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Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon In cooperation with: J. F. Fennell, M. Klida, K. Kudela, V. N. Lutsenko, J. Niehof, J. S. Pickett, J. Roeder, C. T. Russell, G. L. Siscoe, W. N. Spjeldvik, and K. Trattner

Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

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Page 1: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Cusp Radiation Source: A Challenge for Theory and Simulation

Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker,Forrest S. Mozer, and Robert B. Sheldon

In cooperation with:J. F. Fennell, M. Klida, K. Kudela, V. N. Lutsenko, J. Niehof, J. S. Pickett, J. Roeder, C. T. Russell,

G. L. Siscoe, W. N. Spjeldvik, and K. Trattner

Page 2: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Theory and simulation predict:

• Cusp is a precipitation region for particles;

• A positive IMF By would move the dayside northern cusp into post-noon;

• A negative IMF By would move the dayside northern cusp into pre-noon (e.g., Cowley et al., JGR, 96, 5557, 1991).

Page 3: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Cusp Diamagnetic Cavities (CDC): |B|

CDC at 9:30 MLT

(pre-noon)

with turbulence.

Cusp energetic Particle (CEP)

Page 4: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Cusp

CDC at 14-23 UT on 5/13/99 with a size of ~ 6 Re.

Page 5: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Solar wind conditions for the 5/13/99 CDC

Since By < 0,a CDC at pre-noon

was expected.

By < 0

Page 6: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Other CDC observations under different solar wind conditions:

1. Normal solar wind speed, vsw = 450 km/s

2. Fast solar wind stream, vsw = 900 km/s

3. Slow solar wind flow, vsw = 380 km/s (two examples presented)

Page 7: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

1. Normal solar wind speed, vsw=450 km/s

4/22/99

Page 8: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

(Fritz et al., JGR, 108, A1, 1028, 2003)

Pre-noon

Post-noon

Page 9: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

By>0, <Dst>=1.6 nT, CDC at pre-noon; unexpected

By>0

CDC at10:30 MLT

Page 10: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

2. Fast solar wind stream, vsw=900 km/s

6/28/99

Page 11: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Cusp energetic He++

Cusp energetic O+

Page 12: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

By>0, <Dst>=14.7 nT, CDC at 7MLT; unexpected

CDC

+ +

Page 13: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

3a. Slow solar wind flow, vsw=380 km/s4/25/99

Page 14: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

POLAR,4/25/99

Page 15: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

By>0, <Dst>=5.5 nT, CDC at pre-noon; unexpected

By>0

CDC at10:20 MLT

Page 16: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

3b. Slow solar wind flow, vsw=380 km/s

15 UT

19 UT

15 UT

19 UT

Page 17: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

By>0, <Dst>=-82 nT, CDC at 8:30 MLT; unexpected

By>0

CDC

10/30/78

ISEE-1

ISEE-3

IMF

Page 18: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Energetic Charged Particles in CDC

CEP electron

CEP proton

CDC

Page 19: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon
Page 20: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

CEP Energy Spectrum

Page 21: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

CEP vs. Outer Radiation Belt ParticlesProton phase space density

Page 22: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

He++ & O+ phase space densities: Cusp Radiation Source

Page 23: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

CEP and Fields

1. CEP flux increase with E-field increase and B-field Decrease.

2. Emax = 50 mV/m

Page 24: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Blow up cusp E-field near peak fluctuation

Showing some polarizationWaves at different Frequencies.

Page 25: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Left-hand polarization

Page 26: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Left-hand polarization

Page 27: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon
Page 28: Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon

Summary• CDC is a large radiation region, and CEP is a new

radiation source.

• Under different solar wind and geomagnetic conditions, CDCs have been observed at pre-noon in the northern hemisphere when IMF By >0 (duskward).

• These observations are unexpected by the existing models and MHD simulations and provide a new challenge for the current theory and simulations.

• Cusp ions can be energized by both resonant and stochastic acceleration mechanisms.