10/08/2012 05:00:00 UTC - Revision history

Davidwebb: /* References */

2017-03-02T23:43:08Z

‎References

2017-01-20T20:28:38Z

‎References

2017-01-20T20:27:50Z

‎References

2017-01-20T20:27:08Z

‎Comment Section

2014-09-29T20:23:04Z

2014-09-29T20:22:32Z

2014-06-23T17:43:08Z

‎Comment Section

2014-06-23T17:41:39Z

‎Comment Section

2014-06-19T19:06:35Z

‎Video Data

2014-06-19T19:01:19Z

‎Image Data

← Older revision		Revision as of 23:43, 2 March 2017
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	*Thorne, R. M., et al. (2013), Rapid acceleration of relativistic radiation belt electrons by magnetospheric chorus, Nature, 504, 411–414, doi:10.1038/nature12889.		*Thorne, R. M., et al. (2013), Rapid acceleration of relativistic radiation belt electrons by magnetospheric chorus, Nature, 504, 411–414, doi:10.1038/nature12889.
	*Kurita, S., Y. Miyoshi, J. B. Blake, G. D. Reeves, and C. A. Kletzing (2016), Relativistic electron microbursts and variations in trapped MeV electron fluxes during the 8–9 October 2012 storm: SAMPEX and Van Allen Probes observations, Geophys. Res. Lett., 43, 3017–3025, doi:10.1002/2016GL068260.		*Kurita, S., Y. Miyoshi, J. B. Blake, G. D. Reeves, and C. A. Kletzing (2016), Relativistic electron microbursts and variations in trapped MeV electron fluxes during the 8–9 October 2012 storm: SAMPEX and Van Allen Probes observations, Geophys. Res. Lett., 43, 3017–3025, doi:10.1002/2016GL068260.
		+	*Webb, D., N. Nitta: 2017, Study on Understanding Problem Forecasts of ISEST Campaign Flare-CME Events, Solar Phys., submitted.
		+	*Nitta, N. V., T. Mulligan: 2017, Earth-Affecting Coronal Mass Ejections Without Obvious Low Coronal Signatures, Solar Phys., submitted.
		+	*Marubashi, K., K.-S. Cho, H. Ishibashi: 2017, Interplanetary Magnetic Flux Rope as Agent Connecting Solar Eruptions and Geomagnetic Activities, Solar Phys., submitted.

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 =References=
-- Reeves, G. D., et al. (2013), Electron acceleration in the heart of the Van Allen radiation belts, Science, 341(6149), 991–994, doi:10.1126/science.1237743.
+*Reeves, G. D., et al. (2013), Electron acceleration in the heart of the Van Allen radiation belts, Science, 341(6149), 991–994, doi:10.1126/science.1237743.
-- Thorne, R. M., et al. (2013), Rapid acceleration of relativistic radiation belt electrons by magnetospheric chorus, Nature, 504, 411–414, doi:10.1038/nature12889.
+*Thorne, R. M., et al. (2013), Rapid acceleration of relativistic radiation belt electrons by magnetospheric chorus, Nature, 504, 411–414, doi:10.1038/nature12889.
-- Kurita, S., Y. Miyoshi, J. B. Blake, G. D. Reeves, and C. A. Kletzing (2016), Relativistic electron microbursts and variations in trapped MeV electron fluxes during the 8–9 October 2012 storm: SAMPEX and Van Allen Probes observations, Geophys. Res. Lett., 43, 3017–3025, doi:10.1002/2016GL068260.
+*Kurita, S., Y. Miyoshi, J. B. Blake, G. D. Reeves, and C. A. Kletzing (2016), Relativistic electron microbursts and variations in trapped MeV electron fluxes during the 8–9 October 2012 storm: SAMPEX and Van Allen Probes observations, Geophys. Res. Lett., 43, 3017–3025, doi:10.1002/2016GL068260.

← Older revision		Revision as of 20:27, 20 January 2017
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	=References=		=References=
		+	- Reeves, G. D., et al. (2013), Electron acceleration in the heart of the Van Allen radiation belts, Science, 341(6149), 991–994, doi:10.1126/science.1237743.
		+	- Thorne, R. M., et al. (2013), Rapid acceleration of relativistic radiation belt electrons by magnetospheric chorus, Nature, 504, 411–414, doi:10.1038/nature12889.
		+	- Kurita, S., Y. Miyoshi, J. B. Blake, G. D. Reeves, and C. A. Kletzing (2016), Relativistic electron microbursts and variations in trapped MeV electron fluxes during the 8–9 October 2012 storm: SAMPEX and Van Allen Probes observations, Geophys. Res. Lett., 43, 3017–3025, doi:10.1002/2016GL068260.

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 **If the eruption started at 14 UT, Oct. 14, it took a long time (10 hrs) for the eruption to reach the COR1 FOV. It indicates that the eruption has a long-lasting low-speed low-acceleration phase
-At Earth it produced a small storm, Dst=-105. Electron acceleration in the radiation belt has been studied by Reeves, G.D. et al (2013). [Added by D. Webb]
+At Earth it produced a small storm, Dst=-105. Electron acceleration in the radiation belt has been measured by the Van Allen Probes and studied by Reeves, et al (2013), Thorne et al. (2013, and Kurita et al. (2016). studied by Reeves, G.D. et al (2013). [Added by D. Webb]
 =Image Data=

@@ Line 18: / Line 18: @@
 **If the eruption started at 14 UT, Oct. 14, it took a long time (10 hrs) for the eruption to reach the COR1 FOV. It indicates that the eruption has a long-lasting low-speed low-acceleration phase
-At Earth a smaller storm, Dst=-105. Electron acceleration in the radiation belt has been studied by Reeves, G.D. et al (2013). [Added by D. Webb]
+At Earth it produced a small storm, Dst=-105. Electron acceleration in the radiation belt has been studied by Reeves, G.D. et al (2013). [Added by D. Webb]
 =Image Data=

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 * M. Temmer: clear on-disk signatures - movie from SDO - are visible. It is a "silent" CME, hard to catch for space weather forecasters, but not a "stealth" in sense of no solar surface signatures at all.
 http://sdowww.lmsal.com/sdomedia/SunInTime/2012/10/04/daily_211-193-171.mov [October 4, 15UT, central south]
-I out some images showing clear coronal restructuring and some discussion points under> http://www.uni-graz.at/~temmerma/download/varsiti/
 *C. Moestl: looking at the whole October 4 SDO movie, there are also two other minor eruptions which I find very hard to distinguish from the 15 UT one (1. 7 UT, slightly west of disk center; 2. 0930 UT, south-east quadrant)
 * timing - evolution from SDO FoV to coronagraph - is an issue and needs to be looked at in detail

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 =Video Data=
 [http://solar.gmu.edu/wiki/upload/phess4/aia3041005.avi AIA 304 Running Difference Movie] <br />
 [http://solar.gmu.edu/wiki/upload/phess4/aia1931005.avi AIA 195 Running Difference Movie] <br />