Presentation is loading. Please wait.

Presentation is loading. Please wait.

EVE and RHESSI H. S. Hudson Space Sciences Laboratory, University of California, Berkeley, USA RHESSI, April 5, 2011.

Similar presentations


Presentation on theme: "EVE and RHESSI H. S. Hudson Space Sciences Laboratory, University of California, Berkeley, USA RHESSI, April 5, 2011."— Presentation transcript:

1 EVE and RHESSI H. S. Hudson Space Sciences Laboratory, University of California, Berkeley, USA RHESSI, April 5, 2011

2 Outline RHESSI, April 5, 2011 0) SOL2010-06-12T00:57 as seen by HMI 1)What is EVE? 2) How good is EVE? 3)What can we learn from EVE and RHESSI?

3 SOL2010-06-12T00:57 (HMI) RHESSI, April 5, 2011 Martinez-Oliveros et al. 2011

4 The ESP component of EVE RHESSI, April 5, 2011

5 The ESP component of EVE RHESSI, April 5, 2011

6 The ESP component of EVE RHESSI, April 5, 2011

7 The ESP component of EVE RHESSI, April 5, 2011

8 ESP fluxes for SOL2010-06-12 RHESSI, April 5, 2011

9 The MEGS component of EVE RHESSI, April 5, 2011

10 The MEGS component of EVE RHESSI, April 5, 2011

11 EVE 304A for SOL2010-06-12 RHESSI, April 5, 2011 RHESSI 100 keV EVE 30.4 nm

12 EVE 304A for SOL2010-06-12 RHESSI, April 5, 2011

13 EVE 304 Doppler sensitivity RHESSI, April 5, 2011 1 pm = 1 km/s?

14 EVE 304A for SOL2010-06-12 RHESSI, April 5, 2011

15 EVE 304A for SOL2010-06-12 RHESSI, April 5, 2011

16 He 304 Charge Exchange RHESSI, April 5, 2011 Peter et al. 1991

17 SOL2010-06-12 Charge Exchange RHESSI, April 5, 2011

18 SOL2010-06-12 Charge Exchange RHESSI, April 5, 2011

19 SOL2011-02-15 Fe XXIV RHESSI, April 5, 2011

20 SOL2011-02-15 Fe XXIV RHESSI, April 5, 2011

21 What can we learn from EVE and RHESSI? UV/EUV energy distribution for WLF/HXR Charge-exchange observations of  particles at.01-1 MeV/nucleon Transition-region explanation of 511 keV line width Flare dynamics, with big doses of imaging and modeling RHESSI, April 5, 2011

22 Electrodynamic mapping of the solar interior to the corona RHESSI, April 5, 2011 Collisionality drops precipitously Hydrogen ionizes Plasma beta plummets Structurally important radiation escapes Vertical currents threading the photosphere carry the non-potential energy Recall debate between Parker and Melrose in ApJ (1996)


Download ppt "EVE and RHESSI H. S. Hudson Space Sciences Laboratory, University of California, Berkeley, USA RHESSI, April 5, 2011."

Similar presentations


Ads by Google