clilverd et al., 2006], although storm‐time nonadiabatic magnetic field changes also lead to losses through magnetopause shadowing [e.g., Ukhorskiy et al., 2006].”
• On the storm‐time evolution of relativistic electron phase space density in Earth's outer radiation belt (2013, background): “This happens due to sudden inward motion of the magnetopause in response to increased solar wind dynamic pressure and is known as magnetopause shadowing [e.g., Ukhorskiy et al., 2006].”
• Explaining sudden losses of outer radiation belt electrons during geomagnetic storms (2012, background): “Losses to the magnetopause can occur through magnetopause ‘shadowing&rsquo”